Suggested Topics within your search.
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Neutron stars
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Stars
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Neutrons
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Stars: neutrons
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stars: neutron
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Physics
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Research & information: general
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gravitational waves
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Gravitational effects
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Gravitational-waves
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Gravity waves
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Mergers and acquisitions
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Neutron star merger
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neutron star mergers
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Black holes
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Merging
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Pulsars
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X-rays: Binaries
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Binary neutron stars
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Equations of state
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Astronomy, space & time
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Cosmology
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Equation-of-state
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Galaxies
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Method: numerical
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Numerical methods
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Pulsars: general
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R-process
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801“... the Sun, the Earth, or neutron stars. There, they can become non-extremal either from merging...”
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802“... neutron stars endowed with an ultra-strong magnetic field ( B ≈ 10 14 – 10 15 G...”
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803“... might potentially happen in the atmosphere of white dwarfs, neutron stars or even that of stellar...”
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804
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805“... binaries or, in one case, from coalescing neutron stars. These observations opened up the era...”
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806by Masaomi Tanaka“... of two neutron stars or a neutron star and a black hole). Kilonova/macronova is emission powered...”
Published 2016-01-01
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807
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808by Pallanca, Cristina <1985>“...Millisecond Pulsars (MSPs) are fast rotating, highly magnetized neutron stars. According...”
Published 2014
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Doctoral Thesis -
809by Barnes, A.“..., the standard shocktube problem is used to test the code, and perturbed, rotating neutron stars are studied....”
Published 2004
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810by Contenta, Filippo“... the final star cluster properties, such as the neutron stars natal kick distribution. I conclude, through a...”
Published 2017
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811“... squared Gauss–Bonnet (GB) term, compact objects such as neutron stars and black holes (BHs) can...”
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812
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813
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814
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815“... sufficiently accelerated motion of charged stars (specially neutron stars) or charged stellar mass black holes...”
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816by H. Vargas-Rodríguez, A. Gallegos, M. A. Muñiz-Torres, H. C. Rosu, P. J. Domínguez“... are generalizations of the light cylinders found around magnetized neutron stars. In both cases, we give the explicit...”
Published 2020-01-01
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817“... with neutron stars and with black holes) for different parameters of the IMF - slopes: α = 1, α = 1.35 and α...”
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818“... birefringence of GWs. If a nearly edge-on binary neutron-stars with observed electromagnetic counterparts at 40...”
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819by Bell, Elizabeth“..., then the equilibrium ratio of protons to neutrons inside high density neutron stars can be inferred, allowing...”
Published 2005
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820by Charbonneau, Arthur James“... fields, dense matter, and parity violation. We propose that such a current exists in the cores of neutron...”
Published 2011
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