English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
Add to Basket
 Local TagsRelease HistoryDetailsSummary
  Comparison between numerical relativity and a new class of post-Newtonian gravitational-wave phase evolutions: The nonspinning equal-mass case

Gopakumar, A., Hannam, M., Husa, S., & Brügmann, B. (2008). Comparison between numerical relativity and a new class of post-Newtonian gravitational-wave phase evolutions: The nonspinning equal-mass case. Physical Review D, 78(6): 064026. doi:10.1103/PhysRevD.78.064026.

Item is

 

show all hide all

Basic

show hide
Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-13A1-8 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-13A4-2
Genre: Journal Article

Files

show Files
hide Files
:
PRD78-064026.pdf (Publisher version), 213KB
View   Save
File Permalink:
https://hdl.handle.net/11858/00-001M-0000-0013-13A5-F
Name:
PRD78-064026.pdf
Description:
-
OA-Status:
Visibility:
Public
MIME-Type / Checksum:
application/pdf
Technical Metadata:
View
Copyright Date:
-
Copyright Info:
-
License:
-

Locators

show

Creators

show
hide
 Creators:
Gopakumar, Achamveedu1, Author
Hannam, Mark1, Author
Husa, Sascha2, Author           
Brügmann, Bernd1, Author
Affiliations:
1External Organizations, Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, Max-Wien-Platz 107743 Jena, Germany , ou_persistent22              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

Content

show
hide
Free keywords: -
 Abstract: We compare the phase evolution of equal-mass nonspinning black-hole binaries from numerical relativity (NR) simulations with post-Newtonian (PN) results obtained from three PN approximants: the TaylorT1 and T4 approximants, for which NR-PN comparisons have already been performed in the literature, and the recently proposed approximant TaylorEt. The accumulated phase disagreement between NR and PN results over the frequency range Momega=0.0455 to Momega=0.1 is greater for TaylorEt than either T1 or T4, but has the attractive property of decreasing monotonically as the PN order is increased.

Details

show
hide
Language(s):
 Dates: 2008-09-10
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 398321
URI: http://link.aps.org/doi/10.1103/PhysRevD.78.064026
DOI: 10.1103/PhysRevD.78.064026
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Physical Review D
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 78 (6) Sequence Number: 064026 Start / End Page: - Identifier: -