A non radially oscillating star emits gravitational waves at frequencies and with damping times that depend on the equation of state of matter and on the dynamical processes that occur in the interior. In this talk we will discuss how the high density behaviour of matter affects the oscillation frequencies of neutron stars in different phases of their life.
Imprint of the equation of state of dense matter on gravitational waves emitted by oscillating neutron stars / Ferrari, Valeria. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6588. - 8:(2005), pp. 58-70. (Intervento presentato al convegno 11th Conference on Recent Development in Gravity tenutosi a Lesvos, GREECE nel JUN 02-05, 2004) [10.1088/1742-6596/8/1/008].
Imprint of the equation of state of dense matter on gravitational waves emitted by oscillating neutron stars
FERRARI, Valeria
2005
Abstract
A non radially oscillating star emits gravitational waves at frequencies and with damping times that depend on the equation of state of matter and on the dynamical processes that occur in the interior. In this talk we will discuss how the high density behaviour of matter affects the oscillation frequencies of neutron stars in different phases of their life.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
