Scale invariance, unimodular gravity and dark energy
By M. Shaposhnikov, Daniel Zenhausern. 2008
239 citations recorded by the source corpus.
We demonstrate that the combination of the ideas of unimodular gravity, scale invariance, and the existence of an exactly massless dilaton leads to the evolution of the universe supported by present observations: inflation in the past, followed by the radiation and matter dominated stages and accelerated expansion at present. All mass scales in this type of theories come from one and the same source.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/4d6f71592be23d1fff4f50b07cca9814c005903d
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- Lavinia Heisenberg
- H. Hoekstra
- Thomas D. Kitching
- S. Tsujikawa
- Catherine Heymans
- Tomi Koivisto
- Pedro G. Ferreira
- Fedor Bezrukov
In Nuclear and High Energy Physics
- Lavinia Heisenberg
- Fedor Bezrukov
- M. Shaposhnikov
- Tomi Koivisto
- S. Tsujikawa
- Claudia de Rham
- Pedro G. Ferreira
- D. Mota
Citations in the corpus
- A Postquantum Theory of Classical Gravity? (2018, unknown): “…necessary that the dynamics be invariant under the choice of N and N a , and there are sensible theories which break this, such as shape dynamics [157 – 159] or unim-odular gravity [160 – 166], but it is desirable to have some local symmetry, even if it is not full diffeomorphism invariance.”
- Cosmology and Fundamental Physics with the Euclid Satellite (2012, background): “This partial fixed point (other beta functions do not vanish) suggests an enhancement of symmetry at that scale, and the presence of a Nambu–Goldstone boson (the dilaton field) associated with the breaking of scale invariance [820].”
- Higgs inflation: consistency and generalisations (2010, background): “This may indicate that the UVcomplete theory has an exact, but spontaneously broken quantum scale invariance, relevant also for gauge hierarchy, cosmological constant, and dark energy problems [ 31 , 32].”
- Higgs Inflation (2018, unknown): “[84–98].”
- The Role of Sterile Neutrinos in Cosmology and Astrophysics (2008, unknown): “In this section we discuss in detail how the parameters of the Lagrangian (5) should be chosen so as to explain the BSM phenomena without introducing new physics above the electroweak scale.”