All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Search for High-energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F18%3A00329968" target="_blank" >RIV/68407700:21670/18:00329968 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1134/S0021364018240025" target="_blank" >http://dx.doi.org/10.1134/S0021364018240025</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1134/S0021364018240025" target="_blank" >10.1134/S0021364018240025</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Search for High-energy Neutrinos from GW170817 with the Baikal-GVD Neutrino Telescope

  • Original language description

    The Advanced Laser Interferometer Gravitational-Wave Observatory and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst that followed the merger of this binary was also recorded by Fermi gamma-ray burst monitor and International Gamma-Ray Astrophysics Laboratory, indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the TeV – 100 PeV energy range using Baikal Gigaton Volume Detector. No neutrinos directionally coincident with the source were detected within ±500 s around the merger time, as well as during a 14-day period after the gravitational wave detection. We derived 90% confidence level upper limits on the neutrino fluence from GW170817 during a ±500 s window centered on the gravitational wave trigger time, and a 14-day window following the gravitational wave signal under the assumption of an E-2 neutrino energy spectrum.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>ost</sub> - Miscellaneous article in a specialist periodical

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/EF16_019%2F0000766" target="_blank" >EF16_019/0000766: Engineering applications of microworld physics</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2018

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Journal of Experimental and Theoretical Physics Letters

  • ISSN

    0021-3640

  • e-ISSN

    1090-6487

  • Volume of the periodical

    108

  • Issue of the periodical within the volume

    12

  • Country of publishing house

    RU - RUSSIAN FEDERATION

  • Number of pages

    4

  • Pages from-to

    787-790

  • UT code for WoS article

  • EID of the result in the Scopus database