Language:
English
繁體中文
Help
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
Record Type:
Language materials, printed : Monograph/item
Title/Author:
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants/ by Praveen Manoharan.
Author:
Manoharan, Praveen.
Description:
XIV, 65 p. 20 illus.online resource. :
Contained By:
Springer Nature eBook
Subject:
Astronomy. -
Online resource:
https://doi.org/10.1007/978-3-658-36841-8
ISBN:
9783658368418
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
Manoharan, Praveen.
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
[electronic resource] /by Praveen Manoharan. - 1st ed. 2022. - XIV, 65 p. 20 illus.online resource. - BestMasters,2625-3615. - BestMasters,.
Introduction -- Related Work -- Theory -- Methodology -- Results -- Discussion & Conclusion.
In the last 25 years, an extensive body of work has developed various equation of state independent - or (approximately) universal - relations that allow for the inference of neutron star parameters from gravitational wave observations. These works, however, have mostly been focused on singular neutron stars, while our observational efforts at the present, and in the near future, will be focused on binary neutron star (BNS) mergers. In light of these circumstances, the last five years have also given rise to more attempts at developing universal relations that relate BNS pre-merger neutron stars to stellar parameters of the post-merger object, mostly driven by numerical relativity simulations. In this thesis a first attempt at perturbatively deriving universal relations for binary neutron star mergers with long-lived neutron star remnants is presented. The author succeeds in confirming previous results relating pre-merger binary tidal deformabilities to the f-mode frequency of the post-merger object. Combining this result with recent advances of computing the f-mode frequency of fast rotating neutron stars, he also derives a combined relation that relates the pre-merger binary tidal deformability of a BNS to the effective compactness of a long-lived neutron star remnant. Finally, he also proposes a direct relation between these quantities with improved accuracy. About the author Praveen Manoharan is PhD student at Tübingen University, Institute for Theoretical Astrophysics.
ISBN: 9783658368418
Standard No.: 10.1007/978-3-658-36841-8doiSubjects--Topical Terms:
593935
Astronomy.
LC Class. No.: QB1-991
Dewey Class. No.: 520
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
LDR
:02968nam a22004095i 4500
001
1091450
003
DE-He213
005
20220328133807.0
007
cr nn 008mamaa
008
221228s2022 gw | s |||| 0|eng d
020
$a
9783658368418
$9
978-3-658-36841-8
024
7
$a
10.1007/978-3-658-36841-8
$2
doi
035
$a
978-3-658-36841-8
050
4
$a
QB1-991
072
7
$a
PG
$2
bicssc
072
7
$a
SCI004000
$2
bisacsh
072
7
$a
PG
$2
thema
082
0 4
$a
520
$2
23
082
0 4
$a
500.5
$2
23
100
1
$a
Manoharan, Praveen.
$e
author.
$4
aut
$4
http://id.loc.gov/vocabulary/relators/aut
$3
1399035
245
1 0
$a
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
$h
[electronic resource] /
$c
by Praveen Manoharan.
250
$a
1st ed. 2022.
264
1
$a
Wiesbaden :
$b
Springer Fachmedien Wiesbaden :
$b
Imprint: Springer Spektrum,
$c
2022.
300
$a
XIV, 65 p. 20 illus.
$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
BestMasters,
$x
2625-3615
505
0
$a
Introduction -- Related Work -- Theory -- Methodology -- Results -- Discussion & Conclusion.
520
$a
In the last 25 years, an extensive body of work has developed various equation of state independent - or (approximately) universal - relations that allow for the inference of neutron star parameters from gravitational wave observations. These works, however, have mostly been focused on singular neutron stars, while our observational efforts at the present, and in the near future, will be focused on binary neutron star (BNS) mergers. In light of these circumstances, the last five years have also given rise to more attempts at developing universal relations that relate BNS pre-merger neutron stars to stellar parameters of the post-merger object, mostly driven by numerical relativity simulations. In this thesis a first attempt at perturbatively deriving universal relations for binary neutron star mergers with long-lived neutron star remnants is presented. The author succeeds in confirming previous results relating pre-merger binary tidal deformabilities to the f-mode frequency of the post-merger object. Combining this result with recent advances of computing the f-mode frequency of fast rotating neutron stars, he also derives a combined relation that relates the pre-merger binary tidal deformability of a BNS to the effective compactness of a long-lived neutron star remnant. Finally, he also proposes a direct relation between these quantities with improved accuracy. About the author Praveen Manoharan is PhD student at Tübingen University, Institute for Theoretical Astrophysics.
650
0
$a
Astronomy.
$3
593935
650
0
$a
Astrophysics.
$3
646223
650
1 4
$a
Astronomy, Cosmology and Space Sciences.
$3
1366646
710
2
$a
SpringerLink (Online service)
$3
593884
773
0
$t
Springer Nature eBook
776
0 8
$i
Printed edition:
$z
9783658368401
776
0 8
$i
Printed edition:
$z
9783658368425
830
0
$a
BestMasters,
$x
2625-3577
$3
1253531
856
4 0
$u
https://doi.org/10.1007/978-3-658-36841-8
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)
based on 0 review(s)
Multimedia
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login