Results 121 to 130 of about 50,134 (242)
12 pages, 5 figures, reviewed by SCIENCE CHINA Physics, Mechanics & Astronomy (SCPMA)
Jin, Hong-Bo, Qiao, Cong-Feng
openaire +2 more sources
The Japanese space gravitational wave antenna; DECIGO [PDF]
DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. DECIGO is expected to open a new window of observation for gravitational wave astronomy especially between 0.1 Hz and 10 Hz ...
Agatsuma, Kazuhiro +134 more
core
Optical detector topology for third-generation gravitational wave observatories [PDF]
Andreas Freise +6 more
openalex +1 more source
Probing intermediate scale Froggatt-Nielsen models at future gravitational wave observatories [PDF]
Dhruv Ringe
openalex +1 more source
Precision Timing of PSR J0437–4715 with the IAR Observatory and Implications for Low-frequency Gravitational Wave Source Sensitivity [PDF]
Michael T. Lam, Jeffrey S. Hazboun
openalex +1 more source
We explore the potential of lunar-based gravitational-wave detectors to broaden the multimessenger astrophysics landscape by detecting mergers of massive ( M _1 , M _2 > 1 M _⊙ ) double white dwarf (WD) binaries. These systems are potential progenitors
Manuel Pichardo Marcano +2 more
doaj +1 more source
Impact of galactic foreground characterization on a global analysis for the LISA gravitational wave observatory [PDF]
Travis Robson, Neil Cornish
openalex +1 more source
Search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar [PDF]
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasinormal mode oscillations in their parent neutron star that couple to gravitational-wave emission. In August 2006, a timing glitch was observed in the radio emission
Abadie, J. +24 more
core +1 more source
New Primordial-Magnetic-Field Limit from The Latest LIGO S5 data
Since the energy momentum tensor of a magnetic field always contains a spin-2 component in its anisotropic stress, stochastic primordial magnetic field (PMF) in the early universe must generate stochastic gravitational wave (GW) background.
L. P. Grishchuk, S. Wang
core +1 more source
Searches for continuous-wave gravitational radiation in data collected by modern long-baseline interferometers, such as the Laser Interferometer Gravitational-wave Observatory (LIGO), the Virgo interferometer, and the Kamioka Gravitational Wave Detector,
P. Clearwater +3 more
doaj +1 more source

