ITP OpenIR  > 理论物理所2015年知识产出
Interpreting the galactic center gamma-ray excess in the NMSSM
Cao, JJ; Shang, LL; Wu, PW; Yang, JM; Zhang, Y; Cao, JJ (reprint author), Henan Normal Univ, Dept Phys, Xinxiang 453007, Peoples R China.
2015
发表期刊JOURNAL OF HIGH ENERGY PHYSICS
期号10页码:30
文章类型Article
摘要In the Next-to-Minimal Supersymmetric Standard Model (NMSSM), all singlet-dominated particles including one neutralino, one CP-odd Higgs boson and one CP-even Higgs boson can be simultaneously lighter than about 100 GeV. Consequently, dark matter (DM) in the NMSSM can annihilate into multiple final states to explain the galactic center gamma-ray excess (GCE). In this work we take into account the foreground and background uncertainties for the GCE and investigate these explanations. We carry out a sophisticated scan over the NMSSM parameter space by considering various experimental constraints such as the Higgs data, B-physics observables, DM relic density, LUX experiment and the dSphs constraints. Then for each surviving parameter point we perform a fit to the GCE spectrum by using the correlation matrix that incorporates both the statistical and systematic uncertainties of the measured excess. After examining the properties of the obtained GCE solutions, we conclude that the GCE can be well explained by the pure annihilations and with A (1) being the lighter singlet- dominated CP-odd Higgs boson and H (i) denoting the singlet-dominated CP-even Higgs boson or SM-like Higgs boson, and it can also be explained by the mixed annihilation , A (1) H (1). Among these annihilation channels, can provide the best interpretation with the corresponding p-value reaching 0.55. We also discuss to what extent the future DM direct detection experiments can explore the GCE solutions and conclude that the XENON-1T experiment is very promising in testing nearly all the solutions.
关键词Supersymmetry Phenomenology
学科领域Physics
资助者National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; CAS Center for Excellence in Particle Physics (CCEPP) ; CAS Center for Excellence in Particle Physics (CCEPP) ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; CAS Center for Excellence in Particle Physics (CCEPP) ; CAS Center for Excellence in Particle Physics (CCEPP)
DOIhttp://dx.doi.org/10.1007/JHEP10(2015)030
关键词[WOS]SUPERSYMMETRIC DARK-MATTER ; FERMI-LAT ; EXCLUSION BOUNDS ; GENERIC MODEL ; HIGGS SECTORS ; LHC ; TEVATRON ; PROGRAM ; MASS ; PREDICTIONS
收录类别SCI
语种英语
资助者National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; CAS Center for Excellence in Particle Physics (CCEPP) ; CAS Center for Excellence in Particle Physics (CCEPP) ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; National Natural Science Foundation of China (NNSFC) [10821504, 11222548, 11121064, 11135003, 90103013, 11275245] ; CAS Center for Excellence in Particle Physics (CCEPP) ; CAS Center for Excellence in Particle Physics (CCEPP)
WOS类目Physics, Particles & Fields
引用统计
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/20838
专题理论物理所2015年知识产出
通讯作者Cao, JJ (reprint author), Henan Normal Univ, Dept Phys, Xinxiang 453007, Peoples R China.
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GB/T 7714
Cao, JJ,Shang, LL,Wu, PW,et al. Interpreting the galactic center gamma-ray excess in the NMSSM[J]. JOURNAL OF HIGH ENERGY PHYSICS,2015(10):30.
APA Cao, JJ,Shang, LL,Wu, PW,Yang, JM,Zhang, Y,&Cao, JJ .(2015).Interpreting the galactic center gamma-ray excess in the NMSSM.JOURNAL OF HIGH ENERGY PHYSICS(10),30.
MLA Cao, JJ,et al."Interpreting the galactic center gamma-ray excess in the NMSSM".JOURNAL OF HIGH ENERGY PHYSICS .10(2015):30.
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