On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays

TANG Zhi-Cheng; YUAN Qiang; BI Xiao-Jun; CHEN Guo-Ming

doi:10.1088/1674-1137/35/8/006

Chinese Physics C> 2011, Vol. 35> Issue(8) : 725-734 DOI: 10.1088/1674-1137/35/8/006

On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays

Abstract
HTML
Reference
Related

PDF

Abstract：
Monochromatic γ-rays are thought to be the smoking gun signal for identifying dark matter annihilation. However, the flux of monochromatic γ-rays is usually suppressed by virtual quantum effects since dark matter should be neutral and does not couple with γ-rays directly. In this work, we study the detection strategy of the monochromatic γ-rays in a future space-based detector. The flux of monochromatic γ-rays between 50 GeV and several TeV is calculated by assuming the supersymmetric neutralino as a typical dark matter candidate. The detection both by focusing on the Galactic center and in a scan mode that detects γ-rays from the whole Galactic halo are compared. The detector performance for the purpose of monochromatic γ-ray detection, with different energy and angular resolution, field of view, and background rejection efficiencies, is carefully studied with both analytical and fast Monte-Carlo methods.

References

[1]

Gondolo P, Edsj J, Ullio P et al. Journal of Cosmology and Astro Particle Physics, 2004, 7: 82 Catena R, Ullio P. Journal of Cosmology and Astroparticle Physics,2010, 8: 43 Salucci P, Nesti F, Gentile G, Frigerio Martins C. Astron. Astrophys., 2010, 523: A83+4 Komatsu E, Smith K M, Dunkley, J et al. ArXiv e-prints, 2010, arXiv:1001.45385 Navarro J F, Frenk C S, White S D M. Astrophys. J, 1997, 490: 4936 Moore B, Quinn T, Governato F, Stadel J, Lake G. Mon. Not. Roy. Astron. Soc., 1999, 310: 11477 Navarro J F, Ludlow A, Springel V et al. Mon. Not. Roy. Astron. Soc., 2010, 402: 218 Jing Y P, Suto Y. Astrophys. J. Lett., 2000, 529: L699 Berezinsky V S, Gurevich A V, Zybin K P. Physics Letters B, 1992, 294: 22110 Lavalle J, YUAN Q, Maurin D, BI X. Astron. Astrophys., 2008, 479: 42711 Tormen G, Diaferio A, Syer D. Mon. Not. Roy. Astron. Soc., 1998, 299: 72812 Moore B, Ghigna S, Governato F et al. Astrophys. J. Lett., 1999, 524: L1913 Ghigna S, Moore B, Governato F et al. Astrophys. J, 2000, 544: 61614 Zentner A R, Bullock J S. Astrophys. J, 2003, 598: 4915 GAO L, White S D M, Jenkins A, Stoehr F, Springel V. Mon. Not. Roy. Astron. Soc., 2004, 355: 81916 Diemand J, Moore B, Stadel J. Mon. Not. Roy. Astron. Soc., 2004, 352: 53517 Springel V,WANG J, Vogelsberger M et al. Mon. Not. Roy. Astron. Soc., 2008, 391: 168518 Bullock J S, Kolatt T S, Sigad Y et al. Mon. Not. Roy. Astron. Soc., 2001, 321: 55919 Gaisser T K, Honda M, Lipari P, Stanev T. International Cosmic Ray Conference, 2001, 5: 1643-+20 Abdo A A, Ackermann M, Ajello M et al. Physical Review Letters, 2009, 102: 18110121 Aharonian F, Akhperjanian A G, Barres de Almeida U et al. Physical Review Letters, 2008, 101: 26110422 Aharonian F, Akhperjanian A G, Anton G et al. Astron. Astrophys., 2009, 508: 56123 Abdo A A, Ackermann M, Ajello M et al. Physical Review Letters, 2010, 104: 10110124 Sreekumar P, Bertsch D L, Dingus B L et al. Astrophys. J, 1998, 494: 52325 Abdo A A, Ackermann M, Ajello M et al. Astrophys. J, 2009, 703: 124926 Abdo A A, Ackermann M, Ajello M et al. Physical Review Letters, 2009, 103: 25110127 Hunter S D, Bertsch D L, Catelli J R et al. Astrophys. J, 1997, 481: 20528 Bergstrm L, Ullio P, Buckley J H. Astroparticle Physics, 1998, 9: 13729 Aharonian F, Akhperjanian A G, Bazer-Bachi A R et al. Nature, 2006, 439: 69530 Mayer-Hasselwander H A, Bertsch D L, Dingus B L et al. Astron. Astrophys., 1998, 335: 16131 Aharonian F, Akhperjanian A G, Bazer-Bachi A R et al. Physical Review Letters, 2006, 97: 22110232 Abdo A A, Ackermann M, Ajello M et al. Astrophys. J. Supp., 2009, 183: 4633 Aharonian F, Akhperjanian A G, Anton G et al. Astron. Astrophys., 2009, 503: 817

[1]	Zhu Luo , Cheng-feng Cai , Zhao-feng Kang , Zhao-huan Yu , Hong-hao Zhang . Scalar quintuplet minimal dark matter with Yukawa interactions: perturbative up to the Planck scale. Chinese Physics C, 2019, 43(2): 023102. doi: 10.1088/1674-1137/43/2/023102
[2]	Peyman Zakeri , Mohammad Moosavi , Mohammadreza Zakeri , Yaser Ayazi . A minimal model for two-component FIMP dark matter: A basic search. Chinese Physics C, 2018, 42(7): 073101. doi: 10.1088/1674-1137/42/7/073101
[3]	Andrea Addazi , Pietro Donà , Antonino Marcianò . Dynamical interactions of dark energy and dark matter: Yang-Mills condensate and QCD axions. Chinese Physics C, 2018, 42(7): 075102. doi: 10.1088/1674-1137/42/7/075102
[4]	Liuyuan Shen , Yicen Mou , Yunlong Zheng , Mingzhe Li . Direct couplings of mimetic dark matter and their cosmological effects. Chinese Physics C, 2018, 42(1): 015101. doi: 10.1088/1674-1137/42/1/015101
[5]	Yi-Qing Guo , Qiang Yuan . On the knee of Galactic cosmic rays in light of sub-TeV spectral hardenings. Chinese Physics C, 2018, 42(7): 075103. doi: 10.1088/1674-1137/42/7/075103
[6]	null . Constraints on dark matter annihilation and decay from the isotropic gamma-ray background. Chinese Physics C, 2017, 41(4): 045104. doi: 10.1088/1674-1137/41/4/045104
[7]	Shivaramakrishna Singirala . Implications of fermionic dark matter on recent neutrino oscillation data. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102
[8]	Cai-Xun Zhang , Shin-Ted Lin , Jian-Ling Zhao , Xun-Zhen Yu , Li Wang , Jing-Jun Zhu , Hao-Yang Xing . Discrimination of neutrons and γ-rays in liquid scintillator based on Elman neural network. Chinese Physics C, 2016, 40(8): 086204. doi: 10.1088/1674-1137/40/8/086204
[9]	Yi-Ming Hu , Jin Chang , Deng-Yi Chen , Jian-Hua Guo , Yun-Long Zhang , Chang-Qing Feng . Environmental test of the BGO calorimeterfor DArk Matter Particle Explorer. Chinese Physics C, 2016, 40(11): 116003. doi: 10.1088/1674-1137/40/11/116003
[10]	S. A. Alavi , F. S. Kazemian . Photonic dark matter portal and quantum physics. Chinese Physics C, 2016, 40(2): 025101. doi: 10.1088/1674-1137/40/2/025101
[11]	CHANG Xue , LIU Chun , MA Feng-Cai , YANG Shuo . Supersymmetric extension of the minimal dark matter model. Chinese Physics C, 2012, 36(9): 810-817. doi: 10.1088/1674-1137/36/9/003
[12]	LI Xiao-Ping , PEI Guo-Xi , PEI Shi-Lun . Simulation studies on the polarized positron generation from circularly polarized gamma-rays. Chinese Physics C, 2012, 36(10): 1009-1012. doi: 10.1088/1674-1137/36/10/017
[13]	HE Bao-Ping , YAO Zhi-Bin , ZHANG Feng-Qi . A comparison of ionizing radiation damage in CMOS devices from ⁶⁰Co gamma rays, electrons and protons. Chinese Physics C, 2009, 33(6): 436-439. doi: 10.1088/1674-1137/33/6/006
[14]	HE Xiao-Gang . Darkon dark matter, unparticle effects and collider physics. Chinese Physics C, 2009, 33(6): 451-455. doi: 10.1088/1674-1137/33/6/010
[15]	YUAN Qiang , BI Xiao-Jun , ZHANG Juan . Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation. Chinese Physics C, 2009, 33(10): 826-833. doi: 10.1088/1674-1137/33/10/002
[16]	LI Xiao-Ping , PEI Guo-Xi . Experiment studies on the polarized gamma-rays generation at KEK-ATF. Chinese Physics C, 2009, 33(8): 691-695. doi: 10.1088/1674-1137/33/8/018
[17]	Xu Chunxian , Dai Hongyue . Statistic Model for Galactic Cosmic Rays. Chinese Physics C, 1997, 21(S2): 25-32.
[18]	Zhang Li . Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude. Chinese Physics C, 1995, 19(11): 974-979.
[19]	Zhang Tianbao , Wang Haidong , Shen Zhiqi . Measurement of the Radiation Energy in Parapositronium Two Gamma Annihilation. Chinese Physics C, 1991, 15(S3): 227-234.
[20]	Zhou Hongyu , Yan Yiming , Fan Guoying , Lan Liqiao , Wang Qi , Sun Shuxu , Hua Ming , Han Chongzhan , Liu Shuzhen , Rong Yaning , Wen Shenlin , Wang Xinfu , Yan Hua , Wang Wanhong , Tang Lin . Study of Associated Gamma Rays from Niobium under 14,9 MeV Neutron Bombardments. Chinese Physics C, 1989, 13(S1): 97-108.

Access

Get Citation

TANG Zhi-Cheng, YUAN Qiang, BI Xiao-Jun and CHEN Guo-Ming. On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays[J]. Chinese Physics C, 2011, 35(8): 725-734. doi: 10.1088/1674-1137/35/8/006

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2010-11-05
Revised: 1900-01-01

Article Metric

Article Views(2610)
PDF Downloads(651)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays

Received Date: 2010-11-05

Accepted Date: 1900-01-01

Available Online: 2011-08-05

Abstract: Monochromatic γ-rays are thought to be the smoking gun signal for identifying dark matter annihilation. However, the flux of monochromatic γ-rays is usually suppressed by virtual quantum effects since dark matter should be neutral and does not couple with γ-rays directly. In this work, we study the detection strategy of the monochromatic γ-rays in a future space-based detector. The flux of monochromatic γ-rays between 50 GeV and several TeV is calculated by assuming the supersymmetric neutralino as a typical dark matter candidate. The detection both by focusing on the Galactic center and in a scan mode that detects γ-rays from the whole Galactic halo are compared. The detector performance for the purpose of monochromatic γ-ray detection, with different energy and angular resolution, field of view, and background rejection efficiencies, is carefully studied with both analytical and fast Monte-Carlo methods.

HTML

Reference (1)

On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays

HTML

目录