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As a journalist, you can create a free Muck Rack account to customize your profile, list your contact preferences, and upload a portfolio of your best work.Articles
Revealing phase transition in dense matter with gravitational wave spectroscopy of binary neutron star mergers
We use numerical relativity simulations of binary neutron star mergers to show that high density deconfinement phase transitions to quark matter can be probed using multimodal postmerger gravitational wave (GW) spectroscopy. Our simulations suggest that hadron-quark phase transitions may suppress the one-armed spiral instability in the remnant. This is manifested in an anticorrelation between the energy carried in the ℓ=2, m=1 GW mode and energy density gap which separates the two phases.
Detectability of QCD phase transitions in binary neutron star mergers: Bayesian inference with the next generation gravitational wave detectors
Aviral Prakash1,2, Ish Gupta1,2, Matteo Breschi3,4,5, Rahul Kashyap1,2, David Radice1,2,6, Sebastiano Bernuzzi3, Domenico Logoteta7,8, and B. S.
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