Primegrid: Searching for a New World Record Prime Number
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SIMD Extensions
SIMD Extensions PDF generated using the open source mwlib toolkit. See http://code.pediapress.com/ for more information. PDF generated at: Sat, 12 May 2012 17:14:46 UTC Contents Articles SIMD 1 MMX (instruction set) 6 3DNow! 8 Streaming SIMD Extensions 12 SSE2 16 SSE3 18 SSSE3 20 SSE4 22 SSE5 26 Advanced Vector Extensions 28 CVT16 instruction set 31 XOP instruction set 31 References Article Sources and Contributors 33 Image Sources, Licenses and Contributors 34 Article Licenses License 35 SIMD 1 SIMD Single instruction Multiple instruction Single data SISD MISD Multiple data SIMD MIMD Single instruction, multiple data (SIMD), is a class of parallel computers in Flynn's taxonomy. It describes computers with multiple processing elements that perform the same operation on multiple data simultaneously. Thus, such machines exploit data level parallelism. History The first use of SIMD instructions was in vector supercomputers of the early 1970s such as the CDC Star-100 and the Texas Instruments ASC, which could operate on a vector of data with a single instruction. Vector processing was especially popularized by Cray in the 1970s and 1980s. Vector-processing architectures are now considered separate from SIMD machines, based on the fact that vector machines processed the vectors one word at a time through pipelined processors (though still based on a single instruction), whereas modern SIMD machines process all elements of the vector simultaneously.[1] The first era of modern SIMD machines was characterized by massively parallel processing-style supercomputers such as the Thinking Machines CM-1 and CM-2. These machines had many limited-functionality processors that would work in parallel. -
New Formulas for Semi-Primes. Testing, Counting and Identification
New Formulas for Semi-Primes. Testing, Counting and Identification of the nth and next Semi-Primes Issam Kaddouraa, Samih Abdul-Nabib, Khadija Al-Akhrassa aDepartment of Mathematics, school of arts and sciences bDepartment of computers and communications engineering, Lebanese International University, Beirut, Lebanon Abstract In this paper we give a new semiprimality test and we construct a new formula for π(2)(N), the function that counts the number of semiprimes not exceeding a given number N. We also present new formulas to identify the nth semiprime and the next semiprime to a given number. The new formulas are based on the knowledge of the primes less than or equal to the cube roots 3 of N : P , P ....P 3 √N. 1 2 π( √N) ≤ Keywords: prime, semiprime, nth semiprime, next semiprime 1. Introduction Securing data remains a concern for every individual and every organiza- tion on the globe. In telecommunication, cryptography is one of the studies that permits the secure transfer of information [1] over the Internet. Prime numbers have special properties that make them of fundamental importance in cryptography. The core of the Internet security is based on protocols, such arXiv:1608.05405v1 [math.NT] 17 Aug 2016 as SSL and TSL [2] released in 1994 and persist as the basis for securing dif- ferent aspects of today’s Internet [3]. The Rivest-Shamir-Adleman encryption method [4], released in 1978, uses asymmetric keys for exchanging data. A secret key Sk and a public key Pk are generated by the recipient with the following property: A message enciphered Email addresses: [email protected] (Issam Kaddoura), [email protected] (Samih Abdul-Nabi) 1 by Pk can only be deciphered by Sk and vice versa. -
The Pseudoprimes to 25 • 109
MATHEMATICS OF COMPUTATION, VOLUME 35, NUMBER 151 JULY 1980, PAGES 1003-1026 The Pseudoprimes to 25 • 109 By Carl Pomerance, J. L. Selfridge and Samuel S. Wagstaff, Jr. Abstract. The odd composite n < 25 • 10 such that 2n_1 = 1 (mod n) have been determined and their distribution tabulated. We investigate the properties of three special types of pseudoprimes: Euler pseudoprimes, strong pseudoprimes, and Car- michael numbers. The theoretical upper bound and the heuristic lower bound due to Erdös for the counting function of the Carmichael numbers are both sharpened. Several new quick tests for primality are proposed, including some which combine pseudoprimes with Lucas sequences. 1. Introduction. According to Fermat's "Little Theorem", if p is prime and (a, p) = 1, then ap~1 = 1 (mod p). This theorem provides a "test" for primality which is very often correct: Given a large odd integer p, choose some a satisfying 1 <a <p - 1 and compute ap~1 (mod p). If ap~1 pi (mod p), then p is certainly composite. If ap~l = 1 (mod p), then p is probably prime. Odd composite numbers n for which (1) a"_1 = l (mod«) are called pseudoprimes to base a (psp(a)). (For simplicity, a can be any positive in- teger in this definition. We could let a be negative with little additional work. In the last 15 years, some authors have used pseudoprime (base a) to mean any number n > 1 satisfying (1), whether composite or prime.) It is well known that for each base a, there are infinitely many pseudoprimes to base a. -
Primes and Primality Testing
Primes and Primality Testing A Technological/Historical Perspective Jennifer Ellis Department of Mathematics and Computer Science What is a prime number? A number p greater than one is prime if and only if the only divisors of p are 1 and p. Examples: 2, 3, 5, and 7 A few larger examples: 71887 524287 65537 2127 1 Primality Testing: Origins Eratosthenes: Developed “sieve” method 276-194 B.C. Nicknamed Beta – “second place” in many different academic disciplines Also made contributions to www-history.mcs.st- geometry, approximation of andrews.ac.uk/PictDisplay/Eratosthenes.html the Earth’s circumference Sieve of Eratosthenes 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 Sieve of Eratosthenes We only need to “sieve” the multiples of numbers less than 10. Why? (10)(10)=100 (p)(q)<=100 Consider pq where p>10. Then for pq <=100, q must be less than 10. By sieving all the multiples of numbers less than 10 (here, multiples of q), we have removed all composite numbers less than 100. -
Read the Table of Square Roots 1-1000 Txt for Amazon
NCERT Solutions for Class 10 Maths Chapter 12. Numbers In Words 1 50 Number Words Chart Two Worksheets. Do Not Sell My Info (for CA Residents). When autocomplete results are available use up and down arrows to review and enter to select. Touch device users, explore by touch or with swipe gestures. Generated by PureJoy. Creation: 16:14 - May 21, 2020. Last Modification: 00:11 - Aug 29, 2020. If a 2 is present in ternary, turn it into 1T. For example, Your email address will not be published. Required fields are marked *. in the A440 pitch standard, a bit more than an octave higher in pitch than the highest note on a standard piano. Raising a physical quantity to a power results in a new physical quantity having a dimension with the exponents multiplied by the power. cubic meter = cubic feet x 0.028317017 cubic feet = cubic meter x. The MKS system based on the meter, kilogram second was augmented to allow force and energy from electrical quantities to be measured in one rationalized system of units. +91-22-25116741 The system was proposed by Giorgi in 1904. It was adopted by the IEC in 1935 to take [email protected] effect on January 1, 1940. The electrical to mechanical conversion was chosen to be based on the permeability of free space to be. 10111– palindromic prime in bases 3 (111212111 3 ) and 27 (DND 27 ). There are both color and black and white versions of the charts in printable pdf form. "10,000 promises" is a song by the Backstreet Boys. -
Appendix a Tables of Fermat Numbers and Their Prime Factors
Appendix A Tables of Fermat Numbers and Their Prime Factors The problem of distinguishing prime numbers from composite numbers and of resolving the latter into their prime factors is known to be one of the most important and useful in arithmetic. Carl Friedrich Gauss Disquisitiones arithmeticae, Sec. 329 Fermat Numbers Fo =3, FI =5, F2 =17, F3 =257, F4 =65537, F5 =4294967297, F6 =18446744073709551617, F7 =340282366920938463463374607431768211457, Fs =115792089237316195423570985008687907853 269984665640564039457584007913129639937, Fg =134078079299425970995740249982058461274 793658205923933777235614437217640300735 469768018742981669034276900318581864860 50853753882811946569946433649006084097, FlO =179769313486231590772930519078902473361 797697894230657273430081157732675805500 963132708477322407536021120113879871393 357658789768814416622492847430639474124 377767893424865485276302219601246094119 453082952085005768838150682342462881473 913110540827237163350510684586298239947 245938479716304835356329624224137217. The only known Fermat primes are Fo, ... , F4 • 208 17 lectures on Fermat numbers Completely Factored Composite Fermat Numbers m prime factor year discoverer 5 641 1732 Euler 5 6700417 1732 Euler 6 274177 1855 Clausen 6 67280421310721* 1855 Clausen 7 59649589127497217 1970 Morrison, Brillhart 7 5704689200685129054721 1970 Morrison, Brillhart 8 1238926361552897 1980 Brent, Pollard 8 p**62 1980 Brent, Pollard 9 2424833 1903 Western 9 P49 1990 Lenstra, Lenstra, Jr., Manasse, Pollard 9 p***99 1990 Lenstra, Lenstra, Jr., Manasse, Pollard -
CM55: Special Prime-Field Elliptic Curves Almost Optimizing Den Boer's
CM55: special prime-field elliptic curves almost optimizing den Boer's reduction between Diffie–Hellman and discrete logs Daniel R. L. Brown∗ February 24, 2015 Abstract Using the Pohlig{Hellman algorithm, den Boer reduced the discrete logarithm prob- lem to the Diffie–Hellman problem in groups of an order whose prime factors were each one plus a smooth number. This report reviews some related general conjectural lower bounds on the Diffie–Hellman problem in elliptic curve groups that relax the smoothness condition into a more commonly true condition. This report focuses on some elliptic curve parameters defined over a prime field size of size 9 + 55 × 2288, whose special form may provide some efficiency advantages over random fields of similar sizes. The curve has a point of Proth prime order 1 + 55 × 2286, which helps to nearly optimize the den Boer reduction. This curve is constructed using the CM method. It has cofactor 4, trace 6, and fundamental discriminant −55. This report also tries to consolidate the variety of ways of deciding between elliptic curves (or other algorithms) given the efficiency and security of each. Contents 1 Introduction3 2 Previous Work and Motivation4 2.1 den Boer's Reduction between DHP and DLP . .4 2.2 Complex Multiplication Method of Generating Elliptic Curves . .4 2.3 Earlier Publication of the CM55 Parameters . .4 3 Provable Security: Reducing DLP to DHP5 3.1 A Special Case of den Boer's Algorithm . .5 3.2 More Costly Reductions with Fewer Oracle Calls . .7 3.3 Relaxing the Smoothness Requirements . 11 4 Resisting Other Attacks on CM55 (if Trusted) 13 4.1 Resistance to the MOV Attack . -
Spin-Off Successes of SETI Research at Berkeley
**FULL TITLE** ASP Conference Series, Vol. **VOLUME**, c **YEAR OF PUBLICATION** **NAMES OF EDITORS** Spin-Off Successes of SETI Research at Berkeley K. A. Douglas School of Physics, University of Exeter, Exeter, United Kingdom D. P. Anderson, R. Bankay, H. Chen, J. Cobb, E.J. Korpela, M. Lebofsky, A. Parsons, J. Von Korff, D. Werthimer Space Sciences Laboratory, University of California Berkeley, Berkeley CA, USA 94720 Abstract. Our group contributes to the Search for Extra-Terrestrial Intelligence (SETI) by developing and using world-class signal processing computers to analyze data collected on the Arecibo telescope. Although no patterned signal of extra-terrestrial origin has yet been detected, and the immediate prospects for making such a detection are highly uncertain, the SETI@home project has nonetheless proven the value of pursuing such research through its impact on the fields of distributed computing, real-time signal pro- cessing, and radio astronomy. The SETI@home project has spun off the Center for Astronomy Signal Processing and Electronics Research (CASPER) and the Berkeley Open Infrastructure for Networked Computing (BOINC), both of which are responsi- ble for catalyzing a smorgasbord of new research in scientific disciplines in countries around the world. Futhermore, the data collected and archived for the SETI@home project is proving valuable in data-mining experiments for mapping neutral galatic hy- drogen and for detecting black-hole evaporation. 1 The SETI@home Project at UC Berkeley SETI@home is a distributed computing project harnessing the power from millions of volunteer computers around the world (Anderson 2002). Data collected at the Arecibo radio telescope via commensal observations are filtered and calibrated using real-time signal processing hardware, and selectable channels are recorded to disk. -
Goldbach's Conjecture
U.U.D.M. Project Report 2020:37 Goldbach’s Conjecture Johan Härdig Examensarbete i matematik, 15 hp Handledare: Veronica Crispin Quinonez Examinator: Martin Herschend Augusti 2020 Department of Mathematics Uppsala University Goldbach's Conjecture Johan H¨ardig Contents 1 Introduction 3 1.1 Definition of the Conjectures . 3 2 Prime Numbers and their Distribution 4 2.1 Early Results . 4 2.2 Prime Number Theorem . 6 3 Heuristic and Probabilistic Justification 8 3.1 Method Presented by Gaze & Gaze . 8 3.1.1 Sieve Method by Gaze & Gaze . 9 3.1.2 Example . 10 3.2 Prime Number Theorem for Arithmetic Progressions . 11 3.3 Distribution of Primes Across Prime Residue Classes . 14 3.4 Heuristic Justification by Gaze & Gaze . 15 3.4.1 Conclusion . 16 3.5 Goldbach's Comet . 17 4 The Ternary Goldbach's Conjecture 18 4.1 Historical Overview . 18 4.2 Approach . 19 4.3 Theorems and Methods in the Proof . 20 4.3.1 Hardy-Littlewood Circle Method . 20 4.3.2 Vinogradov's Theorem . 22 4.3.3 The Large Sieve . 24 4.3.4 L-functions . 24 4.3.5 Computational Methods . 26 4.4 The Proof . 29 1 CONTENTS 2 Abstract The following text will provide a historical perspective as well as investigate different approaches to the unsolved mathematical problem Goldbach's conjecture stated by Christian Goldbach in the year 1742. First off, there will be an overview of the early history of prime num- bers, and then a brief description of the Prime Number Theorem. Subsequently, an example of a heuristic and probabilistic method of justifying the binary Goldbach's conjecture, proposed by Gaze and Gaze, will be discussed. -
Analysis and Predictions of DNA Sequence Transformations on Grids
Analysis and Predictions of DNA Sequence Transformations on Grids A Thesis Submitted for the Degree of Master of Science (Engineering) in the Faculty of Engineering By Yadnyesh R. Joshi Supercomputer Education and Research Centre INDIAN INSTITUTE OF SCIENCE BANGALORE – 560 012, INDIA August 2007 Acknowledgments First of all I would like to extend my sincere thanks to my research supervisor Dr. Sathish Vadhiyar for his constant guidance and support during the entire period of my post-graduation at IISc. He was always approachable, supportive and ready to help in any sort of problem. I am very thankful to him for being extremely patient and understanding about the silly mistakes that I had made. Under his guidance I learned to approach problems in an organized manner and set realistic goals for my research. I thank him for his extreme patience and excellent technical guidance in writing and presenting research. Finally, he was and continues to be my role model for his hard work and passion for research. I am also thankful to Dr. Nagasuma Chandra, Dr. Debnath Pal from S.E.R.C. and Dr. Narendra Dixit from Chemical Engineering department for their very useful and interesting insights into the biological domain of our research. I am also thankful to all the faculty of S.E.R.C. for always inspiring us with their motivational talks. I would like to mention the names of my colleagues Sandip, Sanjay, Rakhi, Sundari, Antoine and Roshan for making their technical and emotional support. Special thanks to vatyaa kya group members for the adventures and the routines inside and outside the institute. -
Primegrid's Mega Prime Search
PrimeGrid’s Mega Prime Search On 23 October 2012, PrimeGrid’s Proth Prime Search project found the Mega Prime: 9*23497442 +1 The prime is 1,052,836 digits long and will enter Chris Caldwell's “The Largest Known Primes Database” (http://primes.utm.edu/primes) ranked 51st overall. This prime is also a Generalized Fermat prime and ranks as the 12th largest found. The discovery was made by Heinz Ming of Switzerland using an Intel Core(TM) i7 CPU 860 @ 2.80GHz with 8GB RAM, running Windows 7 Professional. This computer took just over 5 hours 59 minutes to complete the primality test using LLR. Heinz is a member of the Aggie The Pew team. The prime was verified by Tim McArdle, a member of the Don't Panic Labs team, using an AMD Athlon(tm) II P340 Dual-Core Processor with 6 GB RAM, running Windows 7 Professional. Credits for the discovery are as follows: 1. Heinz Ming (Swtzerland), discoverer 2. PrimeGrid, et al. 3. Srsieve, sieving program developed by Geoff Reynolds 4. PSieve, sieving program developed by Ken Brazier and Geoff Reynolds 5. LLR, primality program developed by Jean Penné 6. OpenPFGW, a primality program developed by Chris Nash & Jim Fougeron with maintenance and improvements by Mark Rodenkirch OpenPFGW, a primality program developed by Chris Nash & Jim Fougeron, was used to check for Fermat Number divisibility (including generalized and extended). For more information about Fermat and generalized Fermat Number divisors, please see Wilfrid Keller's sites: http://www.prothsearch.net/fermat.html http://www1.uni-hamburg.de/RRZ/W.Keller/GFNfacs.html Generalized and extended generalized Fermat number divisors discovered are as follows: 9*2^3497442+1 is a Factor of GF(3497441,7) 9*2^3497442+1 is a Factor of xGF(3497438,9,8) 9*2^3497442+1 is a Factor of GF(3497441,10) 9*2^3497442+1 is a Factor of xGF(3497439,11,3) 9*2^3497442+1 is a Factor of xGF(3497441,12,5) Using a single PC would have taken years to find this prime. -
A Prime Experience CP.Pdf
p 2 −1 M 44 Mersenne n 2 2 −1 Fermat n 2 2( − )1 − 2 n 3 3 k × 2 +1 m − n , m = n +1 m − n n 2 + 1 3 A Prime Experience. Version 1.00 – May 2008. Written by Anthony Harradine and Alastair Lupton Copyright © Harradine and Lupton 2008. Copyright Information. The materials within, in their present form, can be used free of charge for the purpose of facilitating the learning of children in such a way that no monetary profit is made. The materials cannot be used or reproduced in any other publications or for use in any other way without the express permission of the authors. © A Harradine & A Lupton Draft, May, 2008 WIP 2 Index Section Page 1. What do you know about Primes? 5 2. Arithmetic Sequences of Prime Numbers. 6 3. Generating Prime Numbers. 7 4. Going Further. 9 5. eTech Support. 10 6. Appendix. 14 7. Answers. 16 © A Harradine & A Lupton Draft, May, 2008 WIP 3 Using this resource. This resource is not a text book. It contains material that is hoped will be covered as a dialogue between students and teacher and/or students and students. You, as a teacher, must plan carefully ‘your performance’. The inclusion of all the ‘stuff’ is to support: • you (the teacher) in how to plan your performance – what questions to ask, when and so on, • the student that may be absent, • parents or tutors who may be unfamiliar with the way in which this approach unfolds. Professional development sessions in how to deliver this approach are available.