Primary origin of the PTA nanohertz stochastic gravitational-wave background
Determine whether the stochastic gravitational-wave background reported by pulsar timing array collaborations (NANOGrav, EPTA/InPTA, IPTA) at frequencies around O(10) nanohertz is astrophysical in origin (e.g., supermassive black hole binaries) or primordial in origin (e.g., early-universe processes), by establishing observational and modeling criteria that discriminate between these possibilities in a manner consistent with current datasets.
References
The recent data release by the PTA observations, such as the NANOGrav collaboration, the EPTA/InPTA and IPTA provide tentative evidence for the detection of a background of stochastic GWs at low frequencies (~ O(101) nHz range), whose primary origin, whether astrophysical or primordial, is yet to be established.
While the interpretation of the PTA signal remains open, this has sharpened the broader question of whether future gravitational-wave observations can distinguish standard cosmic strings from superstring-motivated extensions.