Early Direct Detection of Gravity Waves

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dc.creatorFakir, Redouane
dc.date1993-09-21
dc.date.accessioned2026-07-07T03:30:08Z
dc.date.available2026-07-07T03:30:08Z
dc.descriptionRecently, the possibility has emerged of an early detection of astrophysical gravity waves. In certain astronomical configurations, and through a new light-deflection effect, gravity waves can cause apparent shifts in stellar angular positions as large as $10^{-7}arcsec$. In these same configurations, the magnitude of the gravity-wave-induced time-delay effect can exceed $10^{-14}$. Both these figures lie just at present-day theoretical limits of detectability. For instance, cases are described where the very faint neutron-star gravity waves could soon become detectable. The detection meant here involves direct observations of the very wave-forms.
dc.descriptionplain LaTeX, 11p, UBCTP-93-016
dc.identifierhttps://arxiv.org/abs/gr-qc/9309021
dc.identifierhttp://arxiv.org/abs/gr-qc/9309021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35440
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleEarly Direct Detection of Gravity Waves
dc.typetext

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