neutron star merger
Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
... binary neutron star ...the merger of this binary was also recorded by the Fermi Gamma-ray Burst Monitor ( Fermi-GBM ) , and the Anti-Coincidence Shield for the Spectrometer for the International ...
18
Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger
... after merger. Neutrino observations associated with a binary neutron-star merger using the unique characteristics in SK would validate such proposed mechan- ...the merger time and in a ...
7
Properties of the Binary Neutron Star Merger GW170817
... CAASTROs, DFN, DES, INTEGRAL, Virgo, Insight- HXMT, MAXI Team, J-GEM, RATIR, ATLAS, IceCube, LWA, ePESSTO, GRAWITA, RIMAS, SKA South Africa/ MeerKAT, H.E.S.S., Fermi Large Area Telescope, 1M2H Team, IKI-GW Follow-up, ...
32
Compact radio emission indicates a structured jet was produced by a binary neutron star merger
... binary neutron star merger, detected through both electromagnetic radiation and gravitational waves on the 17 th of August 2017, raised the question whether a narrow relativistic jet or a more ...
21
Properties of the binary neutron star merger GW170817
... CAASTROs, DFN, DES, INTEGRAL, Virgo, Insight- HXMT, MAXI Team, J-GEM, RATIR, ATLAS, IceCube, LWA, ePESSTO, GRAWITA, RIMAS, SKA South Africa/ MeerKAT, H.E.S.S., Fermi Large Area Telescope, 1M2H Team, IKI-GW Follow-up, ...
32
Multi messenger observations of a binary neutron star merger
... Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight- Hxmt Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM ...
60
Search for Gravitational Waves from a Long lived Remnant of the Binary Neutron Star Merger GW170817
... binary neutron star coalescence GW170817 is the nature of its post- merger ...possible neutron star remnant with a maximum signal duration of 500 ...the neutron star ...
31
A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
... We estimate the event rate density (or the volumetric rate) of CDF-S XT2-like events to be 1.3 +2.8 −1.1 × 10 4 Gpc −3 yr −1 , taking into account a number of factors that include, e.g., the event searching procedure, ...
29
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
... BNS merger, but even without the connection to GW170817, the spectrum of GRB 170817A in the GBM data strongly disfavored the BB fi t expected for a giant magnetar fl ...
27
Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
... post- merger searches because the highest signal amplitudes are emitted in the early, high-frequency part of the spin-down, where the detectors are currently much less sensitive than around a few hundred ...post- ...
19
Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817
... the merger until the of fi cial end of the LIGO-Virgo second observing ...post- merger signal, though the expected rapid decrease in frequency is likely to pose technical challenges to current ...
13
Multi-messenger Observations of a Binary Neutron Star Merger
... of neutron stars with other neutron stars or with black ...and star-forming galaxies ( Barthelmy et ...by neutron star mergers remained elusive, and interest intensi fi ed in following ...
59
What can neutron stars reveal about the equation of state of dense matter?
... Abstract. Neutron stars are astrophysical objects of extremes, reaching the highest den- sities we can observe in the cosmos, and probing matter under conditions that cannot be recreated in terrestrial ...first ...
6
r Process Nucleosynthesis in Neutron Star Mergers with the New Nuclear Reaction Network SkyNet
... of star formation in our galaxy. Furthermore, neutron star mergers are rare events that release r-process material and that material has to mix with the interstellar medium in the galaxy before it ...
343
The Dynamics of the Neutron Complexes: From Neutron Star to Black Hole
... of neutron complexes, including a large number of neutrons and having finite macroscopic dimensions, is ...that neutron complexes at the final stage of their development are neutron ...of ...
5
Formation and Evolution of Neutron Star Binaries: Masses of Neutron Stars
... In astrophysical side, there are many recent developments on gamma-ray bursts (GRB) and gravi- tational wave radiation. There are two classes of GRBs, long-duration GRB (τ > 2 sec) and short-hard GRB (SHB, τ < 2 ...
6
An Accretion Model for Anomalous X‐Ray Pulsars
... the neutron star following its ...the neutron star towards a “tracking” solution in which the rotation period of the star increases slowly, in tandem with the declining accretion ...
18
Statistical Study of Neutron Star Glitches
... the known glitches. This is inevitable due to increase observation of active pulsars and the use of more sensitive instruments than in past. Within this time scale, the youthful pulsars still dominate the glitch events. ...
6
Probing neutron star physics using accreting neutron stars
... accreting neutron stars systems as probes of neutron star ...accreting neutron stars during ...these neutron stars do not show evidence of spin variations during the ...accreting ...
34
r-process observations
... heavy neutron-capture elements in very metal-poor stars provide unique constraint on the r-process ...of neutron-capture elements could be a result of a single ...
6