Published November 29, 2006
| Version v1
Journal article
Relic Gravitons In The Context Of String Theory
Creators
- 1. Institute of Space Studies of Catalonia (IEEC-CSIC), Sciences Faculty, Tower C5-Even, 2nd floor, North Access, Bellaterra, Barcelona (Spain)
Description
The emission of gravitational waves by multiple phenomena of astrophysical, cosmological and fundamental physics origin is predicted not only in Einstein's General Relativity Theory, but also in other theories of gravity. In this contribution we will sketch the main ideas and steps underlying the computation of primordial gravitational backgrounds arising from more general gravitational theories. We then apply it to obtain the graviton production in different transition epochs of the universe evolution, with gravity described by the Low Order String Effective Action. Finally, we end up pointing out the main characteristics and detection perspectives of the spectra
Additional details
Identifiers
- DOI
- 10.1063/1.2405027;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 873
- Journal Issue
- 1
- Journal Page Range
- p. 99-104
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 6. international LISA (Laser Interferometer Space Antenna) symposium
- Dates
- 19-23 Jun 2006
- Place
- Greenbelt, MD (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38058701
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACTION INTEGRAL; CALCULATION METHODS; GALACTIC EVOLUTION; GENERAL RELATIVITY THEORY; GRAVITATION; GRAVITATIONAL WAVES; GRAVITONS; STRING MODELS; UNIVERSE
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; EVOLUTION; EXTENDED PARTICLE MODEL; FIELD THEORIES; GRAVITATIONAL RADIATION; INTEGRALS; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; POSTULATED PARTICLES; QUARK MODEL; RADIATIONS; RELATIVITY THEORY
Optional Information
- Notes
- (c) 2006 American Institute of Physics