Changes between Version 1 and Version 2 of Talks/Falll2011/SpecialSeminars/111110a
- Timestamp:
- 11/07/11 18:23:47 (15 years ago)
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Talks/Falll2011/SpecialSeminars/111110a
v1 v2 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. 1 Dany Page (UNAM) 2 3 Do Supernovae Make or Kill Pulsars? 4 5 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. CCOs may be candidates for such demagnetized neutron stars.
