Timeline for $S$-Tate-Shafarevich groups of elliptic curves
Current License: CC BY-SA 3.0
12 events
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Jan 23, 2014 at 13:31 | vote | accept | Daniel Loughran | ||
Jan 23, 2014 at 10:48 | answer | added | Chris Wuthrich | timeline score: 7 | |
Jan 23, 2014 at 9:29 | comment | added | Daniel Loughran | Thanks anon. If one of you would like to post your comments as an answer, I will accept it. | |
Jan 23, 2014 at 7:58 | comment | added | abz | The problem is only for torsion at primes in S. More precisely, let m be an integer not divisible by any prime in S. Then the subgroup of the S Tate-Shafarevich group killed by some power of m coincides with the similar subgroup of the usual Tate-Shafarevich group. This is a standard result (see for example Milne's Arithmetic Duality Theorems I, 6.6., but note that his S is the complement of yours). | |
Jan 22, 2014 at 23:23 | history | edited | Daniel Loughran | CC BY-SA 3.0 |
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Jan 22, 2014 at 22:30 | comment | added | user76758 | Example 7.5.1 in the paper "Finiteness theorems for algebraic groups over function fields" in Compositio Math. 148 (2012), which uses just standard methods in global Galois cohomology (duality theorems, etc.) There must be earlier references on this issue as well. | |
Jan 22, 2014 at 19:34 | comment | added | Daniel Loughran | I see, can you offer some references? | |
Jan 22, 2014 at 16:54 | comment | added | user76758 | No, once you allow non-empty $S$ it is often (maybe always?) provably infinite, in contrast with the case of linear algebraic groups, for which the "$S$-version" is provably always finite. | |
Jan 22, 2014 at 14:38 | comment | added | Daniel Loughran | No, my question is about what happens when $S$ is non-empty. I have edited the question to make it clearer. | |
Jan 22, 2014 at 14:36 | history | edited | Daniel Loughran | CC BY-SA 3.0 |
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Jan 22, 2014 at 13:37 | comment | added | Jason Starr | Did you just post the Shafarevich conjecture as a Math Overflow question? | |
Jan 22, 2014 at 13:31 | history | asked | Daniel Loughran | CC BY-SA 3.0 |