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[PDF] Top 20 Exceptional Composite Dark Matter

Has 2437 "Exceptional Composite Dark Matter" found on our website. Below are the top 20 most common "Exceptional Composite Dark Matter".

Exceptional Composite Dark Matter

Exceptional Composite Dark Matter

... (blue continuous line), W + W − (red dotted), hh (green dot-dashed) and ZZ (black dashed). Other (subdominant) channels are not shown. As in previous plots, the vertical grey lines indicate the range of values of f ... Voir le document complet

33

Composite dark matter and direct-search experiments

Composite dark matter and direct-search experiments

... that dark particles are not elementary but consist of structures made of exotic particles, that we could generically call “composite dark ...posite dark matter could either saturate the ... Voir le document complet

70

Dark Matter constraints on composite Higgs models

Dark Matter constraints on composite Higgs models

... In composite Higgs models the pseudo-Nambu-Goldstone Boson (pNGB) na- ture of the Higgs field is an interesting alternative for explaining the smallness of the electroweak scale with respect to the beyond the ... Voir le document complet

42

Some potential problems of OHe composite dark matter

Some potential problems of OHe composite dark matter

... with matter, and lead to a successful OHe ...such composite dark matter (dark atoms of OHe) are dominantly related to the helium shell of OHe and involve only one parameter of new ... Voir le document complet

11

Dark matter from dynamical SUSY breaking

Dark matter from dynamical SUSY breaking

... First, the messenger sector—either a separate sector or part of the DSB sector—has previously been proposed as a possible source for a cold DM candidate in GMSB models [3, 5, 28, 29]. The lightest messenger particle ... Voir le document complet

24

Dark matter

Dark matter

... ● Particles with non-trivial interactions: Various particle physics models providing some features that WIMPs don’t have, such as sizable self-interaction, complicated production mechanism or thermal evolution and so on ... Voir le document complet

19

Searching for dark matter with superheated liquid detectors

Searching for dark matter with superheated liquid detectors

... for dark matter detection, and thus the number of bubbles, the acoustic emission intensity, the count rate, and its energy depen- dence must all be characterized precisely in order to discriminate them ... Voir le document complet

295

Radiative Two-Loop Neutrino Masses with Dark Matter

Radiative Two-Loop Neutrino Masses with Dark Matter

... a dark matter particle as one of the internal ...the dark matter candidate by the addition of a Z 2 symmetry that will also be used to forbid tree level or one-loop ... Voir le document complet

40

Dark matter in a SUSY left-right theory

Dark matter in a SUSY left-right theory

... ts Dark matter in the ΩLR model I) Disappearance of DM regions Even slight changes in the SUSY spectra can lead to sizeable changes in the relic density of the lightest ... Voir le document complet

2

Dark Matter in a SUSY Left-Right Model

Dark Matter in a SUSY Left-Right Model

... shows that one can decrease M 1 (m SU SY ) with respect to the CMSSM value by using a large l 1 and l 2 = 0 and increase it only in the case l 2 > 3l 1 . This change in M 1 (m SU SY ) has a strong impact on ... Voir le document complet

4

Inhomogeneous cosmology : an answer to the Dark Matter and Dark Energy problems?

Inhomogeneous cosmology : an answer to the Dark Matter and Dark Energy problems?

... the contrary a lower Hubble factor (thus a slower expansion) would lead to more compact structures, the expansion would not have any dilution effect and all the matter would collapse faster. The sky would be ... Voir le document complet

204

Status and Perspectives of Direct Dark Matter Searches

Status and Perspectives of Direct Dark Matter Searches

... DSM/DAPNIA/SPP, CEA/Saclay, F-91191 Gif-sur-Yvette Cedex, France Supersymmetric particles represent the best motivated candidates to fill the Dark Matter gap, and are actively hunted by a number of ... Voir le document complet

10

Dark matter dynamics in the early universe

Dark matter dynamics in the early universe

... In section 6, we turn on both the annihilation and catalytic reactions and solve the Boltzmann's equation numerically, and discuss how their combined effect affects d[r] ... Voir le document complet

39

Dark matter assimilation into the baryon asymmetry

Dark matter assimilation into the baryon asymmetry

... 4.1 Dark Matter Searches For both direct and indirect detection experiments, the absence of any wino/higgsino content implies that the expected signals for pure bino DM are quite ... Voir le document complet

29

Coherent neutrino scattering in dark matter detectors

Coherent neutrino scattering in dark matter detectors

... B. The effect of the coherent background on WIMP sensitivity Since coherent neutrino scattering is an irreducible back- ground for WIMP searches, the presence of a neutrino source near a dark matter ... Voir le document complet

9

Dark matter at the LHC: WIMPs and beyond

Dark matter at the LHC: WIMPs and beyond

... of dark matter constitutes a major task for contemporary high-energy physics, astrophysics and ...total dark matter abundance in the Universe in ΛCDM cosmology [ 1 ...cosmic dark ... Voir le document complet

9

Dark Matter Time Projection Chamber : Recent R&D Results

Dark Matter Time Projection Chamber : Recent R&D Results

... limited. For a detailed discussion of this work, see Lopez et al. 2011. 5 Conclusion Following the recent dark matter surface run (Ahlen et al. 2011), the DMTPC collaboration has explored techniques to ... Voir le document complet

7

Can light dark matter solve the core-cusp problem?

Can light dark matter solve the core-cusp problem?

... Note that the data indicate that the de Broglie wavelength is a decreasing function of the galactic core radius. However, this appears to go in the opposite direction to the idea behind the ultralight or “fuzzy” ... Voir le document complet

11

Broadband and Resonant Approaches to Axion Dark Matter Detection

Broadband and Resonant Approaches to Axion Dark Matter Detection

... DOI: 10.1103/PhysRevLett.117.141801 A broad class of well-motivated dark matter (DM) models consists of light pseudoscalar particles a coupled weakly to electromagnetism [1–3] . The most famous example is ... Voir le document complet

7

Antiprotons from Dark Matter: current constraints and future sensitivities

Antiprotons from Dark Matter: current constraints and future sensitivities

... of Dark Matter (DM), in the form of an unknown particle filling the galactic halos, originates from many observations in astrophysics and cos- mology: its gravitational effects are apparent on galactic ... Voir le document complet

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