國立虎尾科技大學 |

Exploring the Early Universe with Gravitational Waves

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
正題名/作者:	Exploring the Early Universe with Gravitational Waves/ by Laura Bianca Bethke.
作者:	Bethke, Laura Bianca.
面頁冊數:	XIII, 139 p. 16 illus., 5 illus. in color.online resource. :
Contained By:	Springer Nature eBook
標題:	Cosmology. -
電子資源:	https://doi.org/10.1007/978-3-319-17449-5
ISBN:	9783319174495

Exploring the Early Universe with Gravitational Waves
Bethke, Laura Bianca.

Exploring the Early Universe with Gravitational Waves[electronic resource] /by Laura Bianca Bethke. - 1st ed. 2015. - XIII, 139 p. 16 illus., 5 illus. in color.online resource. - Springer Theses, Recognizing Outstanding Ph.D. Research,2190-5053. - Springer Theses, Recognizing Outstanding Ph.D. Research,.

Introduction -- Chiral Tensor Power Spectrum from Quantum Gravity -- Anisotropic Gravitational Wave Background from Massless Pre-heating -- Concluding Remarks -- Appendix.

This work investigates gravitational wave production in the early universe and identifies potentially observable features, thereby paving the way for future gravitational wave experiments. It focuses on gravitational wave production in two scenarios: inflation in a model inspired by loop quantum gravity, and preheating at the end of inflation. In the first part, it is demonstrated that gravitational waves’ spectrum differs from the result obtained using ordinary general relativity, with potentially observable consequences that could yield insights into quantum gravity. In the second part, it is shown that the cosmic gravitational wave background is anisotropic at a level that could be detected by future experiments. Gravitational waves promise to be an rich source of information on the early universe. To them, the universe has been transparent from its earliest moments, so they can give us an unobstructed view of the Big Bang and a means to probe the fundamental laws of nature at very high energies.

ISBN: 9783319174495

Standard No.: 10.1007/978-3-319-17449-5doiSubjects--Topical Terms:

579761
Cosmology.

LC Class. No.: QB980-991

Dewey Class. No.: 523.1

Exploring the Early Universe with Gravitational Waves
LDR:02630nam a22004095i 4500 001 965945
003 DE-He213
005 20200704083803.0
007 cr nn 008mamaa
008 201211s2015 gw | s |||| 0|eng d
020 $a 9783319174495 $9 978-3-319-17449-5
024 7 $a 10.1007/978-3-319-17449-5 $2 doi
035 $a 978-3-319-17449-5
050 4 $a QB980-991
072 7 $a PHR $2 bicssc
072 7 $a SCI015000 $2 bisacsh
072 7 $a PHR $2 thema
082 0 4 $a 523.1 $2 23
100 1 $a Bethke, Laura Bianca. $e author. $4 aut $4 http://id.loc.gov/vocabulary/relators/aut $3 1261597
245 1 0 $a Exploring the Early Universe with Gravitational Waves $h [electronic resource] / $c by Laura Bianca Bethke.
250 $a 1st ed. 2015.
264 1 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2015.
300 $a XIII, 139 p. 16 illus., 5 illus. in color. $b online resource.
336 $a text $b txt $2 rdacontent
337 $a computer $b c $2 rdamedia
338 $a online resource $b cr $2 rdacarrier
347 $a text file $b PDF $2 rda
490 1 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $x 2190-5053
505 0 $a Introduction -- Chiral Tensor Power Spectrum from Quantum Gravity -- Anisotropic Gravitational Wave Background from Massless Pre-heating -- Concluding Remarks -- Appendix.
520 $a This work investigates gravitational wave production in the early universe and identifies potentially observable features, thereby paving the way for future gravitational wave experiments. It focuses on gravitational wave production in two scenarios: inflation in a model inspired by loop quantum gravity, and preheating at the end of inflation. In the first part, it is demonstrated that gravitational waves’ spectrum differs from the result obtained using ordinary general relativity, with potentially observable consequences that could yield insights into quantum gravity. In the second part, it is shown that the cosmic gravitational wave background is anisotropic at a level that could be detected by future experiments. Gravitational waves promise to be an rich source of information on the early universe. To them, the universe has been transparent from its earliest moments, so they can give us an unobstructed view of the Big Bang and a means to probe the fundamental laws of nature at very high energies.
650 0 $a Cosmology. $3 579761
650 0 $a Educational sociology. $3 555555
650 2 4 $a Sociology of Education. $3 768504
710 2 $a SpringerLink (Online service) $3 593884
773 0 $t Springer Nature eBook
776 0 8 $i Printed edition: $z 9783319174501
776 0 8 $i Printed edition: $z 9783319174488
776 0 8 $i Printed edition: $z 9783319369099
830 0 $a Springer Theses, Recognizing Outstanding Ph.D. Research, $x 2190-5053 $3 1253569
856 4 0 $u https://doi.org/10.1007/978-3-319-17449-5
912 $a ZDB-2-PHA
912 $a ZDB-2-SXP
950 $a Physics and Astronomy (SpringerNature-11651)
950 $a Physics and Astronomy (R0) (SpringerNature-43715)