Prospects for Primordial Gravitational Waves in String Inflation

Autor: Ivonne Zavala, Susha L. Parameswaran
Jazyk: angličtina
Rok vydání: 2016
Předmět:
High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
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FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
Astrophysics::Cosmology and Extragalactic Astrophysics
String theory
01 natural sciences
String (physics)
Upper and lower bounds
General Relativity and Quantum Cosmology
Moduli
Theoretical physics
High Energy Physics - Phenomenology (hep-ph)
0103 physical sciences
Effective field theory
010306 general physics
Mathematical Physics
media_common
Physics
Inflation (cosmology)
010308 nuclear & particles physics
Gravitational wave
Astronomy and Astrophysics
Universe
High Energy Physics - Phenomenology
High Energy Physics - Theory (hep-th)
Space and Planetary Science
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: International Journal of Modern Physics D
Popis: Assuming that the early universe had (i) a description using perturbative string theory and its field theory limit (ii) an epoch of slow-roll inflation within a four-dimensional effective field theory and a hierarchy of scales $M_{inf} < m_{kk} < m_s \lesssim M_{pl}$ that keeps the latter under control, we derive an upper bound on the amplitude of primordial gravitational waves. The bound is very sensitive to mild changes in numerical coefficients and the expansion parameters. For example, allowing couplings and mass-squared hierarchies $\lesssim 0.2$, implies $r \lesssim 0.05$, but asking more safely for hierarchies $\lesssim 0.1$, the bound becomes $r \lesssim 10^{-6}$. Moreover, large volumes -- typically used in string models to keep backreaction and moduli stabilisation under control -- drive $r$ down. Consequently, any detection of inflationary gravitational waves would present an interesting but difficult challenge for string theory.
Received Honourable Mention in the 2016 Gravity Research Foundation Awards for Essays on Gravitation; submitted to IJMPD Special issue with some revisions and clarifications, 3 pages + refs; v2 further clarifications
Databáze: OpenAIRE