December 6, 2022
12:00PM - 1:00PM
PRB 4138
Add to Calendar
2022-12-06 13:00:00
2022-12-06 14:00:00
CCAPP Seminar: Nihan Pol (Vanderbilt)
Speaker: Nihan Pol (Vanderbilt University)
The Landscape of nanohertz gravitational wave astronomy
The North American, European, Australian, and International pulsar timing arrays have all reported the detection of a spectrally common signal in their latest datasets. However, the smoking gun signature of this signal being astrophysical gravitational waves was missing in all of these datasets. In this talk, I will present an overview of the latest results from pulsar timing arrays, and set the milestones that we can expect pulsar timing arrays to achieve in the next several years.
PRB 4138
OSU ASC Drupal 8
ascwebservices@osu.edu
America/New_York
public
Date Range
Add to Calendar
2022-12-06 12:00:00
2022-12-06 13:00:00
CCAPP Seminar: Nihan Pol (Vanderbilt)
Speaker: Nihan Pol (Vanderbilt University)
The Landscape of nanohertz gravitational wave astronomy
The North American, European, Australian, and International pulsar timing arrays have all reported the detection of a spectrally common signal in their latest datasets. However, the smoking gun signature of this signal being astrophysical gravitational waves was missing in all of these datasets. In this talk, I will present an overview of the latest results from pulsar timing arrays, and set the milestones that we can expect pulsar timing arrays to achieve in the next several years.
PRB 4138
Center for Cosmology and AstroParticle Physics (CCAPP)
ccapp@osu.edu
America/New_York
public
Speaker: Nihan Pol (Vanderbilt University)
The Landscape of nanohertz gravitational wave astronomy
The North American, European, Australian, and International pulsar timing arrays have all reported the detection of a spectrally common signal in their latest datasets. However, the smoking gun signature of this signal being astrophysical gravitational waves was missing in all of these datasets. In this talk, I will present an overview of the latest results from pulsar timing arrays, and set the milestones that we can expect pulsar timing arrays to achieve in the next several years.
