The force-free magnetosphere of a rotating black hole
... developed a few years earlier by [15]. [21] realized that many astrophysicists feel uncomfortable in curved spacetime (sic) and rewrote black hole electrodynamics in an absolute-space/universal-time formulation with the hope that it may catalyze pulsar-experienced astrophysicists to begin research i ...
... developed a few years earlier by [15]. [21] realized that many astrophysicists feel uncomfortable in curved spacetime (sic) and rewrote black hole electrodynamics in an absolute-space/universal-time formulation with the hope that it may catalyze pulsar-experienced astrophysicists to begin research i ...
Lecture 12
... We will see in next lectures what the implications of this are for other phenomena in the Universe. It actually led to the discovery of dark energy! The collapse of massive stars produces two types of remnants - neutron stars and black holes. Their masses have been measured in X-ray emitting binary ...
... We will see in next lectures what the implications of this are for other phenomena in the Universe. It actually led to the discovery of dark energy! The collapse of massive stars produces two types of remnants - neutron stars and black holes. Their masses have been measured in X-ray emitting binary ...
Neutron Stars and Black Holes
... ____ 28. Pulsars could not be pulsating stars because the pulses are too short. ____ 29. We expect neutron stars to spin rapidly because they conserve angular momentum. ____ 30. Many pulsars have periods that are gradually increasing as the spinning neutron stars lose energy. ____ 31. The event hori ...
... ____ 28. Pulsars could not be pulsating stars because the pulses are too short. ____ 29. We expect neutron stars to spin rapidly because they conserve angular momentum. ____ 30. Many pulsars have periods that are gradually increasing as the spinning neutron stars lose energy. ____ 31. The event hori ...
