Coalescing binary systems of compact objects to(post)52-Newtonian order. IV. The gravitational wave tail

1993 ◽  
Vol 48 (10) ◽  
pp. 4757-4770 ◽  
Author(s):  
Alan G. Wiseman
Keyword(s):  
Gravitational Wave ◽  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

Innermost stable orbits for coalescing binary systems of compact objects

1992 ◽  
Vol 9 (9) ◽  
pp. L125-L131 ◽  
Author(s):  
L E Kidder ◽  
C M Will ◽  
A G Wiseman
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

Coalescing Binary Systems of Compact Objects to (Post)5/2-Newtonian Order

1991 ◽  
Vol 631 (1 Nonlinear Pro) ◽  
pp. 126-136 ◽  
Author(s):  
CLIFFORD M. WILL ◽  
CRAIG W. LINCOLN ◽  
ALAN G. WISEMAN
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

scholarly journals Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

2020 ◽  
Vol 23 (1) ◽  
Author(s):  
B. P. Abbott ◽  
◽  
R. Abbott ◽  
T. D. Abbott ◽  
S. Abraham ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Gravitational Wave ◽  
Binary Systems ◽  
Compact Objects ◽  
Binary Neutron Star ◽  
Binary Black Hole ◽  
Credible Region ◽  
Binary Mergers ◽  
Black Hole Binary

AbstractWe present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of providing information to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals for the third (O3), fourth (O4) and fifth observing (O5) runs, including the planned upgrades of the Advanced LIGO and Advanced Virgo detectors. We study the capability of the network to determine the sky location of the source for gravitational-wave signals from the inspiral of binary systems of compact objects, that is binary neutron star, neutron star–black hole, and binary black hole systems. The ability to localize the sources is given as a sky-area probability, luminosity distance, and comoving volume. The median sky localization area (90% credible region) is expected to be a few hundreds of square degrees for all types of binary systems during O3 with the Advanced LIGO and Virgo (HLV) network. The median sky localization area will improve to a few tens of square degrees during O4 with the Advanced LIGO, Virgo, and KAGRA (HLVK) network. During O3, the median localization volume (90% credible region) is expected to be on the order of $$10^{5}, 10^{6}, 10^{7}\mathrm {\ Mpc}^3$$ 10 5 , 10 6 , 10 7 Mpc 3 for binary neutron star, neutron star–black hole, and binary black hole systems, respectively. The localization volume in O4 is expected to be about a factor two smaller than in O3. We predict a detection count of $$1^{+12}_{-1}$$ 1 - 1 + 12 ($$10^{+52}_{-10}$$ 10 - 10 + 52 ) for binary neutron star mergers, of $$0^{+19}_{-0}$$ 0 - 0 + 19 ($$1^{+91}_{-1}$$ 1 - 1 + 91 ) for neutron star–black hole mergers, and $$17^{+22}_{-11}$$ 17 - 11 + 22 ($$79^{+89}_{-44}$$ 79 - 44 + 89 ) for binary black hole mergers in a one-calendar-year observing run of the HLV network during O3 (HLVK network during O4). We evaluate sensitivity and localization expectations for unmodeled signal searches, including the search for intermediate mass black hole binary mergers.

scholarly journals Coalescing Binary Systems of Compact Objects: Dynamics of Angular Momenta

1998 ◽  
Vol 507 (1) ◽  
pp. 287-299 ◽  
Author(s):  
Carlo Del Noce ◽  
Giovanni Preti ◽  
Fernando de Felice
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Angular Momenta ◽  
Coalescing Binary Systems

Coalescing binary systems of compact objects to(post)52-Newtonian order. III. Transition from inspiral to plunge

1993 ◽  
Vol 47 (8) ◽  
pp. 3281-3291 ◽  
Author(s):  
Lawrence E. Kidder ◽  
Clifford M. Will ◽  
Alan G. Wiseman
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

Dynamic matched filter technique for gravitational wave detection from coalescing binary systems

2004 ◽  
Vol 21 (5) ◽  
pp. S807-S810 ◽  
Author(s):  
F Acernese ◽  
F Barone ◽  
R De Rosa ◽  
A Eleuteri ◽  
S Pardi ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Binary Systems ◽  
Matched Filter ◽  
Gravitational Wave Detection ◽  
Filter Technique ◽  
Wave Detection ◽  
Coalescing Binary Systems
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