Cosmology I
ORAL · X11 ·
Presentations
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Dark energy is the cosmological quantum vacuum energy of light particles. The axion and the lightest neutrino.
ORAL
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Authors
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H.J. de Vega
- LPTHE/CNRS/Univ Paris VI-VII
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Systematic Corrections to the Deceleration Parameter due to Local Cosmological Inhomogeneity
ORAL
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Authors
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Ali Vanderveld
- Cornell University
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Ira Wasserman
- Cornell University, Ithaca, NY
- Cornell University
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Eanna Flanagan
- Cornell University
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Locally inhomogeneous cosmology as a possible explanation of dark energy
ORAL
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Authors
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Xinghai Zhao
- University of Notre Dame
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Grant Mathews
- University of Notre Dame
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In-Saeng Suh
- University of Notre Dame
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James Wilson
- LLNL
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Structure Formation Limits on f(R) Gravity
ORAL
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Authors
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David Bernat
- Cornell University
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Rachel Bean
- Cornell University
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Levon Pegosian
- Simon Fraser University
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Alessandra Silvestri
- Syracuse University
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Mark Trodden
- Syracuse University
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Some exact solutions exhibiting inflation and dark energy
ORAL
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Authors
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Chris Vuille
- Embry-Riddle Aeronautical University
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Primordial Black Hole Minimum Mass
ORAL
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Authors
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James Chisholm
- University of Florida
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Nucleosynthesis in plasma-redshift cosmology
ORAL
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Authors
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Ari Brynjolfsson
- Applied Radiation Industries
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How can Brane World physics influence Axion temperature dependence, initial vacuum states, and permissible solutions to the Wheeler-De Witt equation?
ORAL
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Authors
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Andrew Beckwith
- APS/ Fermi contractor
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What is Fine-Structure Constant?
ORAL
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Authors
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Shantilal Goradia
- Gravity Research Institute, Inc.
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