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The **quadratic sieve** algorithm (**QS**) is an integer factorization algorithm and, in practice, the second fastest method known (after the general number field sieve). It is still the fastest for integers under 100 decimal digits or so, and is considerably simpler than the number field sieve. It is a general-purpose factorization algorithm, meaning that its running time depends solely on the size of the integer to be factored, and not on special structure or properties. It was invented by Carl Pomerance in 1981 as an improvement to Schroeppel's linear sieve.^{[1]}

The algorithm attempts to set up a congruence of squares modulo *n* (the integer to be factorized), which often leads to a factorization of *n*. The algorithm works in two phases: the *data collection* phase, where it collects information that may lead to a congruence of squares; and the *data processing* phase, where it puts all the data it has collected into a matrix and solves it to obtain a congruence of squares. The data collection phase can be easily parallelized to many processors, but the data processing phase requires large amounts of memory, and is difficult to parallelize efficiently over many nodes or if the processing nodes do not each have enough memory to store the whole matrix. The block Wiedemann algorithm can be used in the case of a few systems each capable of holding the matrix.

The naive approach to finding a congruence of squares is to pick a random number, square it, divide by *n* and hope the least non-negative remainder is a perfect square. For example, . This approach finds a congruence of squares only rarely for large *n*, but when it does find one, more often than not, the congruence is nontrivial and the factorization is complete. This is roughly the basis of Fermat's factorization method.

The quadratic sieve is a modification of Dixon's factorization method.

The general running time required for the quadratic sieve (to factor an integer *n*) is

in the L-notation.^{[2]}

The constant *e* is the base of the natural logarithm.

To factorize the integer *n*, Fermat's method entails a search for a single number *a*, *n*^{1/2} < *a* < *n*−1, such that the remainder of *a*^{2} divided by *n* is a square. But these *a* are hard to find. The quadratic sieve consists of computing the remainder of *a*^{2}/*n* for several *a*, then finding a subset of these whose product is a square. This will yield a congruence of squares.

For example, consider attempting to factor the number 1649. We have: . None of the integers is a square, but the product is a square. We also had

since . The observation that thus gives a congruence of squares

Hence for some integer . We can then factor

using the Euclidean algorithm to calculate the greatest common divisor.

So the problem has now been reduced to: given a set of integers, find a subset whose product is a square. By the fundamental theorem of arithmetic, any positive integer can be written uniquely as a product of prime powers. We do this in a vector format; for example, the prime-power factorization of 504 is 2^{3}3^{2}5^{0}7^{1}, it is therefore represented by the exponent vector (3,2,0,1). Multiplying two integers then corresponds to adding their exponent vectors. A number is a square when its exponent vector is even in every coordinate. For example, the vectors (3,2,0,1) + (1,0,0,1) = (4,2,0,2), so (504)(14) is a square. Searching for a square requires knowledge only of the parity of the numbers in the vectors, so it is sufficient to compute these vectors mod 2: (1,0,0,1) + (1,0,0,1) = (0,0,0,0).
So given a set of (0,1)-vectors, we need to find a subset which adds to the zero vector mod 2.

This is a linear algebra problem since the ring can be regarded as the Galois field of order 2, that is we can divide by all non-zero numbers (there is only one, namely 1) when calculating modulo 2.
It is a theorem of linear algebra that with more vectors than each vector has entries, a linear dependency always exists. It can be found by Gaussian elimination.
However, simply squaring many random numbers mod *n* produces a very large number of different prime factors, and so very long vectors and a very large matrix. The trick is to look specifically for numbers *a* such that *a*^{2} mod *n* has only small prime factors (they are smooth numbers). They are harder to find, but using only smooth numbers keeps the vectors and matrices smaller and more tractable. The quadratic sieve searches for smooth numbers using a technique called sieving, discussed later, from which the algorithm takes its name.

To summarize, the basic quadratic sieve algorithm has these main steps:

- Choose a smoothness bound
*B*. The number π(*B*), denoting the number of prime numbers less than*B*, will control both the length of the vectors and the number of vectors needed. - Use sieving to locate π(
*B*) + 1 numbers*a*such that_{i}*b*= (_{i}*a*_{i}^{2}mod*n*) is*B*-smooth. - Factor the
*b*and generate exponent vectors mod 2 for each one._{i} - Use linear algebra to find a subset of these vectors which add to the zero vector. Multiply the corresponding
*a*together and give the result mod_{i}*n*the name*a*; similarly, multiply the*b*together which yields a_{i}*B*-smooth square*b*^{2}. - We are now left with the equality
*a*^{2}=*b*^{2}mod*n*from which we get two square roots of (*a*^{2}mod*n*), one by taking the square root in the integers of*b*^{2}namely*b*, and the other the*a*computed in step 4. - We now have the desired identity: . Compute the GCD of
*n*with the difference (or sum) of*a*and*b*. This produces a factor, although it may be a trivial factor (*n*or 1). If the factor is trivial, try again with a different linear dependency or different*a*.

The remainder of this article explains details and extensions of this basic algorithm.

algorithmQuadratic sieveisChoose smoothness bound letfordoChoose (where )while(check-p_t-smooth(b_i) = false)doLet Find let letifandthenreturngcd(x - y, n) , gcd(x + y, n)else :return to main loop.

The quadratic sieve attempts to find pairs of integers *x* and *y*(*x*) (where *y*(*x*) is a function of *x*) satisfying a much weaker condition than *x*^{2} ≡ *y*^{2} (mod *n*). It selects a set of primes called the *factor base*, and attempts to find *x* such that the least absolute remainder of *y*(*x*) = *x*^{2} mod *n* factorizes completely over the factor base. Such *y* values are said to be *smooth* with respect to the factor base.

The factorization of a value of *y*(*x*) that splits over the factor base, together with the value of *x*, is known as a *relation*. The quadratic sieve speeds up the process of finding relations by taking *x* close to the square root of *n*. This ensures that *y*(*x*) will be smaller, and thus have a greater chance of being smooth.

This implies that *y* is on the order of 2*x*[√*n*]. However, it also implies that *y* grows linearly with *x* times the square root of *n*.

Another way to increase the chance of smoothness is by simply increasing the size of the factor base. However, it is necessary to find at least one smooth relation more than the number of primes in the factor base, to ensure the existence of a linear dependency.

Even if for some relation *y*(*x*) is not smooth, it may be possible to merge two of these *partial relations* to form a full one, if the two *y*'s are products of the same prime(s) outside the factor base. [Note that this is equivalent to extending the factor base.] For example, if the factor base is {2, 3, 5, 7} and *n* = 91, there are partial relations:

Multiply these together:

and multiply both sides by (11^{−1})^{2} modulo 91. 11^{−1} modulo 91 is 58, so:

producing a full relation. Such a full relation (obtained by combining partial relations) is called a *cycle*. Sometimes, forming a cycle from two partial relations leads directly to a congruence of squares, but rarely.

There are several ways to check for smoothness of the *y*s. The most obvious is by trial division, although this increases the running time for the data collection phase. Another method that has some acceptance is the elliptic curve method (ECM). In practice, a process called *sieving* is typically used. If *f*(*x*) is the polynomial we have

Thus solving *f(x)* ≡ 0 (mod *p*) for *x* generates a whole sequence of numbers *y* for which *y*=*f*(*x*), all of which are divisible by *p*. This is finding a square root modulo a prime, for which there exist efficient algorithms, such as the Shanks–Tonelli algorithm. (This is where the quadratic sieve gets its name: *y* is a quadratic polynomial in *x*, and the sieving process works like the Sieve of Eratosthenes.)

The sieve starts by setting every entry in a large array *A*[] of bytes to zero. For each *p*, solve the quadratic equation mod *p* to get two roots *α* and *β*, and then add an approximation to log(*p*) to every entry for which *y*(*x*) = 0 mod *p* ... that is, *A*[*kp* + *α*] and *A*[*kp* + *β*]. It is also necessary to solve the quadratic equation modulo small powers of *p* in order to recognise numbers divisible by small powers of a factor-base prime.

At the end of the factor base, any *A*[] containing a value above a threshold of roughly log(*x*^{2}−*n*) will correspond to a value of *y*(*x*) which splits over the factor base. The information about exactly which primes divide *y*(*x*) has been lost, but it has only small factors, and there are many good algorithms for factoring a number known to have only small factors, such as trial division by small primes, SQUFOF, Pollard rho, and ECM, which are usually used in some combination.

There are many *y*(*x*) values that work, so the factorization process at the end doesn't have to be entirely reliable; often the processes misbehave on say 5% of inputs, requiring a small amount of extra sieving.

This example will demonstrate standard quadratic sieve without logarithm optimizations or prime powers. Let the number to be factored *N* = 15347, therefore the ceiling of the square root of *N* is 124. Since *N* is small, the basic polynomial is enough: *y*(*x*) = (*x* + 124)^{2} − 15347.

Since *N* is small, only 4 primes are necessary. The first 4 primes *p* for which 15347 has a square root mod *p* are 2, 17, 23, and 29 (in other words, 15347 is a quadratic residue modulo each of these primes). These primes will be the basis for sieving.

Now we construct our sieve of and begin the sieving process for each prime in the basis, choosing to sieve the first 0 ≤ X < 100 of Y(X):

The next step is to perform the sieve. For each *p* in our factor base solve the equation

to find the entries in the array *V* which are divisible by *p*.

For solve to get the solution .

Thus, starting at X=1 and incrementing by 2, each entry will be divisible by 2. Dividing each of those entries by 2 yields

Similarly for the remaining primes *p* in the equation is solved. Note that for every *p* > 2, there will be 2 resulting linear equations due to there being 2 modular square roots.

Each equation results in being divisible by *p* at *x*=*a* and each *p*th value beyond that. Dividing *V* by *p* at *a*, *a*+*p*, *a*+2*p*, *a*+3*p*, etc., for each prime in the basis finds the smooth numbers which are products of unique primes (first powers).

Any entry of *V* that equals 1 corresponds to a smooth number. Since , , and equal one, this corresponds to:

X + 124 |
Y |
factors |
---|---|---|

124 | 29 | 2^{0} • 17^{0} • 23^{0} • 29^{1} |

127 | 782 | 2^{1} • 17^{1} • 23^{1} • 29^{0} |

195 | 22678 | 2^{1} • 17^{1} • 23^{1} • 29^{1} |

Since smooth numbers *Y* have been found with the property , the remainder of the algorithm follows equivalently to any other variation of Dixon's factorization method.

Writing the exponents of the product of a subset of the equations

as a matrix yields:

A solution to the equation is given by the left null space, simply

Thus the product of all 3 equations yields a square (mod N).

and

So the algorithm found

Testing the result yields GCD(3070860 - 22678, 15347) = 103, a nontrivial factor of 15347, the other being 149.

This demonstration should also serve to show that the quadratic sieve is only appropriate when *n* is large. For a number as small as 15347, this algorithm is overkill. Trial division or Pollard rho could have found a factor with much less computation.

In practice, many different polynomials are used for *y*, since only one polynomial will not typically provide enough (*x*, *y*) pairs that are smooth over the factor base. The polynomials used must have a special form, since they need to be squares modulo *n*. The polynomials must all have a similar form to the original *y*(*x*) = *x*^{2} − *n*:

Assuming is a multiple of A, so that the polynomial y(x) can be written as . If *A* is a square, then only the factor has to be considered.

This approach (called MPQS, Multiple Polynomial Quadratic Sieve) is ideally suited for parallelization, since each processor involved in the factorization can be given *n*, the factor base and a collection of polynomials, and it will have no need to communicate with the central processor until it is finished with its polynomials.

If, after dividing by all the factors less than *A*, the remaining part of the number (the cofactor) is less than *A*^{2}, then this cofactor must be prime. In effect, it can be added to the factor base, by sorting the list of relations into order by cofactor. If y(a) = 7*11*23*137 and y(b) = 3*5*7*137, then y(a)y(b) = 3*5*11*23 * 7^{2} * 137^{2}. This works by reducing the threshold of entries in the sieving array above which a full factorization is performed.

Reducing the threshold even further, and using an effective process for factoring y(x) values into products of even relatively large primes - ECM is superb for this - can find relations with most of their factors in the factor base, but with two or even three larger primes. Cycle finding then allows combining a set of relations sharing several primes into a single relation.

To illustrate typical parameter choices for a realistic example on a real implementation including the multiple polynomial and large prime optimizations, the tool msieve was run on a 267-bit semiprime, producing the following parameters:

- Trial factoring cutoff: 27 bits
- Sieve interval (per polynomial): 393216 (12 blocks of size 32768)
- Smoothness bound: 1300967 (50294 primes)
- Number of factors for polynomial
*A*coefficients: 10*(see Multiple polynomials above)* - Large prime bound: 128795733 (26 bits)
*(see Large primes above)* - Smooth values found: 25952 by sieving directly, 24462 by combining numbers with large primes
- Final matrix size: 50294 × 50414, reduced by filtering to 35750 × 35862
- Nontrivial dependencies found: 15
- Total time (on a 1.6 GHz UltraSPARC III): 35 min 39 seconds
- Maximum memory used: 8 MB

Until the discovery of the number field sieve (NFS), QS was the asymptotically fastest known general-purpose factoring algorithm. Now, Lenstra elliptic curve factorization has the same asymptotic running time as QS (in the case where *n* has exactly two prime factors of equal size), but in practice, QS is faster since it uses single-precision operations instead of the multi-precision operations used by the elliptic curve method.

On April 2, 1994, the factorization of RSA-129 was completed using QS. It was a 129-digit number, the product of two large primes, one of 64 digits and the other of 65. The factor base for this factorization contained 524339 primes. The data collection phase took 5000 MIPS-years, done in distributed fashion over the Internet. The data collected totaled 2GB. The data processing phase took 45 hours on Bellcore's (now Telcordia Technologies) MasPar (massively parallel) supercomputer. This was the largest published factorization by a general-purpose algorithm, until NFS was used to factor RSA-130, completed April 10, 1996. All RSA numbers factored since then have been factored using NFS.

The current QS factorization record is the 140 digit (463 bit) RSA-140, which was factored by Patrick Konsor in June 2020 using approximately 6,000 core hours over 6 days.^{[3]}

- PPMPQS and PPSIQS
- mpqs
- SIMPQS is a fast implementation of the self-initialising multiple polynomial quadratic sieve written by William Hart. It provides support for the large prime variant and uses Jason Papadopoulos' block Lanczos code for the linear algebra stage. SIMPQS is accessible as the qsieve command in the SageMath computer algebra package or can be downloaded in source form. SIMPQS is optimized for use on Athlon and Opteron machines, but will operate on most common 32- and 64-bit architectures. It is written entirely in C.
- a factoring applet by Dario Alpern, that uses the quadratic sieve if certain conditions are met.
- The PARI/GP computer algebra package includes an implementation of the self-initialising multiple polynomial quadratic sieve implementing the large prime variant. It was adapted by Thomas Papanikolaou and Xavier Roblot from a sieve written for the LiDIA project. The self initialisation scheme is based on an idea from the thesis of Thomas Sosnowski.
- A variant of the quadratic sieve is available in the MAGMA computer algebra package. It is based on an implementation of Arjen Lenstra from 1995, used in his "factoring by email" program.
- msieve, an implementation of the multiple polynomial quadratic sieve with support for single and double large primes, written by Jason Papadopoulos. Source code and a Windows binary are available.
- YAFU, written by Ben Buhrow, is similar to msieve but is faster for most modern processors. It uses Jason Papadopoulos' block Lanczos code. Source code and binaries for Windows and Linux are available.
- Ariel, a simple Java implementation of the quadratic sieve for didactic purposes.
- The java-math-library contains probably the fastest quadratic sieve written in Java (the successor of PSIQS 4.0).
- Java QS, an open source Java project containing basic implementation of QS. Released at February 4, 2016 by Ilya Gazman
- C Quadratic Sieve, a factorizer written entirely in C containing implementation of self-initialising Quadratic Sieve. The project is mathematically inspired by a William Hart's FLINT factorizer. The source released in 2022 by Michel Leonard does not rely on external library, it is capable of factoring 220-bit numbers in a minute.
- The RcppBigIntAlgos package by Joseph Wood, provides an efficient implementation of the multiple polynomial quadratic sieve for the R programming language. It is written in C++ and is capable of comfortably factoring 100 digit semiprimes. For example, RSA-100 was factored in under 16 hours on a 2.8 GHz Quad-Core Intel Core i7 personal computer.

**^**Carl Pomerance, Analysis and Comparison of Some Integer Factoring Algorithms, in Computational Methods in Number Theory, Part I, H.W. Lenstra, Jr. and R. Tijdeman, eds., Math. Centre Tract 154, Amsterdam, 1982, pp 89-139.**^**Pomerance, Carl (December 1996). "A Tale of Two Sieves" (PDF).*Notices of the AMS*. Vol. 43, no. 12. pp. 1473–1485.**^**"Useless Accomplishment: RSA-140 Factorization with Quadratic Sieve - mersenneforum.org".*www.mersenneforum.org*. Retrieved 2020-07-07.

- Richard Crandall and Carl Pomerance (2001).
*Prime Numbers: A Computational Perspective*(1st ed.). Springer. ISBN 0-387-94777-9. Section 6.1: The quadratic sieve factorization method, pp. 227–244.

- Samuel S. Wagstaff, Jr. (2013).
*The Joy of Factoring*. Providence, RI: American Mathematical Society. pp. 195–202. ISBN 978-1-4704-1048-3.

- Reference paper "The Quadratic Sieve Factoring Algorithm" by Eric Landquist