De Sitter Relativity: a New Road to Quantum Gravity?


Autoria(s): Aldrovandi, R.; Pereira, J. G.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

30/09/2013

20/05/2014

30/09/2013

20/05/2014

01/01/2009

Resumo

The Poincar, group generalizes the Galilei group for high-velocity kinematics. The de Sitter group is assumed to go one step further, generalizing Poincar, as the group governing high-energy kinematics. In other words, ordinary special relativity is here replaced by de Sitter relativity. In this theory, the cosmological constant I > is no longer a free parameter, and can be determined in terms of other quantities. When applied to the whole universe, it is able to predict the value of I > and to explain the cosmic coincidence. When applied to the propagation of ultra-high energy photons, it gives a good estimate of the time delay observed in extragalactic gamma-ray flares. It can, for this reason, be considered a new paradigm to approach the quantum gravity problem.

Identificador

http://dx.doi.org/10.1007/s10701-008-9258-5

Foundations of Physics. New York: Springer, v. 39, n. 1, p. 1-19, 2009.

0015-9018

http://hdl.handle.net/11449/24169

10.1007/s10701-008-9258-5

WOS:000262315200001

Idioma(s)

eng

Publicador

Springer

Relação

Foundations of Physics

Direitos

closedAccess

Palavras-Chave #de Sitter relativity #Cosmological constant #Quantum gravity
Tipo

info:eu-repo/semantics/article