Edge Rewrite
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a25dcab14d8db965

Jump to content

Golden binary

From Wikipedia, the free encyclopedia

Gravitational wave signal GW250114, the clearest gravitational wave signal discovered as of 2025.

In gravitational wave astronomy, a golden binary is a binary black hole collision event whose inspiral and ringdown phases have been measured accurately enough to provide separate measurements of the initial and final black hole masses.[1][2]

Testing general relativity

[edit source]

Current LIGO/Virgo protocol relies on its library of several hundred thousand precomputed templates of black hole collisions conceivably detectable in their frequency range. A putative binary black hole collision signal consists of inspiral, merger, and ringdown phases. The complete signal is compared with the template library, and event parameters and significance are based on an analysis of such matches.

This allows for self-consistency checks of general relativity. In order to test certain competing theories of gravity, one faces the problem that only general relativity has been studied enough that the complete merger phase is known. Therefore, only a signal that can be matched separately in the inspiral and ringdown phases can be used to allow or contradict such theories.

Identified golden binaries

[edit source]

GW150914 was a golden binary, indeed, this led to additional internal checks done by LIGO.[3][4] GW151226 and LVT151012 were not.[4]

References

[edit source]
  1. Hughes, Scott A; Menou, Kristen (2005). "Golden Binary Gravitational-Wave Sources: Robust Probes of Strong-Field Gravity". The Astrophysical Journal. 623 (2): 689–699. arXiv:astro-ph/0410148. Bibcode:2005ApJ...623..689H. doi:10.1086/428826. S2CID 18971575.
  2. Nakano, Hiroyuki; Tanaka, Takahiro; Nakamura, Takashi (2015). "Possible golden events for ringdown gravitational waves". Physical Review D. 92 (6) 064003. arXiv:1506.00560. Bibcode:2015PhRvD..92f4003N. doi:10.1103/PhysRevD.92.064003. S2CID 85464193.
  3. Ghosh, Abhirup; Ghosh, Archisman; Johnson-Mcdaniel, Nathan K; Mishra, Chandra Kant; Ajith, Parameswaran; Del Pozzo, Walter; Nichols, David A; Chen, Yanbei; Nielsen, Alex B; Berry, Christopher P L; London, Lionel (2016). "Testing general relativity using golden black-hole binaries". Physical Review D. 94 (2) 021101. arXiv:1602.02453. Bibcode:2016PhRvD..94b1101G. doi:10.1103/PhysRevD.94.021101. S2CID 4688859.
  4. 1 2 Berry, Christopher P L (27 August 2016). "Testing general relativity using golden black-hole binaries". Retrieved 19 October 2017.