Sifting the gravitational-wave Universe via multimessenger astronomy: Forthcoming prospects for continuous-wave detection

Leaci, Paola (2017) Sifting the gravitational-wave Universe via multimessenger astronomy: Forthcoming prospects for continuous-wave detection. Il nuovo cimento C, 40 (3). pp. 1-5. ISSN 1826-9885

[img]
Preview
Text
ncc11445.pdf - Published Version

Download (92kB) | Preview
Official URL: https://www.sif.it/riviste/sif/ncc/econtents/2017/...

Abstract

The upgrade of worldwide gravitational-wave detector network has led to the first transient gravitational-wave detection, which has started to hone the comprehension we have about our Universe and some of its constituents. A broader picture would be however provided by the detection of continuous-wave signals, which could be more easily achieved by exploiting the synergy with multimessenger Astronomy. Thanks to electromagnetic observations we may indeed be able to know, with enough accuracy, the sky location, rotational and/or orbital parameters of a broad class of rapidly-rotating neutron stars. This would allow us to perform a multitude of targeted and directed continuous-wave searches, and would facilitate narrow-band searches for the same class of signals. We will describe the prospects for detecting continuous gravitational waves, by especially employing novel strategies for neutron stars in binary systems directed to sources whose parameters have been electromagnetically estimated. Employing those methods to analyze data from the ever-more-sensitive advanced detectors will remarkably increase the chances of a continuous-wave detection.

Item Type: Article
Subjects: 500 Scienze naturali e Matematica > 530 Fisica
Depositing User: Marina Spanti
Date Deposited: 17 Nov 2020 09:55
Last Modified: 17 Nov 2020 09:55
URI: http://eprints.bice.rm.cnr.it/id/eprint/19959

Actions (login required)

View Item View Item