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18 results with keyword: 'binary neutron star mergers gravitational wave era'

Binary neutron star mergers in the gravitational wave era

After the first direct observations of gravitational waves generated by the coales- cence of binary black hole systems, expectations about the possibility to reveal binary neutron

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2021
Source redshifts from gravitational-wave observations of binary neutron star mergers

However, a degeneracy in the information carried by gravitational waves between the total rest-frame mass M and the redshift z of the source implies that neither can be

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2021
Distinguishing Binary Neutron Star from Neutron Star–Black Hole Mergers with Gravitational Waves

Moreover, we obtain an unbiased radius estimate event for A = 30% as our approach is based on identifying radius outliers; any potentially misidentified NSBH will have an

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2021
Computational Methods for Gravitational Wave Physics: Spectral Cauchy Characteristic Extraction and Tidal Splicing

Gravitational waveforms for neutron star binaries from binary black hole simulations... Tidal effects in binary neutron

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2020
Analysis of Gravitational-Wave Signals from Binary Neutron Star Mergers Using Machine Learning

If the input was changed to be (n-1)-dimensional, the same hidden-layer could be used, as its size does not depend on the data or output. Therefore, when designing a

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2021
Neutron Star–Black Hole Mergers from Gravitational-wave Captures

( 2019a ) performed a study of com- pact binary mergers in GN induced by EKL, con- sidering different binary parameter distributions and SMBH masses, and found a NSBH merger rate

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Localization of binary neutron star mergers with second and third generation gravitational-wave detectors

Target noise curves for existing and future detectors [65] : advanced LIGO at design sensitivity (aLIGO); LIGO Voyager; Einstein Telescope (two proposed configurations, ET-B and

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2021
Reverse shocks in the relativistic outflows of gravitational wave-detected neutron star binary mergers

Phenomenologically, these two cases appear similar; the smooth change in the energy and Lorentz factor profile means that, overall, afterglow emission is brighter for longer and

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2021
Modeling the Complete Gravitational Wave Spectrum of Neutron Star Mergers

Postmerger spectra are characterized by a main peak frequency f 2 related to the particular structure and dynamics of the remnant hot hypermassive neutron star.. This observation

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2021
Binary Neutron Star Mergers

The effects of binary eccentricity on NS-NS mergers was recently studied by the Jena group [ 122 ]. Such systems, which would indicate dynamical formation processes rather than

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2021
Tidal deformations of compact objects and gravitational wave emission

As GW170817 has already shown [8, 19–25], gravitational wave detections from coalescing binary neutron star systems will provide information on neutron star matter complementary to

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2021
Multimessenger Probes of High-energy Sources

The merger of binary black holes, binary neutron stars or black hole-neutron star binaries are abundant gravitational wave sources and will likely make up the majority of

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Low mass binary neutron star mergers: Gravitational waves and neutrino emission

These outflows are expected to produce a wide range of elements through r-process nucleosynthesis, as their prop- erties are right at the limit between neutron-rich material

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The detection and parameter estimation of binary black hole mergers

Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals.. Abbott

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Outcome of r-mode Instability on Hypercritically Accreting Neutron Stars Shin'ichirou Yoshida yλ and Yoshiharu Eriguchi z y SISSA, International Schoo

neutron star in an X-ray binary system emits gravitational wave so as to balance the. accretion torque with the gravitational radiation torque of the

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PROPERTIES OF BINARY NEUTRON STARS AS GRAVITATIONAL WAVE SOURCES

PROPERTIES OF BINARY NEUTRON STARS AS GRAVITATIONAL WAVE SOURCES.. Tauris

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2022
Inferring the Post-Merger Gravitational Wave Emission from Binary Neutron Star Coalscences

These plots demonstrate how Bayeswave is capable of reconstructing the dominant features of the injected sig- nal, including the dominant post-merger frequency with only

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Gravitational waves and mass ejecta from binary neutron star mergers: Effect of large eccentricities

(Middle and right panels): The energy estimate computed accounting for displacement- induced mode mixing for the nonspinning SLy and MS1b cases that have multiple encounters

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