Gravitational waves as tracers of nuclear equation of state

Cabezon, Ruben M. and Garcia-Senz, Domingo. (2007) Gravitational waves as tracers of nuclear equation of state. In: Supernovae: lights in the darkness.

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The signal of neutron star (NS) mergers has the imprint of the EOS of dense nuclear matter, which is still not well known. A set of gravitational waves (GW) signals have been calculated from 3D hydrodynamical simulations of NS-NS mergers using the Smoothed Particle Hydrodynamics technique (SPH) with different EOS. By analyzing the morphology and time evolution of the signal we want to be able to discriminate among the variety of proposed EOS after a successful GW detection has been done.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
10 Zentrale universitäre Einrichtungen > sciCORE
UniBasel Contributors:Cabezon, Ruben M.
Item Type:Conference or Workshop Item, refereed
Conference or workshop item Subtype:Conference Paper
Publisher:Proceedings of Science
Series Name:Trobades Científiques de la Mediterrània
Issue Number:23
Note:Publication type according to Uni Basel Research Database: Conference paper
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Last Modified:09 Oct 2019 15:47
Deposited On:09 Oct 2019 15:47

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