How a RandallSundrum BraneWorld Effective Potential Influences Inflation Physics
Abstract
In string theory, even when there are ten to the thousand power vacuum states, does inflation produce overwhelmingly one preferred type of vacuum state? We respond affirmatively to questions whether existence of graviton production is confirmable using present detector methodology. We use an explicit RandallSundrum braneworld effective potential as congruent with an inflationary quadratic potential start. This occurs after Bogomolnyi inequality eliminates need for ad hoc assumption of axion wall mass high temperature related disappearing. Graviton production has explicit links with a fivedimensional braneworld negative cosmological constant and a fourdimensional positive valued cosmological constant, whose temperature dependence permits an early universe graviton production activity burst. We show how di quarks, wave functions, and various forms tie into the WheelerDe Witt equation. This permits investigating a discretized quantum bounce and a possible link to the initial phases of present universe's evolution with a prior universe's collapse to the bounce pointthe initial starting point to inflationary expansion. This opens a possibility of realistically investigating gravitons as part of a space propulsion system and dealing with problems from a beam of gravity waves, which would create a gforce because the geodestic structure is near field. It can be applied to existing and tomore »
 Authors:
 APS/Contractor, Fermi National Laboratory, Menlo Park, CA 94025 (United States)
 Publication Date:
 OSTI Identifier:
 21054534
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: AIP Conference Proceedings; Journal Volume: 880; Journal Issue: 1; Conference: International forumSTAIF 2007: 11. conference on thermophysics applications in microgravity; 24. symposium on space nuclear power and propulsion; 5. conference on human/robotic technology and the vision for space exploration; 5. symposium on space colonization; 4. symposium on new frontiers and future concepts, Albuquerque, NM (United States), 1115 Feb 2007; Other Information: DOI: 10.1063/1.2437564; (c) 2007 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; AXIONS; BRANES; COSMOLOGICAL CONSTANT; COSMOLOGY; FOURDIMENSIONAL CALCULATIONS; GRAVITONS; GRAVITY WAVES; PARTICLE PRODUCTION; POTENTIALS; PROPULSION SYSTEMS; QUARKS; SPACE; STRING MODELS; STRING THEORY; TEMPERATURE DEPENDENCE; UNIVERSE; VACUUM STATES; WAVE FUNCTIONS
Citation Formats
Beckwith, A. W. How a RandallSundrum BraneWorld Effective Potential Influences Inflation Physics. United States: N. p., 2007.
Web. doi:10.1063/1.2437564.
Beckwith, A. W. How a RandallSundrum BraneWorld Effective Potential Influences Inflation Physics. United States. doi:10.1063/1.2437564.
Beckwith, A. W. Tue .
"How a RandallSundrum BraneWorld Effective Potential Influences Inflation Physics". United States.
doi:10.1063/1.2437564.
@article{osti_21054534,
title = {How a RandallSundrum BraneWorld Effective Potential Influences Inflation Physics},
author = {Beckwith, A. W.},
abstractNote = {In string theory, even when there are ten to the thousand power vacuum states, does inflation produce overwhelmingly one preferred type of vacuum state? We respond affirmatively to questions whether existence of graviton production is confirmable using present detector methodology. We use an explicit RandallSundrum braneworld effective potential as congruent with an inflationary quadratic potential start. This occurs after Bogomolnyi inequality eliminates need for ad hoc assumption of axion wall mass high temperature related disappearing. Graviton production has explicit links with a fivedimensional braneworld negative cosmological constant and a fourdimensional positive valued cosmological constant, whose temperature dependence permits an early universe graviton production activity burst. We show how di quarks, wave functions, and various forms tie into the WheelerDe Witt equation. This permits investigating a discretized quantum bounce and a possible link to the initial phases of present universe's evolution with a prior universe's collapse to the bounce pointthe initial starting point to inflationary expansion. This opens a possibility of realistically investigating gravitons as part of a space propulsion system and dealing with problems from a beam of gravity waves, which would create a gforce because the geodestic structure is near field. It can be applied to existing and to new space propulsion concepts.},
doi = {10.1063/1.2437564},
journal = {AIP Conference Proceedings},
number = 1,
volume = 880,
place = {United States},
year = {Tue Jan 30 00:00:00 EST 2007},
month = {Tue Jan 30 00:00:00 EST 2007}
}

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