Search for multi-messenger sources of gravitational waves and high-energy neutrinos with Advanced LIGO during its first observing Run, ANTARES and IceCube

Show simple item record

dc.contributor.author Sengupta, Anand
dc.date.accessioned 2018-11-16T06:05:54Z
dc.date.available 2018-11-16T06:05:54Z
dc.date.issued 2018-08
dc.identifier.citation Sengupta, Anand et al., "Search for multi-messenger sources of gravitational waves and high-energy neutrinos with Advanced LIGO during its first observing Run, ANTARES and IceCube", arXiv, Cornell University Library, DOI: arXiv:1810.10693, Aug. 2018. en_US
dc.identifier.uri http://arxiv.org/abs/1810.10693
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/3998
dc.description.abstract Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origin could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational wave and neutrino emission processes.
dc.description.statementofresponsibility by Anand Sengupta et al.
dc.language.iso en en_US
dc.publisher Cornell University Library en_US
dc.subject High Energy Astrophysical en_US
dc.subject Phenomena en_US
dc.subject Astrophysics en_US
dc.title Search for multi-messenger sources of gravitational waves and high-energy neutrinos with Advanced LIGO during its first observing Run, ANTARES and IceCube en_US
dc.type Preprint en_US


Files in this item

Files Size Format View

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record

Search Digital Repository


Browse

My Account