Skip to main content
SearchLogin or Signup

Supermassive Black-hole Demographics &Environments With Pulsar Timing Arrays

Published onMay 31, 2019
Supermassive Black-hole Demographics &Environments With Pulsar Timing Arrays
·

Abstract

Precision timing of large arrays (>50) of millisecond pulsars will detect the nanohertz gravitational-wave emission from supermassive binary black holes within the next ~3–7 years. We review the scientific opportunities of these detections, the requirements for success, and the synergies with electromagnetic instruments operating in the 2020s.

The full text of this article is only available in PDF format:



Comments
0
comment

No comments here