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The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO framework (Zero Angular Momentum Observers) has been formulated.
Atsnaita Yasrina +3 more
doaj +1 more source
Accretion dynamics in neutron star black hole binaries
We perform three-dimensional, Newtonian hydrodynamic simulations with a nuclear equation of state to investigate the accretion dynamics in neutron star black hole systems.
Balsara +37 more
core +2 more sources
Can we distinguish low mass black holes in neutron star binaries?
The detection of gravitational waves from coalescing binary neutron stars represents another milestone in gravitational-wave astronomy. However, since LIGO is currently not as sensitive to the merger/ringdown part of the waveform, the possibility that ...
East, William E. +2 more
core +1 more source
Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers [PDF]
Banafsheh Shiralilou +6 more
openalex +1 more source
Signatures for quark matter from multi-messenger observations
We review the prospects for detecting quark matter in neutron star cores. We survey the proposed signatures and emphasize the importance of data from neutron star mergers, which provide access to dynamical properties that operate on short timescales that
Alford, Mark G. +2 more
core +1 more source
Neutron stars with submillisecond periods: a population of high mass objects? [PDF]
Fast spinning neutron stars, recycled in low mass binaries, may have accreted a substantial amount of mass. The available relativistic measurements of neutron star masses, all clustering around 1.4 M_sun, however refer mostly to slowly rotating neutron ...
Burderi, Luciano +4 more
core +3 more sources
Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models [PDF]
Chun Huang +4 more
openalex +1 more source
Anisotropic magnetized neutron star
As we know, the effect of strong magnetic field causes the anisotropy for the magnetized compact objects. Therefore, in this paper, we have studied the structure properties of anisotropic case of magnetized neutron star.
Gholam Hossein Bordbar, Mohammad Karami
doaj +1 more source
Neutrino Annihilation between Binary Neutron Stars
We calculate the neutrino pair annihilation rate into electron pairs between two neutron stars in a binary system. We present a closed formula for the energy deposition rate at any point between the stars, where each neutrino of a pair derives from each ...
Salmonson, Jay D., Wilson, James R.
core +1 more source
Neutron stars change their structure with accumulation of dark matter. We study how their mass is influenced from the environment. Close to the sun, the dark matter accretion from the neutron star does not have any effect on it.
Antonino Del Popolo +2 more
doaj +1 more source

