Math::Prime::Util - Utilities related to prime numbers, including fast sieves and factoring
Version 0.31
# Normally you would just import the functions you are using. # Nothing is exported by default. List the functions, or use :all. use Math::Prime::Util ':all'; # Get a big array reference of many primes my $aref = primes( 100_000_000 ); # All the primes between 5k and 10k inclusive my $aref = primes( 5_000, 10_000 ); # If you want them in an array instead my @primes = @{primes( 500 )}; # You can do something for every prime in a range. Twin primes to 10k: forprimes { say if is_prime($_+2) } 10000; # For non-bigints, is_prime and is_prob_prime will always be 0 or 2. # They return 0 (composite), 2 (prime), or 1 (probably prime) say "$n is prime" if is_prime($n); say "$n is ", (qw(composite maybe_prime? prime))[is_prob_prime($n)]; # Strong pseudoprime test with multiple bases, using Miller-Rabin say "$n is a prime or 2/7/61-psp" if is_strong_pseudoprime($n, 2, 7, 61); # Standard and strong Lucas-Selfridge, and extra strong Lucas tests say "$n is a prime or lpsp" if is_lucas_pseudoprime($n); say "$n is a prime or slpsp" if is_strong_lucas_pseudoprime($n); say "$n is a prime or eslpsp" if is_extra_strong_lucas_pseudoprime($n); # step to the next prime (returns 0 if not using bigints and we'd overflow) $n = next_prime($n); # step back (returns 0 if given input less than 2) $n = prev_prime($n); # Return Pi(n) -- the number of primes E<lt>= n. $primepi = prime_count( 1_000_000 ); $primepi = prime_count( 10**14, 10**14+1000 ); # also does ranges # Quickly return an approximation to Pi(n) my $approx_number_of_primes = prime_count_approx( 10**17 ); # Lower and upper bounds. lower <= Pi(n) <= upper for all n die unless prime_count_lower($n) <= prime_count($n); die unless prime_count_upper($n) >= prime_count($n); # Return p_n, the nth prime say "The ten thousandth prime is ", nth_prime(10_000); # Return a quick approximation to the nth prime say "The one trillionth prime is ~ ", nth_prime_approx(10**12); # Lower and upper bounds. lower <= nth_prime(n) <= upper for all n die unless nth_prime_lower($n) <= nth_prime($n); die unless nth_prime_upper($n) >= nth_prime($n); # Get the prime factors of a number @prime_factors = factor( $n ); # Get all factors @divisors = all_factors( $n ); # Euler phi (Euler's totient) on a large number use bigint; say euler_phi( 801294088771394680000412 ); say jordan_totient(5, 1234); # Jordan's totient # Moebius function used to calculate Mertens $sum += moebius($_) for (1..200); say "Mertens(200) = $sum"; # Mertens function directly (more efficient for large values) say mertens(10_000_000); # Exponential of Mangoldt function say "lamba(49) = ", log(exp_mangoldt(49)); # divisor sum $sigma = divisor_sum( $n ); $sigma2 = divisor_sum( $n, sub { $_[0]*$_[0] } ); # primorial n#, primorial p(n)#, and lcm say "The product of primes below 47 is ", primorial(47); say "The product of the first 47 primes is ", pn_primorial(47); say "lcm(1..1000) is ", consecutive_integer_lcm(1000); # Ei, li, and Riemann R functions my $ei = ExponentialIntegral($x); # $x a real: $x != 0 my $li = LogarithmicIntegral($x); # $x a real: $x >= 0 my $R = RiemannR($x) # $x a real: $x > 0 my $Zeta = RiemannZeta($x) # $x a real: $x >= 0 # Precalculate a sieve, possibly speeding up later work. prime_precalc( 1_000_000_000 ); # Free any memory used by the module. prime_memfree; # Alternate way to free. When this leaves scope, memory is freed. my $mf = Math::Prime::Util::MemFree->new; # Random primes my $small_prime = random_prime(1000); # random prime <= limit my $rand_prime = random_prime(100, 10000); # random prime within a range my $rand_prime = random_ndigit_prime(6); # random 6-digit prime my $rand_prime = random_nbit_prime(128); # random 128-bit prime my $rand_prime = random_strong_prime(256); # random 256-bit strong prime my $rand_prime = random_maurer_prime(256); # random 256-bit provable prime
A set of utilities related to prime numbers. These include multiple sieving methods, is_prime, prime_count, nth_prime, approximations and bounds for the prime_count and nth prime, next_prime and prev_prime, factoring utilities, and more.
The default sieving and factoring are intended to be (and currently are) the fastest on CPAN, including Math::Prime::XS, Math::Prime::FastSieve, Math::Factor::XS, Math::Prime::TiedArray, Math::Big::Factors, Math::Factoring, and Math::Primality (when the GMP module is available). For numbers in the 10-20 digit range, it is often orders of magnitude faster. Typically it is faster than Math::Pari for 64-bit operations.
All operations support both Perl UV's (32-bit or 64-bit) and bignums. It requires no external software for big number support, as there are Perl implementations included that solely use Math::BigInt and Math::BigFloat. If you want high performance with big numbers (larger than Perl's UV size), you should install Math::Prime::Util::GMP. This will be a recurring theme throughout this documentation -- while all bignum operations are supported in pure Perl, most methods will be much slower than the C+GMP alternative.
The module is thread-safe and allows concurrency between Perl threads while still sharing a prime cache. It is not itself multi-threaded. See the Limitations section if you are using Win32 and threads in your program.
Two scripts are also included and installed by default:
--help
to see all the options.factor
program. It supports bigint and expression inputs.By default all functions support bignums. With a few exceptions, the module will not turn on bignum support for you -- you will need to use bigint
, use bignum
, or pass in a Math::BigInt or Math::BigFloat object as your input. The functions take some care to perform all bignum operations using the same class as was passed in, allowing the module to work properly with Calc, FastCalc, GMP, Pari, etc. You should try to install Math::Prime::Util::GMP if you plan to use bigints with this module, as it will make it run much faster.
Some of the functions, including:
factor is_pseudoprime is_strong_pseudoprime nth_prime moebius mertens euler_phi exp_mangoldt chebyshev_theta chebyshev_psi is_prime is_prob_prime next_prime prev_prime
work very fast (under 1 microsecond) on small inputs, but the wrappers for input validation and bigint support take more time than the function itself. Using the flag '-bigint', e.g.:
use Math::Prime::Util qw(-bigint);
will turn off bigint support for those functions. Those functions will then go directly to the XS versions, which will speed up very small inputs a lot. This is useful if you're using the functions in a loop, but since the difference is less than a millisecond, it's really not important in general. The last four functions have shortcuts by default so will only skip validation.
If you are using bigints, here are some performance suggestions:
use bigint try => 'GMP,Pari'
in your script, or on the command line -Mbigint=lib,GMP
. Large modular exponentiation is much faster using the GMP or Pari backends, as are the math and approximation functions when called with very large inputs.print "$n is prime" if is_prime($n);
Returns 2 if the number is prime, 0 if not. For numbers larger than 2^64
it will return 0 for composite and 1 for probably prime, using an extra-strong BPSW test. If Math::Prime::Util::GMP is installed, some additional primality tests are also performed on large inputs, and a quick attempt is made to perform a primality proof, so it will return 2 for many other inputs.
Also see the "is_prob_prime" function, which will never do additional tests, and the "is_provable_prime" function which will construct a proof that the input is number prime and returns 2 for almost all primes (at the expense of speed).
For native precision numbers (anything smaller than 2^64
, all three functions are identical and use a deterministic set of tests (selected Miller-Rabin bases or BPSW). For larger inputs both "is_prob_prime" and "is_prime" return probable prime results using the extra-strong Baillie-PSW test, which has had no counterexample found since it was published in 1980.
Returns all the primes between the lower and upper limits (inclusive), with a lower limit of 2
if none is given.
An array reference is returned (with large lists this is much faster and uses less memory than returning an array directly).
my $aref1 = primes( 1_000_000 ); my $aref2 = primes( 1_000_000_000_000, 1_000_000_001_000 ); my @primes = @{ primes( 500 ) }; print "$_\n" for (@{primes( 20, 100 )});
Sieving will be done if required. The algorithm used will depend on the range and whether a sieve result already exists. Possibilities include trial division (for ranges with only one expected prime), a Sieve of Eratosthenes using wheel factorization, or a segmented sieve.
$n = next_prime($n);
Returns the next prime greater than the input number. If the input is not a bigint, then 0 is returned if the next prime is larger than a native integer type (the last representable primes being 4,294,967,291
in 32-bit Perl and 18,446,744,073,709,551,557
in 64-bit).
$n = prev_prime($n);
Returns the prime preceding the input number (i.e. the largest prime that is strictly less than the input). 0 is returned if the input is 2
or lower.
forprimes { say } 100,200; # print primes from 100-200 $sum=0; forprimes { $sum += $_ } 100000; # sum primes to 100k forprimes { say if is_prime($_+2) } 10000; # print twin primes to 10k
Given a block and either an end count or a start and end pair, calls the block for each prime in the range. Compared to getting a big array of primes and iterating through it, this is more memory efficient and perhaps more convenient. There is no way to exit the loop early, so the iterator may be more appropriate for those uses.
my $it = prime_iterator; $sum += $it->() for 1..100000;
Returns a closure-style iterator. The start value defaults to the first prime (2) but an initial value may be given as an argument, which will result in the first value returned being the next prime greater than or equal to the argument. For example, this:
my $it = prime_iterator(200); say $it->(); say $it->();
will return 211 followed by 223, as those are the next primes >= 200. On each call, the iterator returns the current value and increments to the next prime.
In general, "forprimes" will be more efficient, but the generic iterator has more flexibility (e.g. exiting a loop early, or passing the iterator around).
my $primepi = prime_count( 1_000 ); my $pirange = prime_count( 1_000, 10_000 );
Returns the Prime Count function Pi(n)
, also called primepi
in some math packages. When given two arguments, it returns the inclusive count of primes between the ranges (e.g. (13,17)
returns 2, 14,17
and 13,16
return 1, and 14,16
returns 0).
The current implementation decides based on the ranges whether to use a segmented sieve with a fast bit count, or Lehmer's algorithm. The former is preferred for small sizes as well as small ranges. The latter is much faster for large ranges.
The segmented sieve is very memory efficient and is quite fast even with large base values. Its complexity is approximately O(sqrt(a) + (b-a))
, where the first term is typically negligible below ~ 10^11
. Memory use is proportional only to sqrt(a)
, with total memory use under 1MB for any base under 10^14
.
Lehmer's method has complexity approximately O(b^0.7) + O(a^0.7)
. It does use more memory however. A calculation of Pi(10^14)
completes in under 1 minute, Pi(10^15)
in under 5 minutes, and Pi(10^16)
in under 20 minutes, however using about 500MB of peak memory for the last. In contrast, even primesieve using 12 cores would take over a week on this same computer to determine Pi(10^16)
.
Also see the function "prime_count_approx" which gives a very good approximation to the prime count, and "prime_count_lower" and "prime_count_upper" which give tight bounds to the actual prime count. These functions return quickly for any input, including bigints.
my $lower_limit = prime_count_lower($n); my $upper_limit = prime_count_upper($n); # $lower_limit <= prime_count(n) <= $upper_limit
Returns an upper or lower bound on the number of primes below the input number. These are analytical routines, so will take a fixed amount of time and no memory. The actual prime_count
will always be equal to or between these numbers.
A common place these would be used is sizing an array to hold the first $n
primes. It may be desirable to use a bit more memory than is necessary, to avoid calling prime_count
.
These routines use verified tight limits below a range at least 2^35
, and use the Dusart (2010) bounds of
x/logx * (1 + 1/logx + 2.000/log^2x) <= Pi(x) x/logx * (1 + 1/logx + 2.334/log^2x) >= Pi(x)
above that range. These bounds do not assume the Riemann Hypothesis. If the configuration option assume_rh
has been set (it is off by default), then the Schoenfeld (1976) bounds are used for large values.
print "there are about ", prime_count_approx( 10 ** 18 ), " primes below one quintillion.\n";
Returns an approximation to the prime_count
function, without having to generate any primes. For values under 10^36
this uses the Riemann R function, which is quite accurate: an error of less than 0.0005%
is typical for input values over 2^32
, and decreases as the input gets larger. If Math::MPFR is installed, the Riemann R function is used for all values, and will be very fast. If not, then values of 10^36
and larger will use the approximation li(x) - li(sqrt(x))/2
. While not as accurate as the Riemann R function, it still should have error less than 0.00000000000000001%
.
A slightly faster but much less accurate answer can be obtained by averaging the upper and lower bounds.
say "The ten thousandth prime is ", nth_prime(10_000);
Returns the prime that lies in index n
in the array of prime numbers. Put another way, this returns the smallest p
such that Pi(p) >= n
.
For relatively small inputs (below 2 million or so), this does a sieve over a range containing the nth prime, then counts up to the number. This is fairly efficient in time and memory. For larger values, a binary search is performed between the Dusart 2010 bounds using Riemann's R function, then Lehmer's fast prime counting method is used to calculate the count up to that point, then sieving is done in the typically small error zone.
While this method is hundreds of times faster than generating primes, and doesn't involve big tables of precomputed values, it still can take a fair amount of time and space for large inputs. Calculating the 10^11th
prime takes a bit under 2 seconds, the 10^12th
prime takes 10 seconds, and the 10^13th
prime (323780508946331) takes 1 minute. Think about whether a bound or approximation would be acceptable, as they can be computed analytically.
If the bigint or bignum module is not in use, this will generate an overflow exception if the number requested would result in a prime that cannot fit in a native type. If bigints are in use, then the calculation will proceed, though it will be exceedingly slow. A later version of Math::Prime::Util::GMP may include this functionality which would help for 32-bit machines.
my $lower_limit = nth_prime_lower($n); my $upper_limit = nth_prime_upper($n); # $lower_limit <= nth_prime(n) <= $upper_limit
Returns an analytical upper or lower bound on the Nth prime. These are very fast as they do not need to sieve or search through primes or tables. An exact answer is returned for tiny values of n
. The lower limit uses the Dusart 2010 bound for all n
, while the upper bound uses one of the two Dusart 2010 bounds for n >= 178974
, a Dusart 1999 bound for n >= 39017
, and a simple bound of n * (logn + 0.6 * loglogn)
for small n
.
say "The one trillionth prime is ~ ", nth_prime_approx(10**12);
Returns an approximation to the nth_prime
function, without having to generate any primes. Uses the Cipolla 1902 approximation with two polynomials, plus a correction for small values to reduce the error.
Takes a positive number n
and a base a
as input, and returns 1 if n
is a probable prime to base a
. This is the simple Fermat primality test. Removing primes, given base 2 this produces the sequence OEIS A001567.
my $maybe_prime = is_strong_pseudoprime($n, 2); my $probably_prime = is_strong_pseudoprime($n, 2, 3, 5, 7, 11, 13, 17);
Takes a positive number as input and one or more bases. The bases must be greater than 1
. Returns 1 if the input is a strong probable prime to all of the bases, and 0 if not.
If 0 is returned, then the number really is a composite. If 1 is returned, then it is either a prime or a strong pseudoprime to all the given bases. Given enough distinct bases, the chances become very, very strong that the number is actually prime.
This is usually used in combination with other tests to make either stronger tests (e.g. the strong BPSW test) or deterministic results for numbers less than some verified limit (e.g. it has long been known that no more than three selected bases are required to give correct primality test results for any 32-bit number). Given the small chances of passing multiple bases, there are some math packages that just use multiple MR tests for primality testing.
Even inputs other than 2 will always return 0 (composite). While the algorithm does run with even input, most sources define it only on odd input. Returning composite for all non-2 even input makes the function match most other implementations including Math::Primality's is_strong_pseudoprime
function.
An alias for is_strong_pseudoprime
. This name is deprecated.
Takes a positive number as input, and returns 1 if the input is a standard Lucas probable prime using the Selfridge method of choosing D, P, and Q (some sources call this a Lucas-Selfridge pseudoprime). Removing primes, this produces the sequence OEIS A217120.
Takes a positive number as input, and returns 1 if the input is a strong Lucas probable prime using the Selfridge method of choosing D, P, and Q (some sources call this a strong Lucas-Selfridge pseudoprime). This is one half of the BPSW primality test (the Miller-Rabin strong pseudoprime test with base 2 being the other half). Removing primes, this produces the sequence OEIS A217255.
Takes a positive number as input, and returns 1 if the input passes the extra strong Lucas test (as defined in Grantham 2000). This test has more stringent conditions than the strong Lucas test, and produces about 60% fewer pseudoprimes. Performance is typically 20-30% faster than the strong Lucas test.
The parameters are selected using the Baillie-OEIS method method: increment P
from 3
until jacobi(D,n) = -1
. Removing primes, this produces the sequence OEIS A217719.
This is similar to the "is_extra_strong_lucas_pseudoprime" function, but does not calculate U
, so is a little faster, but also weaker. With the current implementations, there is little reason to prefer this unless trying to reproduce specific results. The extra-strong implementation has been optimized to use similar features, removing most of the performance advantage.
An optional second argument (an integer between 1 and 256) indicates the increment amount for P
parameter selection. The default value of 1 yields the parameter selection described in "is_extra_strong_lucas_pseudoprime", creating a pseudoprime sequence which is a superset of the latter's pseudoprime sequence OEIS A217719. A value of 2 yields the method used by Pari.
Because the U = 0
condition is ignored, this produces about 5% more pseudoprimes than the extra-strong Lucas test. However this is still only 66% of the number produced by the strong Lucas-Selfridge test. No BPSW counterexamples have been found with any of the Lucas tests described.
Takes a positive number as input, and returns 1 if the input passes the minimal lambda+2 test (see Underwood 2012 "Quadratic Compositeness Tests"), where (L+2)^(n-1) = 5 + 2x mod (n, L^2 - Lx + 1)
. The computational cost for this is between the cost of 2 and 3 strong pseudoprime tests. There are no known counterexamples, but this is not a well studied test.
my $prob_prime = is_prob_prime($n); # Returns 0 (composite), 2 (prime), or 1 (probably prime)
Takes a positive number as input and returns back either 0 (composite), 2 (definitely prime), or 1 (probably prime).
For 64-bit input (native or bignum), this uses either a deterministic set of Miller-Rabin tests (1, 2, or 3 tests) or a strong BPSW test consisting of a single base-2 strong probable prime test followed by a strong Lucas test. This has been verified with Jan Feitsma's 2-PSP database to produce no false results for 64-bit inputs. Hence the result will always be 0 (composite) or 2 (prime).
For inputs larger than 2^64
, an extra-strong Baillie-PSW primality test is performed (also called BPSW or BSW). This is a probabilistic test, so only 0 (composite) and 1 (probably prime) are returned. There is a possibility that composites may be returned marked prime, but since the test was published in 1980, not a single BPSW pseudoprime has been found, so it is extremely likely to be prime. While we believe (Pomerance 1984) that an infinite number of counterexamples exist, there is a weak conjecture (Martin) that none exist under 10000 digits.
say "$n is definitely prime" if is_provable_prime($n) == 2;
Takes a positive number as input and returns back either 0 (composite), 2 (definitely prime), or 1 (probably prime). This gives it the same return values as "is_prime" and "is_prob_prime". Note that numbers below 2^64 are considered proven by the deterministic set of Miller-Rabin bases or the BPSW test. Both of these have been tested for all small (64-bit) composites and do not return false positives.
Using the Math::Prime::Util::GMP module is highly recommended for doing primality proofs, as it is much, much faster. The pure Perl code is just not fast for this type of operation, nor does it have the best algorithms. It should suffice for proofs of up to 40 digit primes, while the latest MPU::GMP works for primes of hundreds of digits (thousands with an optional larger polynomial set).
The pure Perl implementation uses theorem 5 of BLS75 (Brillhart, Lehmer, and Selfridge's 1975 paper), an improvement on the Pocklington-Lehmer test. This requires n-1
to be factored to (n/2)^(1/3))
. This is often fast, but as n
gets larger, it takes exponentially longer to find factors.
Math::Prime::Util::GMP implements both the BLS75 theorem 5 test as well as ECPP (elliptic curve primality proving). It will typically try a quick n-1
proof before using ECPP. Certificates are available with either method. This results in proofs of 200-digit primes in under 1 second on average, and many hundreds of digits are possible. This makes it significantly faster than Pari 2.1.7's is_prime(n,1)
which is the default for Math::Pari.
my @cert = prime_certificate($n); say verify_prime(@cert) ? "proven prime" : "not prime";
Given a positive integer n
as input, returns a primality certificate as a multi-line string. If we could not prove n
prime, an empty string is returned (n
may or may not be composite). This may be examined or given to "verify_prime" for verification. The latter function contains the description of the format.
Given a positive integer as input, returns a two element array containing the result of "is_provable_prime": 0 definitely composite 1 probably prime 2 definitely prime and a primality certificate like "prime_certificate". The certificate will be an empty string if the first element is not 2.
my $cert = prime_certificate($n); say verify_prime($cert) ? "proven prime" : "not prime";
Given a primality certificate, returns either 0 (not verified) or 1 (verified). Most computations are done using pure Perl with Math::BigInt, so you probably want to install and use Math::BigInt::GMP, and ECPP certificates will be faster with Math::Prime::Util::GMP for its elliptic curve computations.
If the certificate is malformed, the routine will carp a warning in addition to returning 0. If the verbose
option is set (see "prime_set_config") then if the validation fails, the reason for the failure is printed in addition to returning 0. If the verbose
option is set to 2 or higher, then a message indicating success and the certificate type is also printed.
A certificate may have arbitrary text before the beginning (the primality routines from this module will not have any extra text, but this way verbose output from the prover can be safely stored in a certificate). The certificate begins with the line:
[MPU - Primality Certificate]
All lines in the certificate beginning with #
are treated as comments and ignored, as are blank lines. A version number may follow, such as:
Version 1.0
For all inputs, base 10 is the default, but at any point this may be changed with a line like:
Base 16
where allowed bases are 10, 16, and 62. This module will only use base 10, so its routines will not output Base commands.
Next, we look for (using "100003" as an example):
Proof for: N 100003
where the text Proof for:
indicates we will read an N
value. Skipping comments and blank lines, the next line should be "N " followed by the number.
After this, we read one or more blocks. Each block is a proof of the form:
If Q is prime, then N is prime.
Some of the blocks have more than one Q value associated with them, but most only have one. Each block has its own set of conditions which must be verified, and this can be done completely self-contained. That is, each block is independent of the other blocks and may be processed in any order. To be a complete proof, each block must successfully verify. The block types and their conditions are shown below.
Finally, when all blocks have been read and verified, we must ensure we can construct a proof tree from the set of blocks. The root of the tree is the initial N
, and for each node (block), all Q
values must either have a block using that value as its N
or Q
must be less than 2^64
and pass BPSW.
Some other certificate formats (e.g. Primo) use an ordered chain, where the first block must be for the initial N
, a single Q
is given which is the implied N
for the next block, and so on. This simplifies validation implementation somewhat, and removes some redundant information from the certificate, but has no obvious way to add proof types such as Lucas or the various BLS75 theorems that use multiple factors. I decided that the most general solution was to have the certificate contain the set in any order, and let the verifier do the work of constructing the tree.
The blocks begin with the text "Type ..." where ... is the type. One or more values follow. The defined types are:
Small
Type Small N 5791
N must be less than 2^64 and be prime (use BPSW or deterministic M-R).
BLS3
Type BLS3 N 2297612322987260054928384863 Q 16501461106821092981 A 5
A simple n-1 style proof using BLS75 theorem 3. This block verifies if: a Q is odd b Q > 2 c Q divides N-1 . Let M = (N-1)/Q d MQ+1 = N e M > 0 f 2Q+1 > sqrt(N) g A^((N-1)/2) mod N = N-1 h A^(M/2) mod N != N-1
Pocklington
Type Pocklington N 2297612322987260054928384863 Q 16501461106821092981 A 5
A simple n-1 style proof using generalized Pocklington. This is more restrictive than BLS3 and much more than BLS5. This is Primo's type 1, and this module does not currently generate these blocks. This block verifies if: a Q divides N-1 . Let M = (N-1)/Q b M > 0 c M < Q d MQ+1 = N e A > 1 f A^(N-1) mod N = 1 g gcd(A^M - 1, N) = 1
BLS15
Type BLS15 N 8087094497428743437627091507362881 Q 175806402118016161687545467551367 LP 1 LQ 22
A simple n+1 style proof using BLS75 theorem 15. This block verifies if: a Q is odd b Q > 2 c Q divides N+1 . Let M = (N+1)/Q d MQ-1 = N e M > 0 f 2Q-1 > sqrt(N) . Let D = LP*LP - 4*LQ g D != 0 h Jacobi(D,N) = -1 . Note: V_{k} indicates the Lucas V sequence with LP,LQ i V_{m/2} mod N != 0 j V_{(N+1)/2} mod N == 0
BLS5
Type BLS5 N 8087094497428743437627091507362881 Q[1] 98277749 Q[2] 3631 A[0] 11 ----
A more sophisticated n-1 proof using BLS theorem 5. This requires N-1 to be factored only to (N/2)^(1/3)
. While this looks much more complicated, it really isn't much more work. The biggest drawback is just that we have multiple Q values to chain rather than a single one. This block verifies if:
a N > 2 b N is odd . Note: the block terminates on the first line starting with a C<->. . Let Q[0] = 2 . Let A[i] = 2 if Q[i] exists and A[i] does not c For each i (0 .. maxi): c1 Q[i] > 1 c2 Q[i] < N-1 c3 A[i] > 1 c4 A[i] < N c5 Q[i] divides N-1 . Let F = N-1 divided by each Q[i] as many times as evenly possible . Let R = (N-1)/F d F is even e gcd(F, R) = 1 . Let s = integer part of R / 2F . Let f = fractional part of R / 2F . Let P = (F+1) * (2*F*F + (r-1)*F + 1) f n < P g s = 0 OR r^2-8s is not a perfect square h For each i (0 .. maxi): h1 A[i]^(N-1) mod N = 1 h2 gcd(A[i]^((N-1)/Q[i])-1, N) = 1
ECPP
Type ECPP N 175806402118016161687545467551367 A 96642115784172626892568853507766 B 111378324928567743759166231879523 M 175806402118016177622955224562171 Q 2297612322987260054928384863 X 3273750212 Y 82061726986387565872737368000504
An elliptic curve primality block, typically generated with an Atkin/Morain ECPP implementation, but this should be adequate for anything using the Atkin-Goldwasser-Kilian-Morain style certificates. Some basic elliptic curve math is needed for these. This block verifies if:
. Note: A and B are allowed to be negative, with -1 not uncommon. . Let A = A % N . Let B = B % N a N > 0 b gcd(N, 6) = 1 c gcd(4*A^3 + 27*B^2, N) = 1 d Y^2 mod N = X^3 + A*X + B mod N e M >= N - 2*sqrt(N) + 1 f M <= N + 2*sqrt(N) + 1 g Q > (N^(1/4)+1)^2 h Q < N i M != Q j Q divides M . Note: EC(A,B,N,X,Y) is the point (X,Y) on Y^2 = X^3 + A*X + B, mod N . All values work in affine coordinates, but in theory other . representations work just as well. . Let POINT1 = (M/Q) * EC(A,B,N,X,Y) . Let POINT2 = M * EC(A,B,N,X,Y) [ = Q * POINT1 ] k POINT1 is not the identity l POINT2 is the identity
say "$n is definitely prime" if is_aks_prime($n);
Takes a positive number as input, and returns 1 if the input passes the Agrawal-Kayal-Saxena (AKS) primality test. This is a deterministic unconditional primality test which runs in polynomial time for general input.
This function is only included for completeness and as an example. The Perl implementation is fast compared to the only other Perl implementation available (in Math::Primality), and the implementation in Math::Prime::Util::GMP compares favorably to others in the literature. However AKS in general is far too slow to be of practical use. R.P. Brent, 2010: "AKS is not a practical algorithm. ECPP is much faster."
my($U, $V, $Qk) = lucas_sequence($n, $P, $Q, $k)
Computes U_k
, V_k
, and Q_k
for the Lucas sequence defined by P
,Q
, modulo n
. The modular Lucas sequence is used in a number of primality tests and proofs.
The following conditions must hold: - D = P*P - 4*Q != 0
- P > 0
- P < n
- Q < n
- k >= 0
- n >= 2
say "$n is square free" if moebius($n) != 0; $sum += moebius($_) for (1..200); say "Mertens(200) = $sum";
Returns μ(n), the Möbius function (also called the Moebius, Mobius, or MoebiusMu function) for a non-negative integer input. This function is 1 if n = 1
, 0 if n
is not square free (i.e. n
has a repeated factor), and -1^t
if n
is a product of t
distinct primes. This is an important function in prime number theory. Like SAGE, we define moebius(0) = 0
for convenience.
If called with two arguments, they define a range low
to high
, and the function returns an array with the value of the Möbius function for every n from low to high inclusive. Large values of high will result in a lot of memory use. The algorithm used is Deléglise and Rivat (1996) algorithm 4.1, which is a segmented version of Lioen and van de Lune (1994) algorithm 3.2.
say "Mertens(10M) = ", mertens(10_000_000); # = 1037
Returns M(n), the Mertens function for a non-negative integer input. This function is defined as sum(moebius(1..n))
, but calculated more efficiently for large inputs. For example, computing Mertens(100M) takes:
time approx mem 0.4s 0.1MB mertens(100_000_000) 74.8s 7000MB List::Util::sum(moebius(1,100_000_000)) 88.5s 0MB $sum += moebius($_) for 1..100_000_000 [-nobigint] 181.8s 0MB $sum += moebius($_) for 1..100_000_000
The summation of individual terms via factoring is quite expensive in time, though uses O(1) space. This function will generate the equivalent output via a sieving method, which will use some more memory, but be much faster. The current method is a simple n^1/2
version of Deléglise and Rivat (1996), which involves calculating all moebius values to n^1/2
, which in turn will require prime sieving to n^1/4
.
Various algorithms exist for this, using differing quantities of μ(n). The simplest way is to efficiently sum all n
values. Benito and Varona (2008) show a clever and simple method that only requires n/3
values. Deléglise and Rivat (1996) describe a segmented method using only n^1/3
values. The current implementation does a simple non-segmented n^1/2
version of their method. Kuznetsov (2011) gives an alternate method that he indicates is even faster. Lastly, one of the advanced prime count algorithms could be theoretically used to create a faster solution.
say "The Euler totient of $n is ", euler_phi($n);
Returns φ(n), the Euler totient function (also called Euler's phi or phi function) for an integer value. This is an arithmetic function that counts the number of positive integers less than or equal to n
that are relatively prime to n
. Given the definition used, euler_phi
will return 0 for all n < 1
. This follows the logic used by SAGE. Mathematic/WolframAlpha also returns 0 for input 0, but returns euler_phi(-n)
for n < 0
.
If called with two arguments, they define a range low
to high
, and the function returns an array with the totient of every n from low to high inclusive. Large values of high will result in a lot of memory use.
say "Jordan's totient J_$k($n) is ", jordan_totient($k, $n);
Returns Jordan's totient function for a given integer value. Jordan's totient is a generalization of Euler's totient, where jordan_totient(1,$n) == euler_totient($n)
This counts the number of k-tuples less than or equal to n that form a coprime tuple with n. As with euler_phi
, 0 is returned for all n < 1
. This function can be used to generate some other useful functions, such as the Dedikind psi function, where psi(n) = J(2,n) / J(1,n)
.
say "exp(lambda($_)) = ", exp_mangoldt($_) for 1 .. 100;
Returns EXP(Λ(n)), the exponential of the Mangoldt function (also known as von Mangoldt's function) for an integer value. It is equal to log p if n is prime or a power of a prime, and 0 otherwise. We return the exponential so all results are integers. Hence the return value for exp_mangoldt
is:
p if n = p^m for some prime p and integer m >= 1 1 otherwise.
say chebyshev_theta(10000);
Returns θ(n), the first Chebyshev function for a non-negative integer input. This is the sum of the logarithm of each prime where p <= n
. An alternate computation is as the logarithm of n primorial. Hence these functions:
use List::Util qw/sum/; use Math::BigFloat; sub c1a { 0+sum( map { log($_) } @{primes(shift)} ) } sub c1b { Math::BigFloat->new(primorial(shift))->blog }
yield similar results, albeit slower and using more memory.
say chebyshev_psi(10000);
Returns ψ(n), the second Chebyshev function for a non-negative integer input. This is the sum of the logarithm of each prime where p^k <= n
for an integer k. An alternate computation is as the summatory Mangoldt function. Another alternate computation is as the logarithm of LCM(1,2,...,n). Hence these functions:
use List::Util qw/sum/; use Math::BigFloat; sub c2a { 0+sum( map { log(exp_mangoldt($_)) } 1 .. shift ) } sub c2b { Math::BigFloat->new(consecutive_integer_lcm(shift))->blog }
yield similar results, albeit slower and using more memory.
say "Sum of divisors of $n:", divisor_sum( $n );
This function takes a positive integer as input and returns the sum of all the divisors of the input, including 1 and itself. This is known as the sigma function (see Hardy and Wright section 16.7, or OEIS A000203).
The more general form takes a code reference as a second parameter, which is applied to each divisor before the summation. This allows computation of numerous functions such as OEIS A000005 [d(n), sigma_0(n), tau(n)]:
divisor_sum( $n, sub { 1 } );
OEIS A001157 [sigma_2(n)]:
divisor_sum( $n, sub { $_[0]*$_[0] } )
the general sigma_k (OEIS A00005, A000203, A001157, A001158, etc.):
divisor_sum( $n, sub { $_[0] ** $k } );
the 5th Jordan totient (OEIS A059378):
divisor_sum( $n, sub { my $d=shift; $d**5 * moebius($n/$d); } );
though in the last case we have a function "jordan_totient" to compute it more efficiently.
This function is useful for calculating things like aliquot sums, abundant numbers, perfect numbers, etc.
The summation is done as a bigint if the input was a bigint object. You may need to ensure the result of the subroutine does not overflow a native int.
$prim = primorial(11); # 11# = 2*3*5*7*11 = 2310
Returns the primorial n#
of the positive integer input, defined as the product of the prime numbers less than or equal to n
. This is the OEIS series A034386: primorial numbers second definition.
primorial(0) == 1 primorial($n) == pn_primorial( prime_count($n) )
The result will be a Math::BigInt object if it is larger than the native bit size.
Be careful about which version (primorial
or pn_primorial
) matches the definition you want to use. Not all sources agree on the terminology, though they should give a clear definition of which of the two versions they mean. OEIS, Wikipedia, and Mathworld are all consistent, and these functions should match that terminology. This function should return the same result as the mpz_primorial_ui
function added in GMP 5.1.
$prim = pn_primorial(5); # p_5# = 2*3*5*7*11 = 2310
Returns the primorial number p_n#
of the positive integer input, defined as the product of the first n
prime numbers (compare to the factorial, which is the product of the first n
natural numbers). This is the OEIS series A002110: primorial numbers first definition.
pn_primorial(0) == 1 pn_primorial($n) == primorial( nth_prime($n) )
The result will be a Math::BigInt object if it is larger than the native bit size.
$lcm = consecutive_integer_lcm($n);
Given an unsigned integer argument, returns the least common multiple of all integers from 1 to n
. This can be done by manipulation of the primes up to n
, resulting in much faster and memory-friendly results than using a factorial.
my $small_prime = random_prime(1000); # random prime <= limit my $rand_prime = random_prime(100, 10000); # random prime within a range
Returns a pseudo-randomly selected prime that will be greater than or equal to the lower limit and less than or equal to the upper limit. If no lower limit is given, 2 is implied. Returns undef if no primes exist within the range.
The goal is to return a uniform distribution of the primes in the range, meaning for each prime in the range, the chances are equally likely that it will be seen. This is removes from consideration such algorithms as PRIMEINC
, which although efficient, gives very non-random output.
For small numbers, a random index selection is done, which gives ideal uniformity and is very efficient with small inputs. For ranges larger than this ~16-bit threshold but within the native bit size, a Monte Carlo method is used (multiple calls to rand
may be made if necessary). This also gives ideal uniformity and can be very fast for reasonably sized ranges. For even larger numbers, we partition the range, choose a random partition, then select a random prime from the partition. This gives some loss of uniformity but results in many fewer bits of randomness being consumed as well as being much faster.
If an irand
function has been set via "prime_set_config", it will be used to construct any ranged random numbers needed. The function should return a uniformly random 32-bit integer, which is how the irand functions exported by Math::Random::Secure, Math::Random::MT, Math::Random::ISAAC and most other modules behave.
If no irand
function was set, then Bytes::Random::Secure is used with a non-blocking seed. This will create good quality random numbers, so there should be little reason to change unless one is generating long-term keys, where using the blocking random source may be preferred.
Examples of various ways to set your own irand function:
# Math::Random::Secure. Uses ISAAC and strong seed methods. use Math::Random::Secure; prime_set_config(irand => \&Math::Random::Secure::irand); # Bytes::Random::Secure (OO interface with full control of options): use Bytes::Random::Secure (); BEGIN { my $rng = Bytes::Random::Secure->new( Bits => 512 ); sub irand { return $rng->irand; } } prime_set_config(irand => \&irand); # Crypt::Random. Uses Pari and /dev/random. Very slow. use Crypt::Random qw/makerandom/; prime_set_config(irand => sub { makerandom(Size=>32, Uniform=>1); }); # Mersenne Twister. Very fast, decent RNG, auto seeding. use Math::Random::MT::Auto; prime_set_config(irand=>sub {Math::Random::MT::Auto::irand() & 0xFFFFFFFF});
say "My 4-digit prime number is: ", random_ndigit_prime(4);
Selects a random n-digit prime, where the input is an integer number of digits between 1 and the maximum native type (10 for 32-bit, 20 for 64-bit, 10000 if bigint is active). One of the primes within that range (e.g. 1000 - 9999 for 4-digits) will be uniformly selected using the irand
function as described above.
If the number of digits is greater than or equal to the maximum native type, then the result will be returned as a BigInt. However, if the -nobigint
tag was used, then numbers larger than the threshold will be flagged as an error, and numbers on the threshold will be restricted to native numbers. For better performance with large bit sizes, install Math::Prime::Util::GMP.
my $bigprime = random_nbit_prime(512);
Selects a random n-bit prime, where the input is an integer number of bits between 2 and the maximum representable bits (32, 64, or 100000 for native 32-bit, native 64-bit, and bigint respectively). A prime with the nth bit set will be uniformly selected, with randomness supplied via calls to the irand
function as described above.
Since this uses the random_prime function, all uniformity properties of that function apply to this. The n-bit range is partitioned into nearly equal segments less than 2^32
, a segment is randomly selected, then the trivial Monte Carlo algorithm is used to select a prime from within the segment. This gives a reasonably uniform distribution, doesn't use excessive random source, and can be very fast.
The result will be a BigInt if the number of bits is greater than the native bit size. For better performance with large bit sizes, install Math::Prime::Util::GMP.
my $bigprime = random_strong_prime(512);
Constructs an n-bit strong prime using Gordon's algorithm. We consider a strong prime p to be one where
Using a strong prime in cryptography guards against easy factoring with algorithms like Pollard's Rho. Rivest and Silverman (1999) present a case that using strong primes is unnecessary, and most modern cryptographic systems agree. First, the smoothness does not affect more modern factoring methods such as ECM. Second, modern factoring methods like GNFS are far faster than either method so make the point moot. Third, due to key size growth and advances in factoring and attacks, for practical purposes, using large random primes offer security equivalent to strong primes.
Similar to "random_nbit_prime", the result will be a BigInt if the number of bits is greater than the native bit size. For better performance with large bit sizes, install Math::Prime::Util::GMP.
my $bigprime = random_maurer_prime(512);
Construct an n-bit provable prime, using the FastPrime algorithm of Ueli Maurer (1995). This is the same algorithm used by Crypt::Primes. Similar to "random_nbit_prime", the result will be a BigInt if the number of bits is greater than the native bit size. For better performance with large bit sizes, install Math::Prime::Util::GMP.
The differences between this function and that in Crypt::Primes are described in the "SEE ALSO" section.
Internally this additionally runs the BPSW probable prime test on every partial result, and constructs a primality certificate for the final result, which is verified. These add additional checks that the resulting value has been properly constructed.
my($n, $cert) = random_maurer_prime_with_cert(512)
As with "random_maurer_prime", but returns a two-element array containing the n-bit provable prime along with a primality certificate. The certificate is the same as produced by "prime_certificate" or "is_provable_prime_with_cert", and can be parsed by "verify_prime" or any other software that can parse MPU primality certificates. The proof construction consists of a single chain of BLS3
types.
prime_precalc( 1_000_000_000 );
Let the module prepare for fast operation up to a specific number. It is not necessary to call this, but it gives you more control over when memory is allocated and gives faster results for multiple calls in some cases. In the current implementation this will calculate a sieve for all numbers up to the specified number.
prime_memfree;
Frees any extra memory the module may have allocated. Like with prime_precalc
, it is not necessary to call this, but if you're done making calls, or want things cleanup up, you can use this. The object method might be a better choice for complicated uses.
my $mf = Math::Prime::Util::MemFree->new; # perform operations. When $mf goes out of scope, memory will be recovered.
This is a more robust way of making sure any cached memory is freed, as it will be handled by the last MemFree
object leaving scope. This means if your routines were inside an eval that died, things will still get cleaned up. If you call another function that uses a MemFree object, the cache will stay in place because you still have an object.
my $cached_up_to = prime_get_config->{'precalc_to'};
Returns a reference to a hash of the current settings. The hash is copy of the configuration, so changing it has no effect. The settings include:
precalc_to primes up to this number are calculated maxbits the maximum number of bits for native operations xs 0 or 1, indicating the XS code is available gmp 0 or 1, indicating GMP code is available maxparam the largest value for most functions, without bigint maxdigits the max digits in a number, without bigint maxprime the largest representable prime, without bigint maxprimeidx the index of maxprime, without bigint assume_rh whether to assume the Riemann hypothesis (default 0)
prime_set_config( assume_rh => 1 );
Allows setting of some parameters. Currently the only parameters are:
xs Allows turning off the XS code, forcing the Pure Perl code to be used. Set to 0 to disable XS, set to 1 to re-enable. You probably will never want to do this. gmp Allows turning off the use of L<Math::Prime::Util::GMP>, which means using Pure Perl code for big numbers. Set to 0 to disable GMP, set to 1 to re-enable. You probably will never want to do this. assume_rh Allows functions to assume the Riemann hypothesis is true if set to 1. This defaults to 0. Currently this setting only impacts prime count lower and upper bounds, but could later be applied to other areas such as primality testing. A later version may also have a way to indicate whether no RH, RH, GRH, or ERH is to be assumed. irand Takes a code ref to an irand function returning a uniform number between 0 and 2**32-1. This will be used for all random number generation in the module.
my @factors = factor(3_369_738_766_071_892_021); # returns (204518747,16476429743)
Produces the prime factors of a positive number input, in numerical order. The special cases of n = 0
and n = 1
will return n
, which guarantees multiplying the factors together will always result in the input value, though those are the only cases where the returned factors are not prime.
The current algorithm for non-bigints is a sequence of small trial division, a few rounds of Pollard's Rho, SQUFOF, Pollard's p-1, Hart's OLF, a long run of Pollard's Rho, and finally trial division if anything survives. This process is repeated for each non-prime factor. In practice, it is very rare to require more than the first Rho + SQUFOF to find a factor, and I have not seen anything go to the last step.
Factoring bigints works with pure Perl, and can be very handy on 32-bit machines for numbers just over the 32-bit limit, but it can be very slow for "hard" numbers. Installing the Math::Prime::Util::GMP module will speed up bigint factoring a lot, and all future effort on large number factoring will be in that module. If you do not have that module for some reason, use the GMP or Pari version of bigint if possible (e.g. use bigint try => 'GMP,Pari'
), which will run 2-3x faster (though still 100x slower than the real GMP code).
my @divisors = all_factors(30); # returns (2, 3, 5, 6, 10, 15)
Produces all the divisors of a positive number input. 1 and the input number are excluded (which implies that an empty list is returned for any prime number input). The divisors are a power set of multiplications of the prime factors, returned as a uniqued sorted list.
my @factors = trial_factor($n);
Produces the prime factors of a positive number input. The factors will be in numerical order. The special cases of n = 0
and n = 1
will return n
, while with all other inputs the factors are guaranteed to be prime. For large inputs this will be very slow.
my @factors = fermat_factor($n);
Produces factors, not necessarily prime, of the positive number input. The particular algorithm is Knuth's algorithm C. For small inputs this will be very fast, but it slows down quite rapidly as the number of digits increases. It is very fast for inputs with a factor close to the midpoint (e.g. a semiprime p*q where p and q are the same number of digits).
my @factors = holf_factor($n);
Produces factors, not necessarily prime, of the positive number input. An optional number of rounds can be given as a second parameter. It is possible the function will be unable to find a factor, in which case a single element, the input, is returned. This uses Hart's One Line Factorization with no premultiplier. It is an interesting alternative to Fermat's algorithm, and there are some inputs it can rapidly factor. In the long run it has the same advantages and disadvantages as Fermat's method.
my @factors = squfof_factor($n); my @factors = rsqufof_factor($n); # racing multiplier version
Produces factors, not necessarily prime, of the positive number input. An optional number of rounds can be given as a second parameter. It is possible the function will be unable to find a factor, in which case a single element, the input, is returned. This function typically runs very fast.
my @factors = prho_factor($n); my @factors = pbrent_factor($n); # Use a very small number of rounds my @factors = prho_factor($n, 1000);
Produces factors, not necessarily prime, of the positive number input. An optional number of rounds can be given as a second parameter. These attempt to find a single factor using Pollard's Rho algorithm, either the original version or Brent's modified version. These are more specialized algorithms usually used for pre-factoring very large inputs, as they are very fast at finding small factors.
my @factors = pminus1_factor($n); my @factors = pminus1_factor($n, 1_000); # set B1 smoothness my @factors = pminus1_factor($n, 1_000, 50_000); # set B1 and B2
Produces factors, not necessarily prime, of the positive number input. This is Pollard's p-1
method, using two stages with default smoothness settings of 1_000_000 for B1, and 10 * B1
for B2. This method can rapidly find a factor p
of n
where p-1
is smooth (it has no large factors).
my @factors = pplus1_factor($n); my @factors = pplus1_factor($n, 1_000); # set B1 smoothness
Produces factors, not necessarily prime, of the positive number input. This is Williams' p+1
method, using one stage and two predefined initial points.
my $Ei = ExponentialIntegral($x);
Given a non-zero floating point input x
, this returns the real-valued exponential integral of x
, defined as the integral of e^t/t dt
from -infinity
to x
.
If the bignum module has been loaded, all inputs will be treated as if they were Math::BigFloat objects.
For non-BigInt/BigFloat objects, the result should be accurate to at least 14 digits.
For BigInt / BigFloat objects, we first check to see if Math::MPFR is available. If so, then it is used since it is very fast and has high accuracy. Accuracy when using MPFR will be equal to the accuracy()
value of the input (or the default BigFloat accuracy, which is 40 by default).
MPFR is used for positive inputs only. If Math::MPFR is not available or the input is negative, then other methods are used: continued fractions (x < -1
), rational Chebyshev approximation ( -1 < x < 0
), a convergent series (small positive x
), or an asymptotic divergent series (large positive x
). Accuracy should be at least 14 digits.
my $li = LogarithmicIntegral($x)
Given a positive floating point input, returns the floating point logarithmic integral of x
, defined as the integral of dt/ln t
from 0
to x
. If given a negative input, the function will croak. The function returns 0 at x = 0
, and -infinity
at x = 1
.
This is often known as li(x)
. A related function is the offset logarithmic integral, sometimes known as Li(x)
which avoids the singularity at 1. It may be defined as Li(x) = li(x) - li(2)
. Crandall and Pomerance use the term li0
for this function, and define li(x) = Li0(x) - li0(2)
. Due to this terminology confusion, it is important to check which exact definition is being used.
If the bignum module has been loaded, all inputs will be treated as if they were Math::BigFloat objects.
For non-BigInt/BigFloat objects, the result should be accurate to at least 14 digits.
For BigInt / BigFloat objects, we first check to see if Math::MPFR is available. If so, then it is used, as it will return results much faster and can be more accurate. Accuracy when using MPFR will be equal to the accuracy()
value of the input (or the default BigFloat accuracy, which is 40 by default).
MPFR is used for inputs greater than 1 only. If Math::MPFR is not installed or the input is less than 1, results will be calculated as Ei(ln x)
.
my $z = RiemannZeta($s);
Given a floating point input s
where s >= 0
, returns the floating point value of ζ(s)-1, where ζ(s) is the Riemann zeta function. One is subtracted to ensure maximum precision for large values of s
. The zeta function is the sum from k=1 to infinity of 1 / k^s
. This function only uses real arguments, so is basically the Euler Zeta function.
If the bignum module has been loaded, all inputs will be treated as if they were Math::BigFloat objects.
For non-BigInt/BigFloat objects, the result should be accurate to at least 14 digits. The XS code uses a rational Chebyshev approximation between 0.5 and 5, and a series for other values. The PP code uses an identical series for all values.
For BigInt / BigFloat objects, we first check to see if the Math::MPFR module is installed. If so, then it is used, as it will return results much faster and can be more accurate. Accuracy when using MPFR will be equal to the accuracy()
value of the input (or the default BigFloat accuracy, which is 40 by default).
If Math::MPFR is not installed, then results are calculated using either Borwein (1991) algorithm 2, or the basic series. Full input accuracy is attempted, but there are defects in Math::BigFloat with high accuracy computations that make this difficult. It is also very slow. I highly recommend installing Math::MPFR for BigFloat computations.
my $r = RiemannR($x);
Given a positive non-zero floating point input, returns the floating point value of Riemann's R function. Riemann's R function gives a very close approximation to the prime counting function.
If the bignum module has been loaded, all inputs will be treated as if they were Math::BigFloat objects.
For non-BigInt/BigFloat objects, the result should be accurate to at least 14 digits.
For BigInt / BigFloat objects, we first check to see if the Math::MPFR module is installed. If so, then it is used, as it will return results much faster and can be more accurate. Accuracy when using MPFR will be equal to the accuracy()
value of the input (or the default BigFloat accuracy, which is 40 by default). Accuracy without MPFR should be 35 digits.
Print strong pseudoprimes to base 17 up to 10M:
perl -MMath::Prime::Util=:all -E 'my $n=3; while($n <= 10000000) { print "$n " if is_strong_pseudoprime($n,$base) && !is_prime($n); $n+=2; } BEGIN {$|=1; $base=17}'
or, slightly faster, use forprimes and loop over the odds between primes:
# Runs about 5x faster than Pari using A001262's isStrongPsp function perl -MMath::Prime::Util=:all -E '$|=1; $base=17; my $prev = 1; forprimes { $prev += 2; while ($prev < $_) { print "$prev " if is_strong_pseudoprime($prev,$base); $prev += 2; } } 3,10000000'
Print some primes above 64-bit range:
perl -MMath::Prime::Util=:all -Mbigint -E 'my $start=100000000000000000000; say join "\n", @{primes($start,$start+1000)}' # Similar code using Pari: # perl -MMath::Pari=:int,PARI,nextprime -E 'my $start = PARI "100000000000000000000"; my $end = $start+1000; my $p=nextprime($start); while ($p <= $end) { say $p; $p = nextprime($p+1); }'
Examining the η3(x) function of Planat and Solé (2011):
sub nu3 { my $n = shift; my $phix = chebyshev_psi($n); my $nu3 = 0; foreach my $nu (1..3) { $nu3 += (moebius($nu)/$nu)*LogarithmicIntegral($phix**(1/$nu)); } return $nu3; } say prime_count(1000000); say prime_count_approx(1000000); say nu3(1000000);
Construct and use a Sophie-Germain prime iterator:
sub make_sophie_germain_iterator { my $p = shift || 2; my $it = prime_iterator($p); return sub { do { $p = $it->() } while !is_prime(2*$p+1); $p; }; } my $sgit = make_sophie_germain_iterator(); for (1 .. 10000) { print $sgit->(), "\n"; }
Project Euler, problem 3 (Largest prime factor):
use Math::Prime::Util qw/factor/; use bigint; # Only necessary for 32-bit machines. say "", (factor(600851475143))[-1]
Project Euler, problem 7 (10001st prime):
use Math::Prime::Util qw/nth_prime/; say nth_prime(10_001);
Project Euler, problem 10 (summation of primes):
use Math::Prime::Util qw/primes/; my $sum = 0; $sum += $_ for @{primes(2_000_000)}; say $sum;
Project Euler, problem 21 (Amicable numbers):
use Math::Prime::Util qw/divisor_sum/; sub dsum { my $n = shift; divisor_sum($n) - $n; } my $sum = 0; foreach my $a (1..10000) { my $b = dsum($a); $sum += $a + $b if $b > $a && dsum($b) == $a; } say $sum;
Project Euler, problem 41 (Pandigital prime), brute force command line:
perl -MMath::Prime::Util=:all -E 'my @p = grep { /1/&&/2/&&/3/&&/4/&&/5/&&/6/&&/7/} @{primes(1000000,9999999)}; say $p[-1];
Project Euler, problem 47 (Distinct primes factors):
use Math::Prime::Util qw/pn_primorial factor/; use List::MoreUtils qw/distinct/; sub nfactors { scalar distinct factor(shift); } my $n = pn_primorial(4); # Start with the first 4-factor number $n++ while (nfactors($n) != 4 || nfactors($n+1) != 4 || nfactors($n+2) != 4 || nfactors($n+3) != 4); say $n;
Project Euler, problem 69, stupid brute force solution (about 5 seconds):
use Math::Prime::Util qw/euler_phi/; my ($n, $max) = (0,0); do { my $ndivphi = $_ / euler_phi($_); ($n, $max) = ($_, $ndivphi) if $ndivphi > $max; } for 1..1000000; say "$n $max";
Here's the right way to do PE problem 69 (under 0.03s):
use Math::Prime::Util qw/pn_primorial/; my $n = 0; $n++ while pn_primorial($n+1) < 1000000; say pn_primorial($n);'
Project Euler, problem 187, stupid brute force solution, ~3 minutes:
use Math::Prime::Util qw/factor -nobigint/; my $nsemis = 0; do { my @f = factor($_); $nsemis++ if scalar @f == 2; } for 1 .. int(10**8)-1; say $nsemis;
Here's the best way for PE187. Under 30 milliseconds from the command line:
use Math::Prime::Util qw/primes prime_count -nobigint/; use List::Util qw/sum/; my $limit = shift || int(10**8); my @primes = @{primes(int(sqrt($limit)))}; say sum( map { prime_count(int(($limit-1)/$primes[$_-1])) - $_ + 1 } 1 .. scalar @primes );
I have not completed testing all the functions near the word size limit (e.g. 2^32
for 32-bit machines). Please report any problems you find.
Perl versions earlier than 5.8.0 have a rather broken 64-bit implementation, in that the values are accessed as doubles. Hence any value larger than ~ 2^49
will start losing bottom bits. This causes numerous functions to not work properly. The test suite will try to determine if your Perl is broken (this only applies to really old versions of Perl compiled for 64-bit when using numbers larger than ~ 2^49
). The best solution is updating to a more recent Perl.
The module is thread-safe and should allow good concurrency on all platforms that support Perl threads except Win32. With Win32, either don't use threads or make sure prime_precalc
is called before using primes
, prime_count
, or nth_prime
with large inputs. This is only an issue if you use non-Cygwin Win32 and call these routines from within Perl threads.
This section describes other CPAN modules available that have some feature overlap with this one. Also see the "REFERENCES" section. Please let me know if any of this information is inaccurate. Also note that just because a module doesn't match what I believe are the best set of features, doesn't mean it isn't perfect for someone else.
I will use SoE to indicate the Sieve of Eratosthenes, and MPU to denote this module (Math::Prime::Util). Some quick alternatives I can recommend if you don't want to use MPU:
Math::Prime::XS has is_prime
and primes
functionality. There is no bigint support. The is_prime
function uses well-written trial division, meaning it is very fast for small numbers, but terribly slow for large 64-bit numbers. With the latest release, MPU should be faster for all sizes. The prime sieve is an unoptimized non-segmented SoE which returns an array. It works well for 32-bit values, but speed and memory are problematic for larger values.
Math::Prime::FastSieve supports primes
, is_prime
, next_prime
, prev_prime
, prime_count
, and nth_prime
. The caveat is that all functions only work within the sieved range, so are limited to about 10^10
. It uses a fast SoE to generate the main sieve. The sieve is 2-3x slower than the base sieve for MPU, and is non-segmented so cannot be used for larger values. Since the functions work with the sieve, they are very fast. All this functionality is present in MPU as well, though not required.
Bit::Vector supports the primes
and prime_count
functionality in a somewhat similar way to Math::Prime::FastSieve. It is the slowest of all the XS sieves, and has the most memory use. It is, however, faster than the pure Perl code in MPU or elsewhere.
Crypt::Primes supports random_maurer_prime
functionality. MPU has more options for random primes (n-digit, n-bit, ranged, and strong) in addition to Maurer's algorithm. MPU does not have the critical bug RT81858. MPU should have a more uniform distribution as well as return a larger subset of primes (RT81871). MPU does not depend on Math::Pari though can run slow for bigints unless the Math::BigInt::GMP or Math::BigInt::Pari modules are installed. Having Math::Prime::Util::GMP installed also helps performance for MPU. Crypt::Primes is hardcoded to use Crypt::Random, while MPU uses Bytes::Random::Secure, and also allows plugging in a random function. This is more flexible, faster, has fewer dependencies, and uses a CSPRNG for security. What Crypt::Primes has that MPU does not is support for returning a generator.
Math::Factor::XS calculates prime factors and factors, which correspond to the "factor" and "all_factors" functions of MPU. These functions do not support bigints. Both are implemented with trial division, meaning they are very fast for really small values, but quickly become unusably slow (factoring 19 digit semiprimes is over 700 times slower). It has additional functions count_prime_factors
(possible in MPU using scalar factor($n)
) and matches
which has no direct equivalent.
Math::Big version 1.12 includes primes
functionality. The current code is only usable for very tiny inputs as it is incredibly slow and uses lots of memory. RT81986 has a patch to make it run much faster and use much less memory. Since it is in pure Perl it will still run quite slow compared to MPU.
Math::Big::Factors supports factorization using wheel factorization (smart trial division). It supports bigints. Unfortunately it is extremely slow on any input that isn't the product of just small factors. Even 7 digit inputs can take hundreds or thousands of times longer to factor than MPU or Math::Factor::XS. 19-digit semiprimes will take hours versus MPU's single milliseconds.
Math::Factoring is a placeholder module for bigint factoring. Version 0.02 only supports trial division (the Pollard-Rho method does not work).
Math::Prime::TiedArray allows random access to a tied primes array, almost identically to what MPU provides in Math::Prime::Util::PrimeArray. MPU has attempted to fix Math::Prime::TiedArray's shift bug (RT58151). MPU is typically much faster and will use less memory, but there are some cases where MP:TA is faster (MP:TA stores all entries up to the largest request, while MPU:PA stores only a window around the last request).
Math::Primality supports is_prime
, is_pseudoprime
, is_strong_pseudoprime
, is_strong_lucas_pseudoprime
, next_prime
, prev_prime
, prime_count
, and is_aks_prime
functionality. This is a great little module that implements primality functionality. It was the first module to support the BPSW and AKS tests. All inputs are processed using GMP, so it of course supports bigints. In fact, Math::Primality was made originally with bigints in mind, while MPU was originally targeted to native integers, but both have added better support for the other. The main differences are extra functionality (MPU has more functions) and performance. With native integer inputs, MPU is generally much faster, especially with "prime_count". For bigints, MPU is slower unless the Math::Prime::Util::GMP module is installed, in which case MPU is ~2x faster. Math::Primality also installs a primes.pl
program, but it has much less functionality than the one included with MPU.
Math::NumSeq is more a related module rather than one with direct functionality. It does however offer a way to get similar results such as primes, twin primes, Sophie-Germain primes, lucky primes, moebius, divisor count, factor count, Euler totient, primorials, etc. Math::NumSeq is mainly set up for accessing these values in order, rather than for arbitrary values, though some sequences support that. The primary advantage I see is the uniform access mechanism for a lot of sequences. For those methods that overlap, MPU is usually much faster. Importantly, most of the sequences in Math::NumSeq are limited to 32-bit indices.
Math::Pari supports a lot of features, with a great deal of overlap. In general, MPU will be faster for native 64-bit integers, while it's differs for bigints (Pari will always be faster if Math::Prime::Util::GMP is not installed; with it, it varies by function). Some of the highlights:
isprime
Similar to MPU's is_prob_prime or is_prime functions. MPU is deterministic for native integers, and uses a strong BPSW test for bigints (with a quick primality proof tried as well). The default version of Pari used by Math::Pari (2.1.7) uses 10 random M-R bases, which is a probable prime test usually considered much weaker than the BPSW test used by MPU and newer versions of Pari (though better than a fixed set of bases). Calling as isprime($n,1)
performs a Pocklington-Lehmer n-1
proof. This is comparable in performance to MPU:GMP's n-1
proof implementation, and is reasonably fast for about 70 digits, but much slower than ECPP.
If Math::Pari is compiled with version 2.3.5 of Pari (this is not easy to do on many platforms), then the algorithms are completely different. The isprime
function now acts like "is_provable_prime" -- an APRCL proof is performed, which is quite efficient though requires using a larger stack for numbers of 300+ digits. It is somewhat comparable in speed to MPU:GMP's ECPP proof method, but without a certificate. Using the ispseudoprime
function will perform a BPSW test similar to "is_prob_prime".
primepi
Only available with version 2.3 of Pari. Similar to MPU's prime_count function in API, but uses a naive counting algorithm with its precalculated primes, so is not of practical use. Incidently, Pari 2.6 (not usable from Perl) has fixed the pre-calculation requirement so it is more useful, but is still hundreds of times slower than MPU.
primes
Doesn't support ranges, requires bumping up the precalculated primes for larger numbers, which means knowing in advance the upper limit for primes. Support for numbers larger than 400M requires using Pari version 2.3.5. If that is used, sieving is about 2x faster than MPU, but doesn't support segmenting.
factorint
Similar to MPU's factor though with a different return (I find the result value quite inconvenient to work with, but others may like its vector of factor/exponent format). Slower than MPU for all 64-bit inputs on an x86_64 platform, it may be faster for large values on other platforms. With the newer Math::Prime::Util::GMP releases, bigint factoring is slightly faster in MPU.
eulerphi
Similar to MPU's euler_phi. MPU is 2-20x faster for native integers. There is also support for a range, which can be much more efficient. Without Math::Prime::Util::GMP installed, MPU is very slow with bigints. With it installed, it is about 2x slower than Math::Pari.
moebius
Similar to MPU's moebius. Comparisons are similar to eulerphi
.
sumdiv
Similar to MPU's divisor_sum. The standard sum (sigma_1) is very fast in MPU. Giving it a sub makes it much slower, and for numbers with very many factors, Pari is much faster.
eint1
Similar to MPU's ExponentialIntegral.
zeta
A more feature-rich version MPU's RiemannZeta function (supports negative and complex inputs).
Overall, Math::Pari supports a huge variety of functionality and has a sophisticated and mature code base behind it (noting that the default version of Pari used is about 10 years old now). For native integers sometimes the functions can be slower, but bigints are often superior and it rarely has any performance surprises. Some of the unique features MPU offers include super fast prime counts, nth_prime, ECPP primality proofs with certificates, approximations and limits for both, random primes, fast Mertens calculations, Chebyshev theta and psi functions, and the logarithmic integral and Riemann R functions. All with fairly minimal installation requirements.
Counting the primes to 10^10
(10 billion), with time in seconds. Pi(10^10) = 455,052,511. The numbers below are for sieving. Calculating Pi(10^10)
takes 0.064 seconds using the Lehmer algorithm in version 0.12.
External C programs in C / C++: 1.9 primesieve 3.6 forced to use only a single thread 2.2 yafu 1.31 3.8 primegen (optimized Sieve of Atkin, conf-word 8192) 5.6 Tomás Oliveira e Silva's unoptimized segmented sieve v2 (Sep 2010) 6.7 Achim Flammenkamp's prime_sieve (32k segments) 9.3 http://tverniquet.com/prime/ (mod 2310, single thread) 11.2 Tomás Oliveira e Silva's unoptimized segmented sieve v1 (May 2003) 17.0 Pari 2.3.5 (primepi) Small portable functions suitable for plugging into XS: 4.1 My segmented SoE used in this module (with unrolled inner loop) 15.6 My Sieve of Eratosthenes using a mod-30 wheel 17.2 A slightly modified verion of Terje Mathisen's mod-30 sieve 35.5 Basic Sieve of Eratosthenes on odd numbers 33.4 Sieve of Atkin, from Praxis (not correct) 72.8 Sieve of Atkin, 10-minute fixup of basic algorithm 91.6 Sieve of Atkin, Wikipedia-like
Perl modules, counting the primes to 800_000_000
(800 million):
Time (s) Module Version Notes --------- -------------------------- ------- ----------- 0.007 Math::Prime::Util 0.12 using Lehmer's method 0.27 Math::Prime::Util 0.17 segmented mod-30 sieve 0.39 Math::Prime::Util::PP 0.24 Perl (Lehmer's method) 0.9 Math::Prime::Util 0.01 mod-30 sieve 2.9 Math::Prime::FastSieve 0.12 decent odd-number sieve 11.7 Math::Prime::XS 0.26 needs some optimization 15.0 Bit::Vector 7.2 48.9 Math::Prime::Util::PP 0.14 Perl (fastest I know of) 170.0 Faster Perl sieve (net) 2012-01 array of odds 548.1 RosettaCode sieve (net) 2012-06 simplistic Perl 3048.1 Math::Primality 0.08 Perl + Math::GMPz ~11000 Math::Primality 0.04 Perl + Math::GMPz >20000 Math::Big 1.12 Perl, > 26GB RAM used
Python's standard modules are very slow: MPMATH v0.17 primepi
takes 169.5s and 25+ GB of RAM. SymPy 0.7.1 primepi
takes 292.2s. However there are very fast solutions written by Robert William Hanks (included in the xt/ directory of this distribution): pure Python in 12.1s and NUMPY in 2.8s.
is_prime
: my impressions for various sized inputs:
Module 1-10 digits 10-20 digits BigInts ----------------------- ----------- ------------ -------------- Math::Prime::Util Very fast Very fast Slow / Very Fast (1) Math::Prime::XS Very fast Very slow (2) -- Math::Prime::FastSieve Very fast N/A (3) -- Math::Primality Very slow Very slow Fast Math::Pari Slow OK OK / Fast (4) (1) Without / With L<Math::Prime::Util::GMP> installed. (2) Trial division only. Very fast if every factor is tiny. (3) Too much memory to hold the sieve (11dig = 6GB, 12dig = ~50GB) (4) By default L<Math::Pari> installs Pari 2.1.7, which uses 10 M-R tests for is_prime and is not fast. See notes below for 2.3.5.
The differences are in the implementations:
first does simple divisibility tests to quickly recognize composites, then looks in the sieve for a fast bit lookup if possible (default up to 30,000 but can be expanded via prime_precalc
). Next, for relatively small inputs, a deterministic set of Miller-Rabin tests are used, while for larger inputs a strong BPSW test is performed. For native integers, this is faster than any of the other modules. With Bigints, you need the Math::Prime::Util::GMP module installed to get good performance. With that installed, it is about 2x faster than Math::Primality and 10x faster than Math::Pari (default 2.1.7).
does trial divisions, which is wonderful if the input has a small factor (or is small itself). If given a large prime it can be tens of thousands of times slower than MPU. It does not support bigints.
only works in a sieved range, which is really fast if you can do it (M::P::U will do the same if you call prime_precalc
). Larger inputs just need too much time and memory for the sieve.
uses GMP (in Perl) for all work. Under ~32-bits it uses 2 or 3 MR tests, while above 4759123141 it performs a BPSW test. This is great for bigints over 2^64, but it is significantly slower than native precision tests. With 64-bit numbers it is generally an order of magnitude or more slower than any of the others. Once bigints are being used, its performance is quite good. It is faster than this module unless Math::Prime::Util::GMP has been installed, in which case Math::Prime::Util is faster.
has some very effective code, but it has some overhead to get to it from Perl. That means for small numbers it is relatively slow: an order of magnitude slower than M::P::XS and M::P::Util (though arguably this is only important for benchmarking since "slow" is ~2 microseconds). Large numbers transition over to smarter tests so don't slow down much. With the default Pari version, isprime
will do M-R tests for 10 randomly chosen bases, but can perform a Pocklington-Lehmer proof if requested using isprime(x,1)
. Both could fail to identify a composite. If pari 2.3.5 is used instead (this requires hand-building the Math::Pari module) then the options are quite different. ispseudoprime(x,0)
performs a strong BPSW test, while isprime
now performs a primality proof using a fast implementation of the APRCL method. While the APRCL method is very fast it is still much, much slower than a BPSW probable prime test for large inputs.
Factoring performance depends on the input, and the algorithm choices used are still being tuned. Math::Factor::XS is very fast when given input with only small factors, but it slows down rapidly as the smallest factor increases in size. For numbers larger than 32 bits, Math::Prime::Util can be 100x or more faster (a number with only very small factors will be nearly identical, while a semiprime with large factors will be the extreme end). Math::Pari is much slower with native sized inputs, probably due to calling overhead. For bigints, the Math::Prime::Util::GMP module is needed or performance will be far worse than Math::Pari. With the GMP module, performance is pretty similar from 20 through 70 digits, which the caveat that the current MPU factoring uses more memory for 60+ digit numbers.
This slide presentation has a lot of data on 64-bit and GMP factoring performance I collected in 2009. Assuming you do not know anything about the inputs, trial division and optimized Fermat or Lehman work very well for small numbers (<= 10 digits), while native SQUFOF is typically the method of choice for 11-18 digits (I've seen claims that a lightweight QS can be faster for 15+ digits). Some form of Quadratic Sieve is usually used for inputs in the 19-100 digit range, and beyond that is the General Number Field Sieve. For serious factoring, I recommend looking at yafu, msieve, gmp-ecm, GGNFS, and Pari. The latest yafu should cover most uses, with GGNFS likely only providing a benefit for numbers large enough to warrant distributed processing.
The n-1
proving algorithm in Math::Prime::Util::GMP compares well to the version including in Pari. Both are pretty fast to about 60 digits, and work reasonably well to 80 or so before starting to take over many minutes per number on a fast computer. Version 0.09 and newer of MPU::GMP contain an ECPP implementation that works quite well, though is certainly not state of the art. It averages less than a second for proving 200-digit primes, including creating a certificate. Times below 200 digits are faster than Pari 2.3.5's APR-CL proof. For larger inputs the bottleneck is a limited set of discriminants, and time becomes more variable. There is a larger set of discriminants on github that help, with 300-digit primes taking ~5 seconds on average and typically under a minute for 500-digits. For serious primality proving, I recommend Primo.
Dana Jacobsen <dana@acm.org>
Eratosthenes of Cyrene provided the elegant and simple algorithm for finding primes.
Terje Mathisen, A.R. Quesada, and B. Van Pelt all had useful ideas which I used in my wheel sieve.
Tomás Oliveira e Silva has released the source for a very fast segmented sieve. The current implementation does not use these ideas. Future versions might.
The SQUFOF implementation being used is a slight modification to the public domain racing version written by Ben Buhrow. Enhancements with ideas from Ben's later code as well as Jason Papadopoulos's public domain implementations are planned for a later version. The old SQUFOF implementation, still included in the code, is my modifications to Ben Buhrow's modifications to Bob Silverman's code.
Copyright 2011-2012 by Dana Jacobsen <dana@acm.org>
This program is free software; you can redistribute it and/or modify it under the same terms as Perl itself.