Turnaround radius in an accelerated universe with quasi-local mass
Valerio FaraoniPhysics Department, Bishop's University, 2600 College Street, Sherbrooke, Québec, J1M 1Z7 CanadaMarianne Lapierre-LéonardPhysics Department, Bishop's University, 2600 College Street, Sherbrooke, Québec, J1M 1Z7 CanadaAngus PrainPhysics Department, Bishop's University, 2600 College Street, Sherbrooke, Québec, J1M 1Z7 Canada
2015en
ABI
Аннотация
We apply the Hawking-Hayward quasi-local energy construct to obtain in a rigorous way the turnaround radius of cosmic structures in General Relativity. A splitting of this quasi-local mass into local and cosmological parts describes the interplay between local attraction and cosmological expansion.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
10 та иқтибос0 та фойдаланилган манба