Dark energy as a remnant of inflation and electroweak symmetry breaking

Dimopoulos, Konstantinos (0000 0000 8190 6402, Consortium for Fundamental Physics, Physics Department, Lancaster University, Lancaster, LA1 4YB, United Kingdom) ; Markkanen, Tommi (0000 0001 2113 8111, Department of Physics, Imperial College London, London, SW7 2AZ, U.K.)

04 January 2019

Abstract: It is shown that dark energy can be obtained from the interplay of the Higgs boson and the inflaton. A key element is the realization that electroweak symmetry breaking can trigger a second phase of rolling of the inflaton, which, when provided with the appropriate couplings between the fields, can be sufficiently slow to source accelerated expansion in the late time Universe. The observed dark energy density is obtained without fine-tuning of parameters or initial conditions due to an intricate conspiracy of numbers related to inflation, gravity and electroweak physics.


Published in: JHEP 1901 (2019) 029
Published by: Springer/SISSA
DOI: 10.1007/JHEP01(2019)029
arXiv: 1807.04359
License: CC-BY-4.0



Back to search

Fulltext:
Download fulltextXML Download fulltextPDF (PDFA)