Resolubilidade global para campos vetoriais no toro n-dimensional

Gonzalez, Rafael Borro

doi:10.11606/t.55.2016.tde-29092016-163857

Cited by 3 publications

(3 citation statements)

References 3 publications

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“…For scalar DM (Fig. 1, right), p-wave suppression of annihilations at late times results in a weak upper bound on y; the bound is likewise exponentially weakened for inelastic DM as the excited state can decay or be thermally depopulated before recombination [22] (not shown in Fig. 1 left).…”

Section: Existing Data Confronts Light Dmmentioning

confidence: 98%

Analyzing the Discovery Potential for Light Dark Matter

et al. 2015

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Section: Existing Data Confronts Light Dmmentioning

confidence: 98%

Analyzing the Discovery Potential for Light Dark Matter

et al. 2015

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“…This qualitatively alters the cosmological phenomenology: although scattering processes still deplete the cosmological population of χ 2 at late times, several experiments can constrain even this small residual abundance. In particular, parts of the parameter space are constrained by considerations of CMB energy injection from χ 1 − χ 2 coannihilation and/or χ 2 decay, while other regions are constrained by χ 2 downscattering in lowthreshold direct detection experiments such as CRESST II [74].…”

Section: Inelastic Dark Matter At Seaquestmentioning

confidence: 99%

Dark sectors at the Fermilab SeaQuest experiment

et al. 2018

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We analyze the unique capability of the existing SeaQuest experiment at Fermilab to discover wellmotivated dark sector physics by measuring displaced electron, photon, and hadron decay signals behind a compact shield. A planned installation of a refurbished electromagnetic calorimeter could provide powerful new sensitivity to GeV-scale vectors, dark Higgs bosons, scalars, axions, and inelastic and strongly interacting dark matter models. This sensitivity is both comparable and complementary to NA62, SHiP, and FASER. SeaQuest's ability to collect data now and over the next few years provides an especially exciting opportunity.

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“…For MeV scale DM, the splitting can be much smaller ∼ O(keV) to shut off direct detection bounds, but a larger splitting may be necessary in order to sufficiently depopulate the excited state before CMB freeze-out[65], so we conservatively adopt 100 keV.…”

mentioning

confidence: 99%

MeV-scale dark matter deep underground

2015

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We demonstrate that current and planned underground neutrino experiments could offer a powerful probe of few-MeV dark matter when combined with a nearby high-intensity low-to-medium energy electron accelerator. This experimental setup, an underground beam-dump experiment, is capable of decisively testing the thermal freeze-out mechanism for several natural dark matter scenarios in this mass range. We present the sensitivity reach in terms of the mass-coupling parameter space of existing and planned detectors, such as Super-K, SNO+, and JUNO, in conjunction with a hypothetical 100 MeV energy accelerator. This setup can also greatly extend the sensitivity of direct searches for new light weakly-coupled force-carriers independently of their connection to dark matter.

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Resolubilidade global para campos vetoriais no toro n-dimensional

Cited by 3 publications

References 3 publications

Analyzing the Discovery Potential for Light Dark Matter

Analyzing the Discovery Potential for Light Dark Matter

Dark sectors at the Fermilab SeaQuest experiment

MeV-scale dark matter deep underground

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