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Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum (Record no. 48006)

MARC details
000 -LEADER
fixed length control field 03479nam a22005417a 4500
001 - CONTROL NUMBER
control field sulb-eb0025914
003 - CONTROL NUMBER IDENTIFIER
control field BD-SySUS
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20160413122554.0
007 - PHYSICAL DESCRIPTION FIXED FIELD--GENERAL INFORMATION
fixed length control field cr nn 008mamaa
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 130710s2013 ja | s |||| 0|eng d
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9784431541806
-- 978-4-431-54180-6
024 7# - OTHER STANDARD IDENTIFIER
Standard number or code 10.1007/978-4-431-54180-6
Source of number or code doi
050 #4 - LIBRARY OF CONGRESS CALL NUMBER
Classification number QB1-991
Classification number QB460-466
Classification number QB980-991
072 #7 - SUBJECT CATEGORY CODE
Subject category code PGC
Source bicssc
Subject category code SCI004000
Source bisacsh
Subject category code SCI005000
Source bisacsh
082 04 - DEWEY DECIMAL CLASSIFICATION NUMBER
Classification number 520
Edition number 23
100 1# - MAIN ENTRY--PERSONAL NAME
Personal name Shiraishi, Maresuke.
Relator term author.
245 10 - TITLE STATEMENT
Title Probing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum
Medium [electronic resource] /
Statement of responsibility, etc. by Maresuke Shiraishi.
264 #1 - PRODUCTION, PUBLICATION, DISTRIBUTION, MANUFACTURE, AND COPYRIGHT NOTICE
Place of production, publication, distribution, manufacture Tokyo :
Name of producer, publisher, distributor, manufacturer Springer Japan :
-- Imprint: Springer,
Date of production, publication, distribution, manufacture, or copyright notice 2013.
300 ## - PHYSICAL DESCRIPTION
Extent XIII, 180 p.
Other physical details online resource.
336 ## - CONTENT TYPE
Content type term text
Content type code txt
Source rdacontent
337 ## - MEDIA TYPE
Media type term computer
Media type code c
Source rdamedia
338 ## - CARRIER TYPE
Carrier type term online resource
Carrier type code cr
Source rdacarrier
347 ## - DIGITAL FILE CHARACTERISTICS
File type text file
Encoding format PDF
Source rda
490 1# - SERIES STATEMENT
Series statement Springer Theses, Recognizing Outstanding Ph.D. Research,
International Standard Serial Number 2190-5053
505 0# - FORMATTED CONTENTS NOTE
Formatted contents note Introduction -- Fluctuations in the inflation -- Fluctuations in cosmic microwave background radiation -- Primordial non-Gaussianities -- General formalism for the CMB bispectrum from primordial scalar, vector and tensor non-Gaussianities -- CMB bispectrum Induced by the two scalars and a graviton correlator -- Violation of the rotational invariance in the CMB bispectrum -- Parity violation of gravitons in the CMB bispectrum -- CMB bispectrum generated from primordial magnetic fields -- Conclusion.
520 ## - SUMMARY, ETC.
Summary, etc. The non-Gaussianity in the primordial density fluctuations is a key feature to clarify the early Universe and it has been probed with the Cosmic Microwave Background (CMB) bispectrum. In recent years, we have treated the novel-type CMB bispectra, which originate from the vector- and tensor-mode perturbations and include the violation of the rotational or parity invariance. On the basis of our current works, this thesis provides the general formalism for the CMB bispectrum sourced by the non-Gaussianity in the scalar, vector and tensor-mode perturbations. Applying this formalism, we calculate the CMB bispectra from the two scalars and a graviton correlation and primordial magnetic fields, and then outline new constraints on these magnitudes. Furthermore, this formalism can be easily extended to the cases where the rotational or parity invariance is broken. We also compute the CMB bispectra from the scalar-mode non-Gaussianities with a preferred direction and the tensor-mode non-Gaussianities induced by the parity-violating Weyl cubic terms. Here, we show that these bispectra include unique signals, which any symmetry-invariant models can never produce.
650 #0 - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name as entry element Physics.
Topical term or geographic name as entry element Mathematical physics.
Topical term or geographic name as entry element Astronomy.
Topical term or geographic name as entry element Astrophysics.
Topical term or geographic name as entry element Cosmology.
Topical term or geographic name as entry element Physics.
Topical term or geographic name as entry element Astronomy, Astrophysics and Cosmology.
Topical term or geographic name as entry element Mathematical Methods in Physics.
Topical term or geographic name as entry element Mathematical Physics.
710 2# - ADDED ENTRY--CORPORATE NAME
Corporate name or jurisdiction name as entry element SpringerLink (Online service)
773 0# - HOST ITEM ENTRY
Title Springer eBooks
776 08 - ADDITIONAL PHYSICAL FORM ENTRY
Relationship information Printed edition:
International Standard Book Number 9784431541790
830 #0 - SERIES ADDED ENTRY--UNIFORM TITLE
Uniform title Springer Theses, Recognizing Outstanding Ph.D. Research,
International Standard Serial Number 2190-5053
856 40 - ELECTRONIC LOCATION AND ACCESS
Uniform Resource Identifier <a href="http://dx.doi.org/10.1007/978-4-431-54180-6">http://dx.doi.org/10.1007/978-4-431-54180-6</a>
912 ## -
-- ZDB-2-PHA
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Source of classification or shelving scheme
Koha item type

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