Simulation of the evolution of an unequal-mass neutron-star binary shown at successive times. Blue, green, and yellow represent the scalar field, which is initially centered on each star and then develops into a common “envelope,” and dark orange represents the fluid density.
From the article:
No Evidence of Kinetic Screening in Simulations of Merging Binary Neutron Stars beyond General RelativityMiguel Bezares, Ricard Aguilera-Miret, Lotte ter Haar, Marco Crisostomi, Carlos Palenzuela, and Enrico Barausse
Phys. Rev. Lett. 128, 091103 (2022)
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