PIRSA:11070017
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Scale Invariance from Spontaneous Breaking of Conformal Symmetry Speaker(s): Justin Khoury
Abstract: I will discuss a novel framework of the very early universe which addresses the traditional horizon and flatness problems of big bang cosmology and predicts a scale invariant spectrum of perturbations. Unlike
inflation, this scenario requires no exponential superluminal expansion of
space-time... read more
Date: 14/07/2011 - 9:50 am
Collection: Challenges for Early Universe Cosmology
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PIRSA:09050080
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Cascading Gravity and the Cosmological Constant Speaker(s): Justin Khoury
Abstract: TBA
Date: 26/05/2009 - 11:30 am
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PIRSA:08070007
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Chameleon Theories Speaker(s): Justin Khoury
Abstract:
Date: 14/07/2008 - 12:00 pm
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PIRSA:07090025
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Degravitating The Vacuum Speaker(s): Justin Khoury
Abstract:
Date: 11/09/2007 - 11:00 am
Collection: Frontiers of Modern Cosmology
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PIRSA:06070021
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Keynote Presentation - How the universe began Speaker(s): Justin Khoury
Abstract:
Date: 11/07/2006 - 10:35 pm
Collection: Einstein Plus 2006
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PIRSA:06060025
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Cosmology 7 Speaker(s): Justin Khoury
Abstract:
Date: 09/06/2006 - 12:00 pm
Collection: Theory Canada 2
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PIRSA:05030105
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Chameleon Scalar Fields: Detecting Dark Energy with Tests of Gravity Speaker(s): Justin Khoury
Abstract: Chameleon scalar fields are candidates for the dark energy, the mysterious component causing the observed acceleration of the universe. Their defining property is a mass which depends on the local matter density: they are massive on Earth, where the density is high, but essentially massless in the c... read more
Date: 10/03/2005 - 4:00 pm
Series: Cosmology & Gravitation
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