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Limits on Primordial Black Hole evaporation with the H.E.S.S. array of Cherenkov telescopes

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arxiv 1307.4898 v1 pith:KDXVEB55 submitted 2013-07-18 astro-ph.HE

J-F.Glicenstein (1) , A.Barnacka (2) , M.Vivier (1) , T.Herr (3) (for the H.E.S.S. Collaboration) ((1) CEA Saclay , DSM/Irfu , Gif-Sur-Yvette Cedex , France , (2) Nicolaus Copernicus Astronomical Center
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ul. Bartycka Warsaw Poland (3) Max-Planck-Institut für Kernphysik Heidelberg Germany)
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keywords beenlimitsarrayblackburstburstsexplosionshole
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abstract

Data collected by the H.E.S.S. array between 2004 and 2012 have been used to search for photon bursts from primordial black hole explosions. Bursts were searched for in a 30 second time-window. The duration of the search window has been optimized to increase the burst signal while keeping the statistical background low. No evidence for a burst signal was found. Preliminary upper limits on the local rate of PBH explosions of $1.4\times 10^{4} {pc}^{-3} {yr}^{-1}$ have been obtained, which improve previously published limits by almost an order of magnitude

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. VERITAS Observations of Fast Radio Bursts

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    VERITAS found no gamma-ray or optical emission from 15 contemporaneous bursts of FRB 121102 or from the second repeater FRB 180814.J0422+73, setting new 95% upper limits.

  2. Neutrinos from Primordial Black Hole Evaporation

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    The adapted IceCube search is most sensitive to the final 10^3 seconds of PBH evaporation, with a local burst rate sensitivity of 3.8 million per cubic parsec per year.

  3. Constraining the evaporation rate of primordial black holes using archival data from VERITAS

    astro-ph.HE 2019-09 unverdicted novelty 2.0 of 10

    A VERITAS work-in-progress report projects that 2,100 hours of archival data will tighten the primordial black hole evaporation rate-density upper limit by about a factor of two, down to roughly 10^4 pc^-3 yr^-1.

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