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MG12 - Talk detail
 

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 Participant 

Watts, Anna

Institution

Astronomical Institute "Anton Pannekoek", University of Amsterdam  - PO Box 94249 - Amsterdam - - Netherland

Session

Talk

Abstract

APT2

Gravitational waves from neutron stars

Direct detection of gravitational waves (GWs) from neutron stars will eventually enable completely new studies of dense matter composition and dynamics. I will summarize our current understanding of gravitational wave generation mechanisms in neutron stars, as constrained by both theory and electromagnetic astronomy. I will discuss what we can hope to learn from GW observations, how they will complement traditional astronomical methods, and review prospects for direct and indirect detection of GWs.

GW1

X-Ray Inputs into Gravitational Wave Science

Input from X-ray astronomy is critical to gravitational wave searches, providing (for example) trigger times for burst searches and ephemerides for continuous wave searches. Even in cases where it cannot supply a precise signal template, X-ray astronomy can provide constraints on gravitational wave generation mechanisms. I will review the prospects for interaction between these two fields in the light of current and planned X-ray missions.

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