Cosmological Inflation, Dark Matter and Dark Energy
Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In additi...
Saved in:
: | |
---|---|
Year of Publication: | 2019 |
Language: | English |
Physical Description: | 1 electronic resource (236 p.) |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
id |
993548120304498 |
---|---|
ctrlnum |
(CKB)4100000010106253 (oapen)https://directory.doabooks.org/handle/20.500.12854/44151 (EXLCZ)994100000010106253 |
collection |
bib_alma |
record_format |
marc |
spelling |
Bamba, Kazuharu auth Cosmological Inflation, Dark Matter and Dark Energy MDPI - Multidisciplinary Digital Publishing Institute 2019 1 electronic resource (236 p.) text txt rdacontent computer c rdamedia online resource cr rdacarrier Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In addition, according to the rotation curve of galaxies, the existence of dark matter, which does not shine, is also suggested. If primordial gravitational waves are detected in the future, the mechanism for realizing inflation can be revealed. Moreover, there exist two main candidates for dark matter. The first is a new particle, the existence of which is predicted in particle physics. The second is an astrophysical object which is not found by electromagnetic waves. Furthermore, there are two representative approaches to account for the accelerated expansion of the current universe. One is to assume the unknown dark energy in general relativity. The other is to extend the gravity theory to large scales. Investigation of the origins of inflation, dark matter, and dark energy is one of the most fundamental problems in modern physics and cosmology. The purpose of this book is to explore the physics and cosmology of inflation, dark matter, and dark energy. English de Sitter vacuum Einstein-Aether theory of gravity Supernovae apparatus normal galaxies higher dimension gauged super-gravity black hole dark energy model cosmo-particle physics instruments Cosmic Microwave Background (CMB) temperature Dark Energy hyper-color quantum tunneling phenomenon spacetime symmetry parametrizations quantum gravity dynamical Chern-Simons modified gravity comparative planetology properties of specific particles particle physics dark matter Hawking radiation memory junction conditions cosmology composite dark matter dosmological parameters field theory Dark Matter cosmological model extragalactic objects and systems scalar-tensor gravity fundamental astronomy cosmoligical parameters cosmological parameters Baryon Acoustic Oscillation (BAO) dark atoms quantum optical systems brans-dicke theory dark energy models loop quantum cosmology dark energy galactic rotation curve astronomical and space-research instrumentation null hypersurfaces QCD quantum optics Hubble constant and components common to several branches of physics and astronomy statistical analysis 3-03921-764-X |
language |
English |
format |
eBook |
author |
Bamba, Kazuharu |
spellingShingle |
Bamba, Kazuharu Cosmological Inflation, Dark Matter and Dark Energy |
author_facet |
Bamba, Kazuharu |
author_variant |
k b kb |
author_sort |
Bamba, Kazuharu |
title |
Cosmological Inflation, Dark Matter and Dark Energy |
title_full |
Cosmological Inflation, Dark Matter and Dark Energy |
title_fullStr |
Cosmological Inflation, Dark Matter and Dark Energy |
title_full_unstemmed |
Cosmological Inflation, Dark Matter and Dark Energy |
title_auth |
Cosmological Inflation, Dark Matter and Dark Energy |
title_new |
Cosmological Inflation, Dark Matter and Dark Energy |
title_sort |
cosmological inflation, dark matter and dark energy |
publisher |
MDPI - Multidisciplinary Digital Publishing Institute |
publishDate |
2019 |
physical |
1 electronic resource (236 p.) |
isbn |
3-03921-765-8 3-03921-764-X |
illustrated |
Not Illustrated |
work_keys_str_mv |
AT bambakazuharu cosmologicalinflationdarkmatteranddarkenergy |
status_str |
n |
ids_txt_mv |
(CKB)4100000010106253 (oapen)https://directory.doabooks.org/handle/20.500.12854/44151 (EXLCZ)994100000010106253 |
carrierType_str_mv |
cr |
is_hierarchy_title |
Cosmological Inflation, Dark Matter and Dark Energy |
_version_ |
1787548668929245185 |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03964nam-a2200865z--4500</leader><controlfield tag="001">993548120304498</controlfield><controlfield tag="005">20231214132937.0</controlfield><controlfield tag="006">m o d </controlfield><controlfield tag="007">cr|mn|---annan</controlfield><controlfield tag="008">202102s2019 xx |||||o ||| 0|eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">3-03921-765-8</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(CKB)4100000010106253</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(oapen)https://directory.doabooks.org/handle/20.500.12854/44151</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(EXLCZ)994100000010106253</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Bamba, Kazuharu</subfield><subfield code="4">auth</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Cosmological Inflation, Dark Matter and Dark Energy</subfield></datafield><datafield tag="260" ind1=" " ind2=" "><subfield code="b">MDPI - Multidisciplinary Digital Publishing Institute</subfield><subfield code="c">2019</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 electronic resource (236 p.)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">computer</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">online resource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In addition, according to the rotation curve of galaxies, the existence of dark matter, which does not shine, is also suggested. If primordial gravitational waves are detected in the future, the mechanism for realizing inflation can be revealed. Moreover, there exist two main candidates for dark matter. The first is a new particle, the existence of which is predicted in particle physics. The second is an astrophysical object which is not found by electromagnetic waves. Furthermore, there are two representative approaches to account for the accelerated expansion of the current universe. One is to assume the unknown dark energy in general relativity. The other is to extend the gravity theory to large scales. Investigation of the origins of inflation, dark matter, and dark energy is one of the most fundamental problems in modern physics and cosmology. The purpose of this book is to explore the physics and cosmology of inflation, dark matter, and dark energy.</subfield></datafield><datafield tag="546" ind1=" " ind2=" "><subfield code="a">English</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">de Sitter vacuum</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Einstein-Aether theory of gravity</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Supernovae</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">apparatus</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">normal galaxies</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">higher dimension gauged super-gravity black hole</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark energy model</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cosmo-particle physics</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">instruments</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Cosmic Microwave Background (CMB) temperature</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Dark Energy</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">hyper-color</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quantum tunneling phenomenon</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">spacetime symmetry</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">parametrizations</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quantum gravity</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dynamical Chern-Simons modified gravity</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">comparative planetology</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">properties of specific particles</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">particle physics</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Hawking radiation</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">memory</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">junction conditions</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cosmology</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">composite dark matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dosmological parameters</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">field theory</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Dark Matter</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cosmological model</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">extragalactic objects and systems</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">scalar-tensor gravity</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">fundamental astronomy</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cosmoligical parameters</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">cosmological parameters</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Baryon Acoustic Oscillation (BAO)</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark atoms</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quantum optical systems</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">brans-dicke theory</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark energy models</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">loop quantum cosmology</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">dark energy</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">galactic rotation curve</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">astronomical and space-research instrumentation</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">null hypersurfaces</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">QCD</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">quantum optics</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Hubble constant</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">and components common to several branches of physics and astronomy</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">statistical analysis</subfield></datafield><datafield tag="776" ind1=" " ind2=" "><subfield code="z">3-03921-764-X</subfield></datafield><datafield tag="906" ind1=" " ind2=" "><subfield code="a">BOOK</subfield></datafield><datafield tag="ADM" ind1=" " ind2=" "><subfield code="b">2023-12-15 05:36:49 Europe/Vienna</subfield><subfield code="f">system</subfield><subfield code="c">marc21</subfield><subfield code="a">2020-02-01 22:26:53 Europe/Vienna</subfield><subfield code="g">false</subfield></datafield><datafield tag="AVE" ind1=" " ind2=" "><subfield code="i">DOAB Directory of Open Access Books</subfield><subfield code="P">DOAB Directory of Open Access Books</subfield><subfield code="x">https://eu02.alma.exlibrisgroup.com/view/uresolver/43ACC_OEAW/openurl?u.ignore_date_coverage=true&portfolio_pid=5338758640004498&Force_direct=true</subfield><subfield code="Z">5338758640004498</subfield><subfield code="b">Available</subfield><subfield code="8">5338758640004498</subfield></datafield></record></collection> |