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Gravitational Wave Sources from New Physics

2006/01/01 by Craig J. Hogan · 5 citations
Physics and Astronomy · #Broadband #COSMIC cancer database #Cosmology #Cosmology and Gravitation Theories #Gravitation #Gravitational wave #Gravitational-wave astronomy #Mesoscopic physics #Pulsars and Gravitational Waves Research #Quantum and Classical Electrodynamics #Range (aeronautics) #astro-ph

paper · pdf · doi:10.1063/1.2405019

published as AIPConf.Proc.873:30-40,2006 · 11 pages, Latex, 4 figures, invited talk at Sixth International LISA Symposium

openalex publication_date 2006/01/01 · arxiv created 2006/08/25 · arxiv updated 2009/12/01 · openalex created_date 2019/06/27 · openalex updated_date 2026/08/05

Abstract

Forthcoming advances in direct gravitational wave detection from kilohertz to nanohertz frequencies have unique capabilities to detect signatures from or set meaningful constraints on a wide range of new cosmological phenomena and new fundamental physics. A brief survey is presented of the post‐inflationary gravitational radiation backgrounds predicted in cosmologies that include intense new classical sources such as first‐order phase transitions, late‐ending inflation, and dynamically active mesoscopic extra dimensions. LISA will provide the most sensitive direct probes of such phenomena near TeV energies or Terascale. LISA will also deeply probe the broadband background, and possibly bursts, from loops of cosmic superstrings predicted to form in current models of brane inflation.

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