Rheology and electric field response of fumed nanoparticles in nematic liquid crystal suspensions

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dc.contributor.author Kumar, Saket
dc.contributor.author Thareja, Prachi
dc.contributor.other Annual European Rheology Conference (AERC-2018)
dc.coverage.spatial Hilton Sorrento Palace, Sorrento, IT
dc.date.accessioned 2018-05-15T10:39:53Z
dc.date.available 2018-05-15T10:39:53Z
dc.date.issued 2018-04-17
dc.identifier.citation Kumar, Saket and Thareja, Prachi, "Rheology and electric field response of fumed nanoparticles in nematic liquid crystal suspensions", in the Annual European Rheology Conference (AERC-2018), Hilton Sorrento Palace, Sorrento, IT, Apr. 17-20, 2018. en_US
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/3659
dc.description.abstract We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and 90% credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5- 20 deg2 requires at least three detectors of sensitivity within a factor of ?2 of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.
dc.description.statementofresponsibility by Saket Kumar and Prachi Thareja
dc.language.iso en en_US
dc.subject Gravitational waves en_US
dc.subject Gravitational-wave detectors en_US
dc.subject Electromagnetic counterparts en_US
dc.subject Data analysis en_US
dc.title Rheology and electric field response of fumed nanoparticles in nematic liquid crystal suspensions en_US
dc.type Article en_US

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