Gravitational radiation at null infinity is characterized via asymptotic super-momentum properties for any cosmological constant, matching the news tensor when Lambda equals zero and providing a reliable definition otherwise.
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Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.
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Characterization of gravitational radiation at infinity with a cosmological constant
Gravitational radiation at null infinity is characterized via asymptotic super-momentum properties for any cosmological constant, matching the news tensor when Lambda equals zero and providing a reliable definition otherwise.
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Radiation in Fluid/Gravity and the Flat Limit
Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.