Towards the final word on neutralino dark matter
Abstract
We present a complete phenomenological prospectus for thermal relic neutralinos. Including Sommerfeld enhancements to relic abundance and halo annihilation calculations, we obtain direct, indirect, and collider discovery prospects for all neutralinos with mass parameters M1, M2, |μ|<4 TeV, which freeze out to the observed dark matter abundance, with scalar superpartners decoupled. Much of the relic neutralino sector will be uncovered by the direct detection experiments Xenon1T and LZ, as well as indirect detection with Cerenkov Telescope Array. We emphasize that thermal relic Higgsinos will be found by next-generation direct detection experiments, so long as M1,2<4 TeV. Charged tracks at a 100 TeV hadron collider complement indirect searches for relic winos. Thermal relic bino-winos still evade all planned experiments, including disappearing charged-track searches. However, they can be discovered by compressed electroweakino searches at a 100 TeV collider, completing the full coverage of the relic neutralino surface.
- Authors:
-
- Univ. of Notre Dame, Notre Dame, IN (United States)
- Univ. Heidelberg, Heidelberg (Germany)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Univ. of Notre Dame, Notre Dame, IN (United States); Univ. of Oregon, Eugene, OR (United States)
- Publication Date:
- Research Org.:
- Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Univ. of Oregon, Eugene, OR (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1253007
- Alternate Identifier(s):
- OSTI ID: 1244139; OSTI ID: 1601487
- Report Number(s):
- FERMILAB-PUB-15-543-T; arXiv:1510.03460
Journal ID: ISSN 2470-0010; 1397650
- Grant/Contract Number:
- AC02-07CH11359; SC0011640
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Volume: 93; Journal Issue: 6; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Bramante, Joseph, Desai, Nishita, Fox, Patrick, Martin, Adam, Ostdiek, Bryan, and Plehn, Tilman. Towards the final word on neutralino dark matter. United States: N. p., 2016.
Web. doi:10.1103/PhysRevD.93.063525.
Bramante, Joseph, Desai, Nishita, Fox, Patrick, Martin, Adam, Ostdiek, Bryan, & Plehn, Tilman. Towards the final word on neutralino dark matter. United States. https://doi.org/10.1103/PhysRevD.93.063525
Bramante, Joseph, Desai, Nishita, Fox, Patrick, Martin, Adam, Ostdiek, Bryan, and Plehn, Tilman. Fri .
"Towards the final word on neutralino dark matter". United States. https://doi.org/10.1103/PhysRevD.93.063525. https://www.osti.gov/servlets/purl/1253007.
@article{osti_1253007,
title = {Towards the final word on neutralino dark matter},
author = {Bramante, Joseph and Desai, Nishita and Fox, Patrick and Martin, Adam and Ostdiek, Bryan and Plehn, Tilman},
abstractNote = {We present a complete phenomenological prospectus for thermal relic neutralinos. Including Sommerfeld enhancements to relic abundance and halo annihilation calculations, we obtain direct, indirect, and collider discovery prospects for all neutralinos with mass parameters M1, M2, |μ|<4 TeV, which freeze out to the observed dark matter abundance, with scalar superpartners decoupled. Much of the relic neutralino sector will be uncovered by the direct detection experiments Xenon1T and LZ, as well as indirect detection with Cerenkov Telescope Array. We emphasize that thermal relic Higgsinos will be found by next-generation direct detection experiments, so long as M1,2<4 TeV. Charged tracks at a 100 TeV hadron collider complement indirect searches for relic winos. Thermal relic bino-winos still evade all planned experiments, including disappearing charged-track searches. However, they can be discovered by compressed electroweakino searches at a 100 TeV collider, completing the full coverage of the relic neutralino surface.},
doi = {10.1103/PhysRevD.93.063525},
journal = {Physical Review D},
number = 6,
volume = 93,
place = {United States},
year = {Fri Mar 25 00:00:00 EDT 2016},
month = {Fri Mar 25 00:00:00 EDT 2016}
}
Web of Science
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