Results 81 to 90 of about 910,791 (369)
Is GW190425 Consistent with Being a Neutron Star–Black Hole Merger? [PDF]
GW190425 is the second neutron star merger event detected by the Advanced LIGO/Virgo detectors. If interpreted as a double neutron star merger, the total gravitational mass is substantially larger than that of the binary systems identified in the Galaxy.
Ming-Zhe Han+7 more
semanticscholar +1 more source
Gravitational waves from neutron star binary inspirals contain information on strongly interacting matter in unexplored, extreme regimes. Extracting this requires robust theoretical models of the signatures of matter in the gravitational-wave signals due
Jan Steinhoff+3 more
doaj +1 more source
High-Frequency QPOs as a Product of Inner Disk Dynamics around Neutron Stars
The kHz QPOs observed in a neutron star low mass X-ray binary are likely to be produced in the innermost regions of accretion disk around the neutron star.
Erkut, M. H.
core +1 more source
Neutrostriction in Neutron Stars [PDF]
It is demonstrated that not only gravity, but also neutrostriction forces due to optical potential created by coherent elastic neutron-neutron scattering can hold a neutron star together. The latter forces can be stronger than gravitational ones. The effect of these forces on mass, radius and structure of the neutron star is estimated.
openaire +3 more sources
Deep crustal heating by neutrinos from the surface of accreting neutron stars
We present a new mechanism for deep crustal heating in accreting neutron stars. Charged pions ($\pi^+$) are produced in nuclear collisions on the neutron star surface during active accretion and upon decay they provide a flux of neutrinos into the ...
Brown, Edward F.+6 more
core +1 more source
On magnetized neutron stars [PDF]
6 Figures + Appendix.
Débora P. Menezes+2 more
openaire +3 more sources
Double and single recycled pulsars: an evolutionary puzzle? [PDF]
We investigate the statistics of isolated recycled pulsars and double neutron star binaries in the Galactic disk. Since recycled pulsars are believed to form through accretion and spinup in close binaries, the isolated objects presumably originate from ...
Abbott+83 more
core +3 more sources
This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.
Mallory S. E. Roberts+2 more
openaire +2 more sources
This article investigates residual stress formation during single‐spot nanosecond laser ablation of stainless steel. Experimental validation and a parametric study using finite element simulations are employed to analyze thermal effects, ablation dynamics, and stress evolution.
Yutaka Tsumura+7 more
wiley +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