Talk:Cosmic inflation: Difference between revisions

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==Working notes==
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===Vacuum energy===
*[http://math.ucr.edu/home/baez/vacuum.html What's the Energy Density of the Vacuum?] John Baez (2006) UC Riverside
*[http://www.astro.ucla.edu/~wright/cosmo_constant.html Vacuum Energy Density, or How Can Nothing Weigh Something?] Edward Wright (2006) UCLA Division of Astronomy and Astrophysics
*[http://www.space.com/scienceastronomy/generalscience/darkenergy_folo_010410.html Astrophysics Challenged By Dark Energy Finding] Ray Villard (2001) Space.com
*[http://focus.aps.org/story/v10/st7 Deflating Vacuum Energy] JR Minkel (2002). Focus Physical Review
*[http://arXiv.org/abs/hep-th/0007146 Cosmological Breaking of Supersymmetry?] T. Banks (2000) UC Santa Cruz and Rutgers. arXiv:hep-th/0007146v1
*[http://www.nasa.gov/centers/glenn/research/warp/possible.html#vac Vacuum Fluctuations of Quantum Physics] Kathleen Zona (2007) Glenn Research Center, NASA
*[http://arxiv.org/abs/hep-th/0012062 Vacuum energy] Mark D. Roberts (2001)  arXiv:hep-th/0012062v3

Latest revision as of 18:40, 27 March 2008

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 Definition:  Theorized exponential expansion of the universe at the end of the grand unification epoch, 10−36 seconds after the Big Bang, driven by a negative-pressure vacuum energy density. [d] [e]
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Vacuum energy

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