PIRSA:11090082
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
What Dark Matter Microhalos Can Tell us About Reheating Speaker(s): Adrienne Erickcek
Abstract: The expansion history of the Universe before big bang nucleosynthesis is unknown; in many models, the Universe was effectively matter-dominated between the end of inflation and the onset of radiation domination. I will show how an early matter-dominated era leaves an imprint on the small-scale matte... read more
Date: 22/09/2011 - 4:20 pm
Collection: Unravelling Dark Matter Conference
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PIRSA:10040078
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Generation of Perturbations During Inflation Speaker(s): Adrienne Erickcek
Abstract:
Date: 20/04/2010 - 12:00 pm
Collection: Cosmology Mini Course
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PIRSA:10040076
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Cosmological Perturbation Theory Speaker(s): Adrienne Erickcek
Abstract:
Date: 15/04/2010 - 4:00 pm
Collection: Cosmology Mini Course
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PIRSA:10040075
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Review of FRW Spacetime and Inflation Speaker(s): Adrienne Erickcek
Abstract:
Date: 13/04/2010 - 12:00 pm
Collection: Cosmology Mini Course
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PIRSA:08120031
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Inflationary Origins of the Cosmic Power Asymmetry Speaker(s): Adrienne Erickcek
Abstract: WMAP measurements of CMB temperature anisotropies reveal a power asymmetry: the average amplitude of temperature fluctuations in one hemisphere is larger than the average amplitude in the opposite hemisphere at the 99% confidence level. This power asymmetry may be generated during inflation by a lar... read more
Date: 09/12/2008 - 4:00 pm
Collection: Young Researchers Conference 2008
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PIRSA:08100031
( Flash Presentation , Windows Presentation , Windows Video File , MP3 , PDF) Which Format?
Structure Beyond the Horizon: Inflationary Origins of the Cosmic Power Asymmetry Speaker(s): Adrienne Erickcek
Abstract: WMAP measurements of CMB temperature anisotropies reveal a power asymmetry: the average amplitude of temperature fluctuations in one hemisphere is larger than the average amplitude in the opposite hemisphere at the 99% confidence level. This power asymmetry may be generated during inflation by a lar... read more
Date: 14/10/2008 - 4:00 pm
Series: Cosmology & Gravitation
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