Results 31 to 40 of about 685,566 (247)
Prospects for measuring dark energy with 21 cm intensity mapping experiments [PDF]
Abstract Using the 21 cm intensity mapping (IM) technique can efficiently perform large-scale neutral hydrogen (HI) surveys, and this method has great potential for measuring dark-energy parameters. Some 21 cm IM experiments aiming at measuring dark energy in the redshift range of 0<z<3 have been proposed and performed, in which ...
Wu, Peng-Ju, Zhang, Xin
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Investigating the collinear splitting effects of boosted dark matter at neutrino detectors
We study the probing prospects of cosmic ray boosted dark matter (DM) in the framework of simplified electron-philic dark photon model. Focusing on the dark matter and dark photon masses around keV ~ MeV scale, we consider the bounds obtained from the ...
Jinmian Li, Junle Pei, Cong Zhang
doaj +1 more source
The prospects for constraining dark energy with future X-ray cluster gas mass fraction measurements [PDF]
We examine the ability of a future X-ray observatory to constrain dark energy via measurements of the cluster X-ray gas mass fraction, fgas. We find that fgas measurements for a sample of ~500 hot, X-ray bright, dynamically relaxed clusters, to a ...
Adam Mantz +108 more
core +1 more source
Optimizing New Dark Energy Experiments [PDF]
Next generation “Stage IV” dark energy experiments under design during this grant, and now under construction, will enable the determination of the properties of dark energy and dark matter to unprecedented precision using multiple complementary probes.
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Status of the PADME experiment and review of dark photon searches
While accelerator particle physics has traditionally focused on exploring dark matter through highenergy experiments, testing dark-sectors hypothesis requires innovative low energy experiments that use highintensity beams and high-sensitivity detectors ...
Raggi M.
doaj +1 more source
Tritium beta decay with modified neutrino dispersion relations: KATRIN in the dark sea
We explore beta decays in a dark background field, which could be formed by dark matter, dark energy or a fifth force potential. In such scenarios, the neutrino's dispersion relation will be modified by its collective interaction with the dark field ...
Guo-yuan Huang, Werner Rodejohann
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Large Scale Cosmic Microwave Background Anisotropies and Dark Energy [PDF]
In this note we investigate the effects of perturbations in a dark energy component with a constant equation of state on large scale cosmic microwave background anisotropies. The inclusion of perturbations increases the large scale power.
A. M. Lewis +39 more
core +2 more sources
Evidence for Dark Energy Driven by Star Formation: Information Dark Energy?
Evidence is presented for dark energy resulting directly from star formation. A survey of stellar mass density measurements, SMD(a), as a function of universe scale size a, was found to be described by a simple CPL w0 − wa parameterisation that was in ...
Michael Paul Gough
doaj +1 more source
Resolving XENON excess with decaying cold dark matter
We propose a decaying cold dark matter model to explain the excess of electron recoil observed at the XENON1T experiment. In this scenario, the daughter dark matter from the parent dark matter decay easily obtains velocity large enough to saturate the ...
Shuai Xu, Sibo Zheng
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Dark Seesaw at Low Energy Experiments
Based on 2007.11813 With Silvia Pascoli, Matheus ...
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