東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back to Search results for [ null ]

Switch To: Labeled | MARC Mode | ISBD

Exploring the String Landscape: The ...

Ahlqvist, Stein Pontus.

Linked to FindBook

Google Book

Amazon

博客來

Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds.

Record Type:	Language materials, printed : Monograph/item
Title/Author:	Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds./
Author:	Ahlqvist, Stein Pontus.
Description:	187 p.
Notes:	Source: Dissertation Abstracts International, Volume: 74-05(E), Section: B.
Contained By:	Dissertation Abstracts International74-05B(E).
Subject:	Physics, General. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3548129
ISBN:	9781267833587

Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds.
Ahlqvist, Stein Pontus.

Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds. - 187 p.

Source: Dissertation Abstracts International, Volume: 74-05(E), Section: B.

Thesis (Ph.D.)--Columbia University, 2013.

This dissertation explores various facets of the low-energy solutions in string theory known as the string landscape. Three separate questions are addressed -- the tunneling dynamics between these vacua, the statistics of their location in moduli space, and the potential realization of slow-roll inflation in the flux potentials generated in string theory. We find that the tunneling transitions that occur between a certain class of supersymmetric vacua related to each other via monodromies around the conifold point are sensitive to the details of warping in the near-conifold regime. We also study the impact of warping on the distribution of vacua near the conifold and determine that while previous work has concluded that the conifold point acts as an accumulation point for vacua, warping highly dilutes the distribution in precisely this regime. Finally we investigate a novel form of inflation dubbed spiral inflation to see if it can be realized near the conifold point. We conclude that for our particular models, spiral inflation seems to rely on a de Sitter-like vacuum energy. As a result, whenever spiral inflation is realized, the inflation is actually driven by a vacuum energy.

ISBN: 9781267833587Subjects--Topical Terms:

1018488
Physics, General.

Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds.
LDR:02078nam a2200277 4500 001 1965391
005 20141022133322.5
008 150210s2013 ||||||||||||||||| ||eng d
020 $a 9781267833587
035 $a (MiAaPQ)AAI3548129
035 $a AAI3548129
040 $a MiAaPQ $c MiAaPQ
100 1 $a Ahlqvist, Stein Pontus. $3 2102043
245 1 0 $a Exploring the String Landscape: The Dynamics, Statistics, and Cosmology of Parallel Worlds.
300 $a 187 p.
500 $a Source: Dissertation Abstracts International, Volume: 74-05(E), Section: B.
500 $a Adviser: Brian Greene.
502 $a Thesis (Ph.D.)--Columbia University, 2013.
520 $a This dissertation explores various facets of the low-energy solutions in string theory known as the string landscape. Three separate questions are addressed -- the tunneling dynamics between these vacua, the statistics of their location in moduli space, and the potential realization of slow-roll inflation in the flux potentials generated in string theory. We find that the tunneling transitions that occur between a certain class of supersymmetric vacua related to each other via monodromies around the conifold point are sensitive to the details of warping in the near-conifold regime. We also study the impact of warping on the distribution of vacua near the conifold and determine that while previous work has concluded that the conifold point acts as an accumulation point for vacua, warping highly dilutes the distribution in precisely this regime. Finally we investigate a novel form of inflation dubbed spiral inflation to see if it can be realized near the conifold point. We conclude that for our particular models, spiral inflation seems to rely on a de Sitter-like vacuum energy. As a result, whenever spiral inflation is realized, the inflation is actually driven by a vacuum energy.
590 $a School code: 0054.
650 4 $a Physics, General. $3 1018488
650 4 $a Physics, Astrophysics. $3 1671120
690 $a 0605
690 $a 0596
710 2 $a Columbia University. $b Physics. $3 2101563
773 0 $t Dissertation Abstracts International $g 74-05B(E).
790 $a 0054
791 $a Ph.D.
792 $a 2013
793 $a English
856 4 0 $u http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3548129