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Search for events in XENON1T associated with gravitational waves

Aprile, E. (author)
Antochi, Vasile Cristian, 1992- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Conrad, Jan, 1973- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Rosso, Andrea Gallo, 1991- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Joy, Ashley, 1988- (author)
Stockholms universitet,Oskar Klein-centrum för kosmopartikelfysik (OKC),Fysikum
Mahlstedt, Jörn, 1985- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Tan, Pueh-Leng, 1990- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Zhu, T. (author)
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 (creator_code:org_t)
2023
2023
English.
In: Physical Review D. - 2470-0010 .- 2470-0029. ; 108:7
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We perform a blind search for particle signals in the XENON1T dark matter detector that occur close in time to gravitational-wave signals in the LIGO and Virgo observatories. No particle signal is observed in the nuclear recoil and electronic recoil channels within ±500 seconds of observations of the gravitational-wave signals GW170104, GW170729, GW170817, GW170818, and GW170823. We use this null result to constrain monoenergetic neutrinos and axion-like particles emitted in the closest coalescence GW170817, a binary neutron star merger. We set new upper limits on the fluence (time-integrated flux) of coincident neutrinos down to 17 keV at the 90% confidence level. Furthermore, we constrain the product of the coincident fluence and cross section of axion-like particles to be less than 10−29  cm2/cm2 in the [5.5–210] keV energy range at the 90% confidence level.

Subject headings

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)

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