#9407: fixed fields for dirichlet characters and conductors and dirichlet
characters for abelian fields
-----------------------------------------------------------+----------------
   Reporter:  wuthrich                                     |       Owner:  
davidloeffler                                           
       Type:  enhancement                                  |      Status:  
needs_work                                              
   Priority:  minor                                        |   Milestone:  
sage-4.6.1                                              
  Component:  number fields                                |    Keywords:  
Dirichlet characters, abelian fields, class field theory
     Author:  Michael Daub, John Bergdall, Chris Wuthrich  |    Upstream:  N/A  
                                                   
   Reviewer:                                               |      Merged:       
                                                   
Work_issues:                                               |  
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Comment(by wuthrich):

 > #9400 is now merged: does that help?

 Maybe, I did not think about it.

 > How hard is it to get the 2-part of the conductor?  If it is really
 hard, why not just honestly return the odd part (and change the name, or
 something)?

 I don't know. Right now it give the right thing quite frequently, but not
 always. I would have to think harder to see if one can put the 2-part in
 as well. I won't do that, I fear.

 > I am a bit worried about the 53-bit precision used to compute the
 polynomials.  Do you now that it always enough (surely not!), or is that
 wishful thinking?  Is it much too slow to use the appropriate cyclotomic
 field?

 It is really very very slow with cyclotomic fields. To be honest, I do not
 think anyone wants to construct a field of the size that would require
 higher precision in this computation. But that is not an argument to
 improve this.

-- 
Ticket URL: <http://trac.sagemath.org/sage_trac/ticket/9407#comment:4>
Sage <http://www.sagemath.org>
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