Akif Baha Balantekin
(U.of Wisconsin)
29/06/2017, 11:25
Oral Presentation
Collective oscillations of neutrinos represent emergent nonlinear flavor evolution phenomena instigated by neutrino-neutrino interactions in astrophysical environments with sufficiently high neutrino densities. The symmetries of the problem in the full three flavor mixing scheme and in the exact many-body formulation by including the effects of CP violation and neutrino magnetic moment will be...
Meng-Ru Wu
29/06/2017, 11:50
Oral Presentation
The merger of binary neutron stars or a neutron star and a black hole can eject an amount of 0.001-0.1 solar mass of neutron-rich matter after the merger. The rapid neutron capture process (r-process) is expected to occur in these ejecta and may be responsible for the electromagnetic transient called kilonova or macronova, which is an important counterpart of the future gravitational wave...
Norhasliza Yusof
(U. of Malaysia)
29/06/2017, 12:15
Oral Presentation
In the work, we are going to discuss the stellar evolution of Very Massive Stars (M>100 Mo) in different metallicities. This includes the general properties, impact on the chemical abundances due to the rotational impact, dependences in metallicities and mass loss of very massive stars. Very massive stars has very large convective core during the main sequence thus their evolution do not...
