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相关论文: The Physics Case for Axions, WIMPs, WISPs and Othe…

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Progress in observational cosmology over the past five years has established that the Universe is dominated dynamically by dark matter and dark energy. Both these new and apparently independent forms of matter-energy have properties that…

天体物理学 · 物理学 2009-11-10 J. M. Overduin , P. S. Wesson

Axions are among the most sought-after candidates for dark matter. In the ultralight regime, they could help alleviate puzzles in small scale cosmology. Searches for a halo of axion dark matter rely on the electromagnetic response to a…

高能物理 - 唯象学 · 物理学 2023-12-08 Joshua Berger , Amit Bhoonah

A short summary is given of the current status of B physics. Reasons for physics beyond the Standard Model are discussed. Constraints on New Physics are given using measurements of B mixing, Bs mixing, and CP violation, along with |Vub.…

高能物理 - 唯象学 · 物理学 2009-11-11 Sheldon Stone

High energy physics aims to understand the fundamental laws of particles and their interactions at both the largest and smallest scales of the universe. This typically means probing very high energies or large distances or using…

Weakly Interacting Massive Particles (WIMPs) are leading candidates for the dominant part of the mass density of the Universe. Here we will review direct WIMP detection techniques by giving examples of currently running experiments, and…

天体物理学 · 物理学 2007-05-23 Laura Baudis , H. V. Klapdor-Kleingrothaus

Axion physics has received a boost with the recent claim of the PVLAS collaboration. Their results can be interpreted as due to a new axionlike particle but the CAST collaboration has not found trace of it. While the axionlike particle…

高能物理 - 唯象学 · 物理学 2008-11-26 Javier Redondo

The Wilkinson Microwave Anisotropy Probe microwave background data may be giving us clues about new physics at the transition from a ``stringy'' epoch of the universe to the standard Friedmann Robertson Walker description. Deviations on…

高能物理 - 唯象学 · 物理学 2009-11-10 Mar Bastero-Gil , Katherine Freese , Laura Mersini-Houghton

Weakly interacting massive particles (WIMPs) are one of very few probes of cosmology before Big Bang nucleosynthesis (BBN). We point out that in scenarios in which the Universe evolves in a non-standard manner during and after WIMP kinetic…

天体物理学 · 物理学 2009-06-23 Graciela B. Gelmini , Paolo Gondolo

The axion is a highly motivated elementary particle which could address two fundamental questions in physics - the strong CP problem and the dark matter mystery. Experimental searches for this hypothetical particle have started to reach…

高能物理 - 唯象学 · 物理学 2021-10-28 Yannis K. Semertzidis , SungWoo Youn

It was recently proposed that weakly interacting massive particles (WIMP) may provide new ways of generating the observed baryon asymmetry in the early universe, as well as addressing the cosmic coincidence between dark matter and baryon…

高能物理 - 唯象学 · 物理学 2015-11-18 Yanou Cui

We study the prospects for detecting Weakly Interacting Massive Particles (WIMPs), in a number of phenomenological scenarios, with a detector composed of a target simultaneously sensitive to both spin-dependent and spin-independent…

天体物理学 · 物理学 2008-11-26 G. Bertone , D. G. Cerdeno , J. I. Collar , B. Odom

Neutron stars involve extreme physics which is difficult (perhaps impossible) to explore in laboratory experiments. We have to turn to astrophysical observations, and try to extract information from the entire range of the electromagnetic…

高能天体物理现象 · 物理学 2017-09-22 N. Andersson

Linear stability of an isothermal, pressure-bounded, self-gravitating gas slab which is gravitationally coupled with the background weakly interacting massive particles (WIMPs) is investigated. Analytic dispersion relations describing such…

天体物理学 · 物理学 2009-10-31 David Tsiklauri

The existence of dark matter was suggested, using simple gravitational arguments, seventy years ago. Although we are now convinced that most of the mass in the Universe is indeed some non-luminous matter, we still do not know its…

高能物理 - 唯象学 · 物理学 2009-11-10 Carlos Munoz

There is a strong possibility that the particles making up the dark matter in the Universe have a mass below 1 eV and in many important situations exhibit a wave-like behavior. Amongst the candidates the axion stands out as particularly…

高能物理 - 唯象学 · 物理学 2022-09-20 Joerg Jaeckel , Gray Rybka , Lindley Winslow

Dark matter accounts for 26% of the mass-energy density of the Universe, however, its nature and origins remain the most important open questions in physics. The search for Weakly Interacting Massive Particles (WIMPs), one of the leading…

高能物理 - 唯象学 · 物理学 2024-01-17 Marcin Kuźniak

We briefly review the constraints on the search for low mass wimps (< 15 GeV) and the various experimental methods. These experiments depend on the response of detectors to low energy signals (less than 15 KeV equivalent energy). We then…

高能天体物理现象 · 物理学 2015-05-20 David B. Cline

These lectures on non-baryonic dark matter matter are divided into two parts. In the first part, I discuss the need for non-baryonic dark matter in light of recent results in cosmology, and I present some of the most popular candidates for…

天体物理学 · 物理学 2007-05-23 Paolo Gondolo

We investigate a new class of dark matter: superweakly-interacting massive particles (superWIMPs). As with conventional WIMPs, superWIMPs appear in well-motivated particle theories with naturally the correct relic density. In contrast to…

高能物理 - 唯象学 · 物理学 2010-11-11 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

Astrophysics plays a pivotal role in the quest for axions and axion-like particles, offering guidance to experimental efforts and enabling the investigation of axion properties that cannot be probed otherwise. In this context, the extreme…

高能物理 - 唯象学 · 物理学 2026-04-24 Alessandro Lella