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Found 4 papers, 1 papers with code
When are LIGO/Virgo's Big Black-Hole Mergers?
An abrupt cutoff in the mass spectrum is expected from (pulsational) pair instability supernova simulations; however, GWTC-2 is only consistent with a Truncated mass model if the location of the cutoff increases from $45^{+13}_{-5}\, M_\odot$ at $z < 0. 4$ to $80^{+16}_{-13}\, M_\odot$ at $z > 0. 4$.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(α,γ\right)^{16}\!\rm{O}$ rate
With the first ten gravitational-wave detections of black holes, we constrain the astrophysical S-factor for $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$, at $300\rm{keV}$, to $S_{300}>175\rm{\, keV\, barns}$ at 68% confidence.
High Energy Astrophysical Phenomena
Enabling real-time multi-messenger astrophysics discoveries with deep learning
Multi-messenger astrophysics is a fast-growing, interdisciplinary field that combines data, which vary in volume and speed of data processing, from many different instruments that probe the Universe using different cosmic messengers: electromagnetic waves, cosmic rays, gravitational waves and neutrinos.
Does the Black Hole Merger Rate Evolve with Redshift?
The evolution of the merger rate across redshifts $0 < z \lesssim 1$ is directly tied to the formation and evolutionary processes, providing insight regarding the progenitor formation rate together with the distribution of time delays between formation and merger.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
