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相关论文: Cosmic-ray upscattered inelastic dark matter

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Ultralight dark matter induces time-dependent perturbations in the spacetime metric, enabling its gravitational direct detection. In this work, we propose using astrometry to detect dark matter. After reviewing the calculation of the metric…

高能物理 - 唯象学 · 物理学 2025-08-06 Jeff A. Dror , Sarunas Verner

Dark matter is poorly constrained by direct detection experiments at masses below 1 MeV. This is an important target for the next generation of experiments, and several methods have been proposed to probe this mass range. One class of such…

高能物理 - 唯象学 · 物理学 2020-07-31 Benjamin V. Lehmann , Stefano Profumo

Direct detection experiments aim at the detection of dark matter in the form of weakly interacting massive particles (WIMPs) by searching for signals from elastic dark matter nucleus scattering. Additionally, inelastic scattering in which…

高能物理 - 唯象学 · 物理学 2020-01-08 G. Arcadi , C. Döring , C. Hasterok , S. Vogl

If compact baryonic objects contribute significantly to the dark matter in our Galaxy, their mass function will present vital clues for galaxy formation theories and star formation processes in the early Universe. Here we discuss what one…

天体物理学 · 物理学 2008-11-26 E. J. Kerins , B. J. Carr

The aperture mass has been shown in a series of recent publications to be a useful quantitative tool for weak lensing studies, ranging from cosmic shear to the detection of a mass-selected sample of dark matter haloes. Quantitative…

天体物理学 · 物理学 2011-05-23 Katrin Reblinsky , Guido Kruse , Bhuvnesh Jain , Peter Schneider

Dark Matter (DM) is an elusive form of matter which has been postulated to explain astronomical observations through its gravitational effects on stars and galaxies, gravitational lensing of light around these, and through its imprint on…

高能物理 - 唯象学 · 物理学 2016-06-07 James Bateman , Ian McHardy , Alexander Merle , Tim R. Morris , Hendrik Ulbricht

Cosmic-ray positrons have long been considered a powerful probe of dark matter annihilation. In particular, myriad studies of the unexpected rise in the positron fraction have debated its dark matter or pulsar origins. In this paper, we…

高能天体物理现象 · 物理学 2022-01-07 Isabelle John , Tim Linden

We propose that the dark matter abundance is set by the decoupling of inelastic scattering instead of annihilations. This coscattering mechanism is generically realized if dark matter scatters against states of comparable mass from the…

高能物理 - 唯象学 · 物理学 2017-12-19 Raffaele Tito D'Agnolo , Duccio Pappadopulo , Joshua T. Ruderman

Inelastic dark matter (IDM) models feature an energy threshold for scattering with Standard Model particles, which enables their consistency with the increasingly stringent limits placed by direct detection experiments. In a typical…

高能物理 - 唯象学 · 物理学 2025-10-15 Zamiul Alam , Christopher V. Cappiello , Francesc Ferrer

LHAASO, a ground-based observatory, is unveiling new frontiers in our understanding of high-energy $\gamma-$rays and cosmic rays. It has recently observed high energy diffuse $\gamma-$rays from the Galactic plane in the TeV-PeV range. For…

高能物理 - 唯象学 · 物理学 2025-09-17 Celine Boehm , Ranjan Laha , Tarak Nath Maity

Traditional dark matter models, eg. WIMPs, assume dark matter is weakly coupled to the standard model so that elastic scattering between dark matter and baryons can be described perturbatively by Born approximation. Most direct detection…

高能物理 - 唯象学 · 物理学 2021-12-03 Xingchen Xu , Glennys R. Farrar

Ordinary baryonic particles (such as protons and neutrons) account for only one-sixth of the total matter in the Universe. The remainder is a mysterious "dark matter" component, which does not interact via electromagnetism and thus neither…

There is currently vast evidence for Dark Matter (DM) from astronomical observations. However, in spite of tremendous efforts by large experimental groups, there is no confirmed direct detection of the dark matter in our galaxy. Recent…

天体物理仪器与方法 · 物理学 2014-11-20 Juan Estrada

In this thesis, I study the expected direct and indirect detection signals of dark matter. More precisely, I study three aspects of dark matter; I use hydrodynamic simulations to extract properties of weakly interacting dark matter that are…

高能物理 - 唯象学 · 物理学 2017-06-06 Lina Necib

We describe cosmic gamma-ray and neutrino signals of dark matter annihilation, explaining how the complementarity of these signals provides additional information that, if observable, can enlighten the particle nature of dark matter. This…

高能物理 - 唯象学 · 物理学 2013-05-30 Rouzbeh Allahverdi , Sheldon Campbell , Bhaskar Dutta

Strong gravitational lensing is a promising way of uncovering the nature of dark matter, by finding perturbations to images that cannot be well accounted for by modeling the lens galaxy without additional structure, be it subhalos (smaller…

宇宙学与河外天体物理 · 物理学 2020-01-29 Ana Diaz Rivero , Cora Dvorkin

We present the results of a study of weak lensing by galaxies based on 45.5 deg$^2$ of $R_C$ band imaging data from the Red-Sequence Cluster Survey (RCS). We present the first weak lensing detection of the flattening of galaxy dark matter…

天体物理学 · 物理学 2008-11-26 Henk Hoekstra , Howard K. C. Yee , Michael D. Gladders

Recent experiments have measured the Galactic $\gamma$-ray diffuse emission up to PeV energies, opening a window to study acceleration of Galactic cosmic rays and their propagation up to the cosmic-ray knee. Furthermore, these observations…

高能天体物理现象 · 物理学 2025-09-12 Manuel Rocamora , Pedro De La Torre Luque , Miguel A. Sánchez-Conde

A brief review of the indirect detection signatures of dark matter is given. In particular, detection methods of dark matter particle annihilation to antimatter and gamma-rays are reviewed. With the GLAST satellite soon to be launched, a…

天体物理学 · 物理学 2008-11-26 Lars Bergstrom

I discuss recent progress in dark matter searches, focusing in particular on how rigorous modeling the dark matter distribution in the Galaxy and in its satellite galaxies improves our interpretation of the limits on the annihilation and…

宇宙学与河外天体物理 · 物理学 2015-06-11 Louis E. Strigari