Volume rendering of the entropy distribution in a 3D magnetorotational core-collapse supernova simulation, about 200 ms after core bounce. (Msta et al., SXS Collaboration, read more and see Christian Ott's blog post) \"Race tracks\" followed by a pair of two unequal mass black holes with misaligned spins. The orbits are precessing. The two black holes have formed a common horizon, which is shown as a third surface around the two individucal horizons. (SXS Collaboration, learn more) 3D structure of the remnant accretion disk of a black-holeneutron-star merger color-coded for outgoing neutrino luminosity (Deaton et al., SXS Collaboration, read more) Volume rendering of the specific entropy distribution in a 3D GR core-collapse supernova simulation. The blue outer layer indicates the expanding shock front. (Ott et al. 2013, SXS Collaboration, read more) Black hole horizon appearing in a 3D full-GR simulation of the collapse of a very massive star by Ott et al. 2011 Read more Vertex and Tendex fields describing outgoing gravitational waves from a black hole horizon Read more Specific entropy distribution in the equatorial plane of a rapidly spinning, non-axisymmetric proto-neutron star, formed in a 3D GR collapse simulation by Ott et al. 2007 Read more Temperature and electron fraction (Y_e) in an accretion disk formed by the merger of a neutron-star and a black hole. (Deaton et al. 2013, SXS Collaboration, read more) Two black holes formed in the collapse and fragmentation of a cosmological supermassive star. (Reisswig et al. 2013, SXS Collaboration, read more) <\/p>\n<\/p>\n
TAPIR is part of the Division of Physics, Mathematics, and Astronomy at Caltech. We are located in the Cahill Center for Astronomy and Astrophysics. <\/p>\n
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TAPIR at Caltech<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" Volume rendering of the entropy distribution in a 3D magnetorotational core-collapse supernova simulation, about 200 ms after core bounce. (Msta et al., SXS Collaboration, read more and see Christian Ott's blog post) \"Race tracks\" followed by a pair of two unequal mass black holes with misaligned spins. Continue reading