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Exploring the early universe with gr...
~
Bethke, Laura Bianca.
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Exploring the early universe with gravitational waves
Record Type:
Electronic resources : Monograph/item
Title/Author:
Exploring the early universe with gravitational waves/ by Laura Bianca Bethke.
Author:
Bethke, Laura Bianca.
Published:
Cham :Springer International Publishing : : 2015.,
Description:
xiii, 139 p. :ill., digital ;24 cm.
[NT 15003449]:
Introduction -- Chiral Tensor Power Spectrum from Quantum Gravity -- Anisotropic Gravitational Wave Background from Massless Pre-heating -- Concluding Remarks -- Appendix.
Contained By:
Springer eBooks
Subject:
Gravitational waves. -
Online resource:
http://dx.doi.org/10.1007/978-3-319-17449-5
ISBN:
9783319174495 (electronic bk.)
Exploring the early universe with gravitational waves
Bethke, Laura Bianca.
Exploring the early universe with gravitational waves
[electronic resource] /by Laura Bianca Bethke. - Cham :Springer International Publishing :2015. - xiii, 139 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- Chiral Tensor Power Spectrum from Quantum Gravity -- Anisotropic Gravitational Wave Background from Massless Pre-heating -- Concluding Remarks -- Appendix.
This work investigates gravitational wave production in the early universe and identifies potentially observable features, thereby paving the way for future gravitational wave experiments. It focuses on gravitational wave production in two scenarios: inflation in a model inspired by loop quantum gravity, and preheating at the end of inflation. In the first part, it is demonstrated that gravitational waves' spectrum differs from the result obtained using ordinary general relativity, with potentially observable consequences that could yield insights into quantum gravity. In the second part, it is shown that the cosmic gravitational wave background is anisotropic at a level that could be detected by future experiments. Gravitational waves promise to be an rich source of information on the early universe. To them, the universe has been transparent from its earliest moments, so they can give us an unobstructed view of the Big Bang and a means to probe the fundamental laws of nature at very high energies.
ISBN: 9783319174495 (electronic bk.)
Standard No.: 10.1007/978-3-319-17449-5doiSubjects--Topical Terms:
805566
Gravitational waves.
LC Class. No.: QC179
Dewey Class. No.: 539.754
Exploring the early universe with gravitational waves
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Introduction -- Chiral Tensor Power Spectrum from Quantum Gravity -- Anisotropic Gravitational Wave Background from Massless Pre-heating -- Concluding Remarks -- Appendix.
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This work investigates gravitational wave production in the early universe and identifies potentially observable features, thereby paving the way for future gravitational wave experiments. It focuses on gravitational wave production in two scenarios: inflation in a model inspired by loop quantum gravity, and preheating at the end of inflation. In the first part, it is demonstrated that gravitational waves' spectrum differs from the result obtained using ordinary general relativity, with potentially observable consequences that could yield insights into quantum gravity. In the second part, it is shown that the cosmic gravitational wave background is anisotropic at a level that could be detected by future experiments. Gravitational waves promise to be an rich source of information on the early universe. To them, the universe has been transparent from its earliest moments, so they can give us an unobstructed view of the Big Bang and a means to probe the fundamental laws of nature at very high energies.
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Physics and Astronomy (Springer-11651)
based on 0 review(s)
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電子資源
11.線上閱覽_V
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EB QC179
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