Predictive Physics of Inflation and Grand Unification for and from the CMB observations

Autor: Norma G. Sanchez
Přispěvatelé: Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Sanchez, Norma G.
Jazyk: angličtina
Rok vydání: 2020
Předmět:
High Energy Physics - Theory
inflaton: potential
04.70.Dy
Cosmic microwave background
cosmic background radiation
CMB data
01 natural sciences
trans-Planckian physics
Cosmology
General Relativity and Quantum Cosmology
[PHYS] Physics [physics]
Gravitation
vacuum energy
High Energy Physics - Phenomenology (hep-ph)
effective field theory
Vacuum energy
05.10.Cc
98.80.-k
Grand Unified Theory
dark energy
010303 astronomy & astrophysics
Ginsburg–Landau effective theory
Physics
[PHYS]Physics [physics]
[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
Atomic and Molecular Physics
and Optics

High Energy Physics - Phenomenology
98.70.Vc
grand unified theory
quantum inflation
[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
83F05
81T20

Astrophysics - Cosmology and Nongalactic Astrophysics
Nuclear and High Energy Physics
scale: inflation
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Unification
FOS: Physical sciences
General Relativity and Quantum Cosmology (gr-qc)
Astrophysics::Cosmology and Extragalactic Astrophysics
[SDU] Sciences of the Universe [physics]
Theoretical physics
0103 physical sciences
04.90.+e
inflation
Landau-Ginzburg model
Inflation (cosmology)
010308 nuclear & particles physics
large scale surveys
98.80.Cq
Astronomy and Astrophysics
grand unification physics
Standard Model of the Universe
High Energy Physics - Theory (hep-th)
11.10.-z
gravitation
primordial gravity waves
Dark energy
[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Zdroj: Int.J.Mod.Phys.A
Int.J.Mod.Phys.A, 2020, 35 (17), pp.2030008. ⟨10.1142/S0217751X20300082⟩
DOI: 10.1142/S0217751X20300082⟩
Popis: This White Paper for the CNRS IN2P3 Prospective 2020 focuses on realistic and timely situations of inflation in connection with the CMB, gravitational and particle physics, adding inter-disciplinarity and unification values within a strongly predictive physical approach. The formulation of inflation in the Ginsburg-Landau approach developed by de Vega and Sanchez [1] and by Boyanovsky, de Vega, Sanchez and Destri [2]-[4] clarifies and places inflation in the setting of the effective field theories of particle physics. In addition, it sets up a clean way to directly confront the inflationary predictions with the available and forthcoming CMB data and select a definitive model. All CMB + LSS data until now show how powerful is the Ginsburg-Landau effective theory of inflation in predicting observables in agreement with observations including the inflation energy scale and the inflaton potential, and which has much more to provide in the future. It paves the way to discoveries, new learning and understanding.
Comment: White Paper presented at the CNRS IN2P3 Prospectives 2020, GT05 Steering Group {\guillemotleft} Physics of Inflation and Dark Energy {\guillemotright}, and the GT05 IN2P3 Topical Meeting held on 9-10 December 2019 in Grenoble, France. 12 pages, no figures
Databáze: OpenAIRE