Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3643
Articles: 2'487'895
Articles rated: 2609

28 March 2024
 
  » arxiv » 1903.7644

 Article overview


Multi-Messenger Astrophysics with Pulsar Timing Arrays
Luke Zoltan Kelley ; Maria Charisi ; Sarah Burke-Spolaor ; Joseph Simon ; Laura Blecha ; Tamara Bogdanovic ; Monica Colpi ; Julie Comerford ; Daniel J. D'Orazio ; Massimo Dotti ; Michael Eracleous ; Matthew Graham ; Jenny E. Greene ; Zoltán Haiman ; Kelly Holley-Bockelmann ; Erin Kara ; Bernard Kelly ; S. Komossa ; Shane L. Larson ; Xin Liu ; Chung-Pei Ma ; Scott Noble ; Vasileios Paschalidis ; Roman R. Rafikov ; Vikram Ravi ; Jessie C. Runnoe ; Alberto Sesana ; Daniel Stern ; Michael A. Strauss ; Vivian U ; Marta Volonteri ; NANOGrav Collaboration ;
Date 18 Mar 2019
AbstractPulsar timing arrays (PTAs) are on the verge of detecting low-frequency gravitational waves (GWs) from supermassive black hole binaries (SMBHBs). With continued observations of a large sample of millisecond pulsars, PTAs will reach this major milestone within the next decade. Already, SMBHB candidates are being identified by electromagnetic surveys in ever-increasing numbers; upcoming surveys will enhance our ability to detect and verify candidates, and will be instrumental in identifying the host galaxies of GW sources. Multi-messenger (GW and electromagnetic) observations of SMBHBs will revolutionize our understanding of the co-evolution of SMBHs with their host galaxies, the dynamical interactions between binaries and their galactic environments, and the fundamental physics of accretion. Multi-messenger observations can also make SMBHBs ’standard sirens’ for cosmological distance measurements out to $zsimeq0.5$. LIGO has already ushered in breakthrough insights in our knowledge of black holes. The multi-messenger detection of SMBHBs with PTAs will be a breakthrough in the years $2020-2030$ and beyond, and prepare us for LISA to help complete our views of black hole demographics and evolution at higher redshifts.
Source arXiv, 1903.7644
Services Forum | Review | PDF | Favorites   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser claudebot






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica