Results 1 to 10 of about 492,459 (298)

Transmuted gravity wave signals from primordial black holes

open access: yesPhysics Letters B, 2018
Primordial black holes (PBHs) interacting with stars in binaries lead to a new class of gravity wave signatures that we explore. A small 10−16–10−7M⊙ PBH captured by a neutron star or a white dwarf will eventually consume the host.
Volodymyr Takhistov
doaj   +4 more sources

Neutron Star Mergers and the Quark Matter Equation of State [PDF]

open access: yesEPJ Web of Conferences, 2022
As neutron stars merge they can approach very high nuclear density. Here, we summarized recent results for the evolution and gravitational wave emission from binary-neutron star mergers using a a variety of nuclear equations of state with and without a ...
Mathews Grant J.   +3 more
doaj   +1 more source

Detection and parameter estimation of gravitational waves from binary neutron-star mergers in real LIGO data using deep learning

open access: yesPhysics Letters B, 2021
One of the key challenges of real-time detection and parameter estimation of gravitational waves from compact binary mergers is the computational cost of conventional matched-filtering and Bayesian inference approaches.
Plamen G. Krastev   +3 more
doaj   +1 more source

Boson Stars as Solitary Waves [PDF]

open access: yesCommunications in Mathematical Physics, 2007
Communications in Mathematical Physics, 274 (1)
Fröhlich, Jürg   +2 more
openaire   +6 more sources

NEARBY STARS AS GRAVITATIONAL WAVE DETECTORS [PDF]

open access: yesThe Astrophysical Journal, 2015
Sun-like stellar oscillations are excited by turbulent convection and have been discovered in some 500 main sequence and sub-giant stars and in more than 12,000 red giant stars. When such stars are near gravitational wave sources, low-order quadrupole acoustic modes are also excited above the experimental threshold of detectability, and they can be ...
Lopes, Ilídio, Silk, Joseph
openaire   +2 more sources

Real-time detection of gravitational waves from binary neutron stars using artificial neural networks

open access: yesPhysics Letters B, 2020
The groundbreaking discoveries of gravitational waves from binary black-hole mergers [1–3] and, most recently, coalescing neutron stars [4] started a new era of Multi-Messenger Astrophysics and revolutionized our understanding of the Cosmos.
Plamen G. Krastev
doaj   +1 more source

Wave chaos in rapidly rotating stars [PDF]

open access: yesPhysical Review E, 2008
Effects of rapid stellar rotation on acoustic oscillation modes are poorly understood. We study the dynamics of acoustic rays in rotating polytropic stars and show using quantum chaos concepts that the eigenfrequency spectrum is a superposition of regular frequency patterns and an irregular frequency subset respectively associated with near-integrable ...
Lignieres, F., Georgeot, Bertrand
openaire   +4 more sources

Photons generated by gravitational waves in the near-zone of a neutron star

open access: yesNuclear Physics B, 2022
When a gravitational wave or a graviton travels through an electric or magnetic background, it could convert into a photon with some probability. In this paper, a dipole magnetic field is considered as this kind of background in both the Minkowski ...
Chao-Jun Feng   +3 more
doaj   +1 more source

Monster Radiative Shocks in the Perturbed Magnetospheres of Neutron Stars

open access: yesThe Astrophysical Journal, 2023
Magnetospheres of neutron stars can be perturbed by star quakes, interaction in a binary system, or sudden collapse of the star. The perturbations are typically in the kilohertz band and excite magnetohydrodynamic waves.
Andrei M. Beloborodov
doaj   +1 more source

Optical detection of the density-wave instability in the kagome metal KV3Sb5

open access: yesnpj Quantum Materials, 2022
Coexisting density-wave and superconducting states along with the large anomalous Hall effect in the absence of local magnetism remain intriguing and enigmatic features of the AV3Sb5 kagome metals (A = K, Rb, Cs).
Ece Uykur   +4 more
doaj   +1 more source

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