Abstract
Cosmic string cusps are sources of short-lived, linearly polarised gravitational wave bursts which can be searched for in gravitational wave detectors. We assess the capability of LISA to detect these bursts using the latest LISA configuration and operational assumptions. For such short bursts, we verify that LISA can be considered...
Description
Keywords
LISA , Cosmology and Nongalactic Astrophysics (astro-ph.CO) , string tension , gravitational radiation , 500 , FOS: Physical sciences , General Relativity and Quantum Cosmology (gr-qc) , 530 , gravitational radiation detector , General Relativity and Quantum Cosmology , supernova remnant , High Energy Physics - Phenomenology , High Energy Physics - Phenomenology (hep-ph) , cosmic string, network , [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] , network , [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc] , cosmic string , [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] , burst , gravitational radiation, burst , Astrophysics - Cosmology and Nongalactic Astrophysics