Results 91 to 100 of about 8,643,173 (282)
Interacting Agegraphic Dark Energy
A new dark energy model, named "agegraphic dark energy", has been proposed recently, based on the so-called K\'{a}rolyh\'{a}zy uncertainty relation, which arises from quantum mechanics together with general relativity.
A.A. Coley+72 more
core +1 more source
Early Dark Energy from Massive Neutrinos as a Natural Resolution of the Hubble Tension. [PDF]
The Hubble tension can be significantly eased if there is an early component of dark energy that becomes active around the time of matter-radiation equality.
Jeremy Sakstein, M. Trodden
semanticscholar +1 more source
Large imaging surveys, such as the Legacy Survey of Space and Time, rely on photometric redshifts and tomographic binning for 3 × 2 pt analyses that combine galaxy clustering and weak lensing.
Irene Moskowitz+6 more
doaj +1 more source
Exploring the diversity of dark energy dynamics, we discover a calibration relation, a uniform stretching of the amplitude of the equation of state time variation with scale factor. This defines homogeneous families of dark energy physics.
de Putter, Roland, Linder, Eric V.
core +1 more source
Gravitational Rainbows: LIGO and Dark Energy at its Cutoff. [PDF]
The recent direct detection of gravitational waves from a neutron star merger with optical counterpart has been used to severely constrain models of dark energy that typically predict a modification of the gravitational wave speed.
Claudia de Rham, S. Melville
semanticscholar +1 more source
Changes in Microbial Energy Metabolism Measured by Nanocalorimetry during Growth Phase Transitions
Calorimetric measurements of the change in heat due to microbial metabolic activity convey information about the kinetics, as well as the thermodynamics, of all chemical reactions taking place in a cell.
Alberto Robador+11 more
doaj +1 more source
We explore the physics of a gas of particles interacting with a condensate that spontaneously breaks Lorentz invariance. The equation of state of this gas varies from 1/3 to less than -1 and can lead to the observed cosmic acceleration. The particles are
Boss, A. P.+6 more
core +2 more sources
Tale of stable interacting dark energy, observational signatures, and the H0 tension [PDF]
We investigate the observational consequences of a novel class of stable interacting dark energy (IDE) models, featuring interactions between dark matter (DM) and dark energy (DE).
Weiqiang Yang+5 more
semanticscholar +1 more source
Braneworlds and dark energy [PDF]
12 pages, latex, 3 eps figures. Talk given at the Seventh Workshop on Quantum Field Theory under the Influence of External Conditions, IEEC, CSIC and University of Barcelona, Barcelona, Catalonia, Spain, 5-9 September 2005. Revised version published in the workshop proceedings, J. Phys. A: Mathematical and General.
Rui Neves, Rui Neves, Cenalo Vaz
openaire +4 more sources
Quantum Haplodynamics, Dark Matter, and Dark Energy
In quantum haplodynamics (QHD) the weak bosons, quarks, and leptons are bound states of fundamental constituents, denoted as haplons. The confinement scale of the associated gauge group SU(2)h is of the order of Λh≃0.3 TeV.
Harald Fritzsch, Joan Solà
doaj +1 more source