Published December 18, 2019
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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.
Additional Information
Submitted to the Astro2020 Decadal Survey. One of 5 core white-papers authored by members of the NANOGrav Collaboration.Attached Files
Submitted - 1903.08183.pdf
Files
1903.08183.pdf
Files
(5.6 MB)
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Additional details
- Eprint ID
- 100359
- Resolver ID
- CaltechAUTHORS:20191218-140758849
- Created
-
2019-12-18Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Series Name
- Astro2020 Science White Paper