Two years of work in the J0737-3039 laboratory

Possenti, A, Burgay, M, D'Amico, N, Lyne, A, Kramer, M, McLaughlin, M, Lorimer, D, Manchester, D, Camilo, F, Sarkissian, J, Freire, P, Joshi, BC, Stairs, IH and Ferdman, R ORCID: https://orcid.org/0000-0002-2223-1235 (2005) Two years of work in the J0737-3039 laboratory. In: Astrophysical sources of high-energy particles and radiation: Proceedings, Torun, Poland, 20-24 June 2005. AIP Conference Proceedings . American Institute of Physics, POL, pp. 272-277.

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Abstract

We report on the results achieved in the first two years of observations of the double-pulsar system J0737-3039A/B. Its orbital parameters and close distance allow to perform unprecedented tests of the theories of Gravity and of the physics of highly condensed matter. The discovery of this system enhances of about an order of magnitude the estimate of the merger rate of double neutron stars systems, opening new possibilities for the current generation of gravitational wave detectors. The high orbital inclination offers the opportunity of using the radio beams from one of the two sources as a probe for studying the magnetosphere of the other.

Item Type:	Book Section
Faculty \ School:	Faculty of Science > School of Chemistry (former - to 2024)
UEA Research Groups:	Faculty of Science > Research Groups > Quantum Matter Faculty of Science > Research Groups > Numerical Simulation, Statistics & Data Science
Depositing User:	LivePure Connector
Date Deposited:	12 Jul 2018 10:30
Last Modified:	07 Nov 2024 12:49
URI:	https://ueaeprints.uea.ac.uk/id/eprint/67596
DOI:

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