EPJ Web of Conferences
Volume 121, 2016Roma International Conference on Astroparticle Physics 2014 (RICAP-14)
|Number of page(s)||7|
|Published online||06 July 2016|
Gravitational waves and multimessenger astronomy
1 Dipartimento di Fisica, Università di Roma La Sapienza, Italy
2 INFN Sezione di Roma, Rome, Italy
a e-mail: firstname.lastname@example.org
Published online: 6 July 2016
It is widely expected that in the coming quinquennium the first gravitational wave signal will be directly detected. The ground-based advanced LIGO and Virgo detectors are being upgraded to a sensitivity level such that we expect to be measure a significant binary merger rate. Gravitational waves events are likely to be accompanied by electromagnetic counterparts and neutrino emission carrying complementary information to those associated to the gravitational signals. If it becomes possible to measure all these forms of radiation in concert, we will end up an impressive increase in the comprehension of the whole phenomenon. In the following we summarize the scientific outcome of the interferometric detectors in the past configuration. Then we focus on some of the potentialities of the advanced detectors once used in the new context of the multimessenger astronomy.
© The Authors, published by EDP Sciences
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
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