The cosmological constant of emergent spacetime in the Newtonian approximation

[EN] We present a simple quantum-mechanical estimate of the cosmological constant of a Newtonian Universe. We first mimic the dynamics of a Newtonian spacetime by means of a nonrelativistic quantum mechanics for the matter contents of the Universe (baryonic and dark) within a fixed (i.e. nondynamica...

Descripción completa

Detalles Bibliográficos
Autores: Castro-Palacio, Juan Carlos|||0000-0002-0132-9989, Fernández de Córdoba, Pedro|||0000-0002-0347-7280, Isidro, J.M.|||0000-0002-0720-9945
Tipo de recurso: artículo
Fecha de publicación:2020
País:España
Institución:Universitat Politècnica de València (UPV)
Repositorio:RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia
Idioma:inglés
OAI Identifier:oai:riunet.upv.es:10251/169342
Acceso en línea:https://riunet.upv.es/handle/10251/169342
Access Level:acceso abierto
Palabra clave:Emergent spacetime
Cosmological constant
Newtonian cosmology
MATEMATICA APLICADA
Descripción
Sumario:[EN] We present a simple quantum-mechanical estimate of the cosmological constant of a Newtonian Universe. We first mimic the dynamics of a Newtonian spacetime by means of a nonrelativistic quantum mechanics for the matter contents of the Universe (baryonic and dark) within a fixed (i.e. nondynamical) Euclidean spacetime. Then we identify an operator that plays, on the matter states, a role analogous to that played by the cosmological constant. Finally, we prove that there exists a quantum state for the matter fields, in which the above-mentioned operator has an expectation value equal to the cosmological constant of the given Newtonian Universe.