Changes between Version 1 and Version 2 of Talks/Falll2011/SpecialSeminars/111110a


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Timestamp:
11/07/11 18:23:47 (15 years ago)
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jules@…
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  • Talks/Falll2011/SpecialSeminars/111110a

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    1 I'll present results of numerical simulations of post-supernova hypercritical (i.e. highly super-Eddington) accretion onto a new-born magnetized neutron star. The purpose of these is to study whether such accretion is able to submerge the magnetic field and produce a non-magnetized star. CCO may be candidate for such demagnetized neutron stars.
     1Dany Page (UNAM)
     2
     3Do Supernovae Make or Kill Pulsars?
     4
     5I'll present results of numerical simulations of post-supernova hypercritical (i.e. highly super-Eddington) accretion onto a new-born magnetized neutron star. The purpose of these is to study whether such accretion is able to submerge the magnetic field and produce a non-magnetized star. CCOs may be candidates for such demagnetized neutron stars.