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#45 | ||
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Jun 2005
lehigh.edu
210 Posts |
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ahead of the current curve (a jump from the record p68 to a new record p73) than I was when my p66 broke the p59 record. The reason is not the number of digits (plus 5 -vs- plus 7), but rather on my impression (based on no math whatsoever) that the ratio of likelihoods for p73 over p69 represents a more substantial jump than the corresponding likelihood ratio p66 over p59. In an email reply to Phil McLaughlin, PaulZ reports a very substantial view of the current ecm status: Quote:
t55's up towards 3t55's (Aoki and Thorsten hold the range above 3t55), I'm doubtful. Aoki, Thorsten and PaulZ himself have demonstrated having the resources to run ECM above 2t55, but my experience suggests that people with moderate-to-midling resources will find the search for factors in this range too un-rewarding. Again, the formulation is that we're running ECM on numbers for which a full test (to 62%) for p55-factors is already complete (resp. 2t55 and 3t55; 1-e^2 and 1-e^3). On the topic of ecm-misses, I'm still most interested in the topic of Silverman-Wagstaff on allocating resources most effectively between ecm and sieving. As Bob's agreed, our current extreme hetrogeneous environment massively complicates their situation, in which it is possible to imagine a reasonable comparison based on using the same hardware for both ecm and for sieving. Post-Kansas (or Indiana, maybe?) we've had the sieving hardware distinct from running ecm of a grid of PCs not suitable for sieving (at the time); then (briefly!) running ecm under Yoyo/BOINC; and now (for the fortunate few) on GPUs (cell or ...). We currently have the Batalov+D range of sieving (both snfs and gnfs) in difficulty below snfs difficulty 250; and Greg's NFS@Home range of mid-250 to (mostly) just below 270. I'm still holding firm on something like 1.5t55 (for B+D) and somewhere between 2t55-to-3t55 (for Greg). Regards, Bruce PS -- Uhm, there are actually (at least) two fronts in the ecm attack on the dwindling current Cunningham list. The one above is where both ecm and sieving are plausible. The two most recent Aoki factors of p50/p51 represent numbers from c234-c366 that aren't near-term sieving candidates. These numbers need to have ecm testing raised from 2t50 to 3t50 (to start ...). There's a different difficulty here; with too many numbers having no prime factors in ecm range. Already we can see lots of these in diff below 250, resp. below 270; and this will get worse with the rest of c234-c366 (the "Largest Cunninghams"). PaulZ's email seems to suggest (to me at least ...) a third front of smaller numbers, having passed (failed?) a larger ecm test. A moving target here, this was c154-c189.99; currently c161-c209.99; and working toward c176-c233.99 (the "Smallest Cunninghams"). If I'm reading PaulZ correctly, he seems to suggest more extended ecm effort even on numbers for which sieving is not-so-difficulty; sort-of "yes, we can" factor these numbers by ecm! |
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#46 |
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Jul 2003
So Cal
40728 Posts |
NFS@Home has finished 5,427+ by SNFS as usual.
Code:
prp54 factor: 563755283862496929168659991708057447948580426252052767 prp145 factor: 2723528882195134624435365406241362651957822673755720745626178581944304857470575651366951292535191262712823827955524329324491207238166486348539107 |
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#47 | |
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Nov 2003
22·5·373 Posts |
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#48 | |
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Jun 2005
lehigh.edu
210 Posts |
Quote:
finding this p54. The C199 was from the c190-c209.99 range; initially from c190-c233, over diff 249.99 (at diff 255.8). So that was an initial 3t50; then the +3t50 for c190-c233 was Code:
1236333 Aug 8 2009 c9009/aug07-cu3140-p55-1t50-h2 1503832 Sep 29 2009 c9009/sep27-cu3800leaf-p60-2t50-h2 Code:
Mar 12 13:02 c9009/c99.h2-5p427needs4 Code:
3036044 Mar 22 09:49 c9009/mar18-cu7593-p60-4t50-c9h2-fin of the pre-history curves had limits under t50 (perhaps one of the t50's), the rest t55 or t60; all of which were suitable (within 5-digits of optimal runtime) for finding this p54. Then 3140 curves with t55 (B1 = 110M) limits, 3800+7593 curves with t60 (B1 = 260M) limits. That part alone, without counting the initial 3t50 miss, was a solid t55. So this one meets my view of an ecm miss, the curves were actually run; ecm had its chance to find this p54. The only slight quibble is a review of what a t55, resp. 2t55 means. That's a 62% chance of finding a known p55; resp. 80% chance. The probabilistic test finds just short of 2-out-of-3 p55's; resp. 4-out-of-5 p55's. Since the above count is a bit short of 2t55, perhaps ecm ought to have found 3-out-of-4 of these p54's. So if we look at the pool of Cunninghams from Nov 2003 (when I started these condor searches) of size c190-c209.99; drop the ones with a factor below p50; wait until the rest of that initial pool are factored, and drop the ones with smallest factor p60-or-larger; _then_ we could check to see whether ecm had done better or worse than finding 3-of-4 of the p54/p55's. ("Probablity with sample size one is meaningless.") For another view, suppose that we knew this C199 had this p54 factor; and that 10t50 had missed. Would we try to remove this factor (to prob 80%?) using ecm? Note that the prevous curves have already missed; we don't get to count them, this would be a new 2t55 (or t55). That's more favorable than the actual situation. All we actually know is that 10t50 "missed", not that there's a lurking p54 in this c199; rather that there's nearly certain that some p53-p57's haven't yet been found among a pool of near-term sieving candidates. I placed my bet on this one, contributing c. 10% of the NFS@Home sieving; and I'll continue with subsequent diff < 260's that have passed 10t50. Better that than adding another 3t50 on a pool of candidates, most, far-and-away-most, having their factors above p60 and hard for ecm to find. (This isn't a Mersenne number, ps3 standards don't apply.) Not sure that having the first clearcut miss occur on the 50th factorization matters that much to me (a random NFS@Home contributor...); rather I'm still glad not to have gotten one from the ones sieved with the 16e siever, diff 270-and-up. Then I'd have to think about bumping the curve counts up (depending upon what the condor pc/pool looks like; most of the core2's seem to have dropped out on the switch to windows7 --- skipping past vista, which we never used here). -Bruce |
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#49 |
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Jul 2003
So Cal
2×34×13 Posts |
NFS@Home has completed 5,448+ by SNFS. A 16.1M matrix was solved using 64 computers (256 cores) in a bit under 41 hours. The log is attached.
Code:
prp65 factor: 23371863775658144623538828456854573496104607906605333794952273409 prp141 factor: 698965867837568984299398033395117263633121275562035049049008890847786442548362928940407820059804253774285034574979465129314235059775249213313 |
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#50 |
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Noodles
"Mr. Tuch"
Dec 2007
Chennai, India
3×419 Posts |
5,415+ c204 lovely split up: p102.p102 wonderful natural RSA like number!
Previous Venus transit was on June 8, 2004 Next Venus transit will be upon June 6, 2012 Yesterday, that Venus crossed up with that position of Inferior Conjunction 5,415+ was started up when it was rather even before its eastern most elongation position One of my hardest jobs ever 5,415+ c204, SNFS difficulty = 232.0584144 nominally; with a quartic polynomial is equal to that value for that 332*log(5) that is being in use, that way. By using parameters as: Algebraic polynomial = x^4-x^3+x^2-x+1 Rational polynomial = x-5^83 Sieved up from special-q ranges for that values of 110M to 300M (190M range) upon that rational side with that help of gnfs-lasieve4I15e lattice siever By using that following parameters scale:-> As, Code:
n: 409070648357903876177895795121676558808515790800199330391475022633084608638318069844299258901345227277398314550159052254251424043657457443453213674736966457975676435972876537687720951817693078563918161701 m: 10339757656912845935892608650874535669572651386260986328125 c4: 1 c3: -1 c2: 1 c1: -1 c0: 1 skew: 1 type: snfs rlim: 200000000 alim: 33554431 lpbr: 31 lpba: 29 mfbr: 62 mfba: 58 rlambda: 2.6 alambda: 2.6 that was solved by using that msieve software within 36 days of calendar time, under that 4 threads (hyperthreading model), singularly, without making any uses for that MPI interface for that cluster computing facilities at all Ultimately, for that number 5,415+ its factors are respectively, as follows Code:
prp102 factor: 542386699809206521167664377679235482113503370942017294492342497725064744615307084697173312788543096361 prp102 factor: 754204792451218350821809245865692448592809318994740143792927132204178344974350929553423826459243126941 like that for a natural RSA number, right then! that has been encountered by me up, for ever of course |
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#51 |
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"Serge"
Mar 2008
Phi(4,2^7658614+1)/2
22·23·103 Posts |
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#52 |
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Noodles
"Mr. Tuch"
Dec 2007
Chennai, India
3·419 Posts |
Thank you, but why so late?
5 days after that time when I posted with its factors? Were you searching up for this picture, which you thought that you would post it as soon as you saw with the nice split of the factors for that number immediately? Or that it was a leisurely thought later on? By the way, what is that nice split over there? An jumping athlete, who has been photographed with his/her left, right parts of body being partitioned into half, as he jumps over the ground when he keeps up with his own body style? For everyone, let me know up about the fact that who maintains up with that odd perfect number search page, at http://www.oddperfect.org/ -> thus, is it wblipp? so, and then that Fermat number factors page, at http://www.prothsearch.net/fermat.html Is it Mr. Wilfred Keller, or that is it someone else who has taken up in charge for that page, from within this forum itself? Last fiddled with by Raman on 2010-11-03 at 19:21 |
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#53 | |
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"William"
May 2003
New Haven
44768 Posts |
Quote:
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#54 |
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Noodles
"Mr. Tuch"
Dec 2007
Chennai, India
3×419 Posts |
Then, why is the status for that number 3,607- which has been factored as of now, not yet been updated, still?
thus, even in spite of reading up with that post !! Last fiddled with by Raman on 2010-11-04 at 05:58 |
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#55 |
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Jul 2003
So Cal
2·34·13 Posts |
Patience! Real life interferes.
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