2015/05/06 by C. J. A. P. Martins, A. M. M. Pinho, Ana Marta Pinho · 23 citations
Physics and Astronomy · #Astrophysics #Constant (computer programming) #Cosmological constant #Cosmology #Cosmology and Gravitation Theories #Coupling (piping) #Coupling constant #Dark Matter and Cosmic Phenomena #Dark energy #Dimensionless quantity #Energy (signal processing) #Equation of state #Fine-structure constant #Hubble's law #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Supernova #Theoretical physics #Type (biology) #astro-ph.CO #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.91.103501
published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 91(10) (American Physical Society) · 5 pages, 3 figures
openalex publication_date 2015/05/06 · arxiv created 2015/05/08 · arxiv updated 2015/05/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We use astrophysical and atomic clock tests of the stability of the fine-structure constant \ensuremathα, together with type Ia supernova and Hubble parameter data, to constrain the simplest class of dynamical dark energy models where the same degree of freedom is assumed to provide both the dark energy and (through a dimensionless coupling \ensuremathζ to the electromagnetic sector) the \ensuremathα variation. We show how current data tightly constrain a combination of \ensuremathζ and the dark energy equation of state w0. At the 95% confidence level and marginalizing over w0 we find |\ensuremathζ|<5\ifmmode×\else\texttimes\fi10^\ensuremath-6, with the atomic clock tests dominating the constraints. The forthcoming generation of high-resolution ultrastable spectrographs will enable significantly tighter constraints.