Constraints on dark matter annihilation and decay from the isotropic gamma-ray background

null

doi:10.1088/1674-1137/41/4/045104

Chinese Physics C> 2017, Vol. 41> Issue(4) : 045104 DOI: 10.1088/1674-1137/41/4/045104

Constraints on dark matter annihilation and decay from the isotropic gamma-ray background

null

Abstract
HTML
Reference
Related

PDF

Abstract：
We study the constraints on dark matter (DM) annihilation/decay from the Fermi-LAT Isotropic Gamma-Ray Background (IGRB) observation. We consider the contributions from both extragalactic and galactic DM components. For DM annihilation, the evolution of extragalactic DM halos is taken into account. We find that the IGRB annihilation constraints under some DM subhalo models can be comparable to those derived from the observations of dwarf spheroidal galaxies and CMB. We also use the IGRB results to constrain the parameter regions accounting for the latest AMS-02 electron-positron anomaly. We find that the majority of DM annihilation/decay channels are strongly disfavored by the latest Fermi-LAT IGRB observation; only DM decays to μ⁺μ^- and 4μ channels may be valid.
- dark matter theory

References

[1]	P. A. R. Ade, N. Aghanim. et al (Planck Collaboration) AA, 594:A13 (2016)
[2]	C. Consolandi et al (the AMS-02 Collaboration), arXiv:1402.0467
[3]	O. Adriani, G. C. Barbarino, G. A. Bazilevskaya et al, Nature, 458:607
[4]	S. Torii, T. Yamagami, T. Tamura et al, arXiv:0809.0760
[5]	J. Chang, J. H. Adams, H. S. Ahn et al, Nature, 456:362 (2008)
[6]	F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida et al, Physical Review Letters, 101:261104 (2008)
[7]	F. Aharonian, A. G. Akhperjanian, G. Anton et al, AA, 508:561 (2009)
[8]	A. A. Abdo, M. Ackermann, M. Ajello et al, Physical Review Letters, 102:181101 (2009)
[9]	M. Aguilar, D. Aisa, A. Alvino et al, Physical Review Letters, 113:121102
[10]	L. Accardo, M. Aguilar, D. Aisa et al, Physical Review Letters, 113:121101
[11]	C. E. Fichtel, G. A. Simpson, and D. J Thompson. ApJ, 222:833 (1978)
[12]	P. Sreekumar, D. L. Bertsch, B. L. Dingus et al, ApJ, 494:523 (1998)
[13]	A. A. Abdo, M. Ackermann, M. Ajello et al, Physical Review Letters, 104:101101 (2010)
[14]	M. Ackermann, M. Ajello, A. Albert et al, ApJ, 799:86 (2015)
[15]	M. Cirelli, G. Corcella, A. Hektor et al, Phys, 3, 051 (2011)
[16]	P. Ullio, L. Bergstrm, J. Edsj, and C Lacey, Phys, 66:123502 (2002)
[17]	J. E. Taylor and J Silk, MNRAS, 339:505 (2003)
[18]	S. Profumo and T. E Jeltema, J. Cosmology Astropart. Phys., 7:020 (2009)
[19]	M. Kawasaki, K. Kohri, and K. Nakayama, Phys. Rev. D, 80:023517 (2009)
[20]	A. A. Abdo, M. Ackermann, M. Ajello et al, J. Cosmology Astropart. Phys., 4:014 (2010)
[21]	Q. Yuan, B. Yue, X.-J. Bi, X. Chen, and X Zhang, J. Cosmology Astropart. Phys., 10:023 (2010)
[22]	M. Cirelli, P. Panci, and P. D. Serpico, Nuclear Physics B, 840:284 (2010)
[23]	C.-R. Chen, S. K. Mandal, and F. Takahashi, J. Cosmology Astropart. Phys., 1:023 (2010)
[24]	S. Blanchet and J. Lavalle, J. Cosmology Astropart. Phys., 11:021 (2012)
[25]	M. Cirelli, E. Moulin, P. Panci, P. D. Serpico, and A. Viana, Phys. Rev. D, 86:083506 (2012)
[26]	K. N. Abazajian, S. Blanchet, and J. P Harding, Phys. Rev. D, 85:043509 (2012)
[27]	T. Bringmann, F. Calore, M. Di Mauro, and F. Donato, Phys. Rev. D, 89:023012
[28]	I. Cholis, D. Hooper, and S. D. McDermott, J. Cosmology Astropart. Phys., 2:014 (2014)
[29]	M. Ajello, D. Gasparrini, M. Snchez-Conde et al, ApJ, 800:L27 (2015)
[30]	The Fermi LAT Collaboration, J. Cosmology Astropart. Phys.,9:008 (2015)
[31]	M. Di Mauro and F. Donato, Phys. Rev. D, 91:123001 (2015)
[32]	S. Ando and K. Ishiwata, J. Cosmology Astropart. Phys., 5:024 (2015)
[33]	J.-Q. Xia, A. Cuoco, E. Branchini, and M. Viel, ApJS, 217:15 (2015)
[34]	A. Cuoco, J.-Q. Xia, M. Regis et al, ApJS, 221:29 (2015)
[35]	M. Ackermann, M. Ajello, A. Allafort et al, ApJ, 755:164 (2012)
[36]	B. C. Lacki, S. Horiuchi, and J. F. Beacom, ApJ, 786:40 (2014)
[37]	T. M. Venters and V. Pavlidou, ApJ, 737:80
[38]	D. Yan, H. Zeng, and L. Zhang, MNRAS, 422:1779 (2012)
[39]	H. Zeng, D. Yan, and L. Zhang, MNRAS, 431:997 (2013)
[40]	H. D. Zeng, D. H. Yan, Y. Q. Sun, and L. Zhang, ApJ, 749:151 (2012)
[41]	Y. Inoue, ApJ, 733:66 (2011)
[42]	M. Di Mauro, F. Calore, F. Donato, M. Ajello, and L. Latronico, ApJ, 780:161 (2014)
[43]	M. Fornasa and M. A. Snchez-Conde, Phys. Rep., 598:1 (2015)
[44]	M. Ackermann, M. Ajello, A. Albert et al, Physical Review Letters, 116:151105 (2016)
[45]	G. L. Bryan and M. L. Norman, ApJ, 495:80 (1998)
[46]	J. F. Navarro, C. S. Frenk, and S. D. M. White, ApJ, 462:563 (1996)
[47]	J. S. Bullock, T. S. Kolatt, Y. Sigad et al, MNRAS, 321:559 (2001)
[48]	V. R. Eke, S. Cole, and C. S. Frenk, MNRAS, 282, (1996)
[49]	A. V. Macci, A. A. Dutton, and F. C. van den Bosch, MNRAS, 391:1940 (2008)
[50]	K. A. Olive (Particle Data Group), Chinese Physics C, 38:090001 (2014)
[51]	H. Mo, F. C. van den Bosch, and S. White, Galaxy Formation and Evolution (Cambridge, UK:Cambridge University Press, 2010)
[52]	S. M. Carroll, W. H. Press, and E. L. Turner, ARAA, 30:499 (1992)
[53]	J. M. Bardeen, J. R. Bond, N. Kaiser, and A. S. Szalay, ApJ, 304:15 (1986)
[54]	R. C. Gilmore, R. S. Somerville, J. R. Primack, and A. Domnguez, MNRAS, 422:3189 (2012)
[55]	R. J. Gould and G. Schrder, Physical Review Letters, 16:252 (1996)
[56]	F. W. Stecker, O. C. de Jager, and M. H. Salamon, ApJl, 390:L49 (1992)
[57]	M. Ackermann, M. Ajello, A. Allafort et al, J. Cosmology Astropart. Phys., 5:025 (2010)
[58]	Q. Yuan, P.-F. Yin, X.-J. Bi, X.-M. Zhang, and S.-H. Zhu, Phys. Rev. D, 82:023506 (2010)
[59]	E. Nezri, R. White, C. Combet et al, MNRAS, 425, 477 (2012)
[60]	A. Abramowski, F. Acero, F. Aharonian et al, Physical Review Letters, 106:161301 (2011)
[61]	M. Ackermann, A. Albert, B. Anderson et al, Phys. Rev. D, 89:042001 (2014)
[62]	M. Ackermann, A. Albert, B. Anderson et al, Physical Review Letters, 115:231301 (2015)
[63]	M. Boudaud, S. Aupetit, S. Caroff et al, AA, 575:A67 (2015)
[64]	X. Li, Z.-Q. Shen, B.-Q. Lu et al, Physics Letters B, 749:267 (2015)
[65]	E. Carqun, M. A. Daz, G. A. Gmez-Vargas, B. Panes, and N. Viaux, Physics of the Dark Universe, 11:1 (2016)
[66]	T. Basak, S. Mohanty, and G. Tomar, Journal of High Energy Physics, 3:62 (2016)
[67]	M. Kamionkowski and S. M. Koushiappas, Phys. Rev. D, 77:103509 (2008)
[68]	M. Kamionkowski, S. M. Koushiappas, and M. Kuhlen, Phys. Rev. D, 81:043532 (2010)
[69]	L. J. Rosenberg and K. A. van Bibber, Phys. Rep., 325:1 (2000)
[70]	S. J. Asztalos, L. J. Rosenberg, K. van Bibber, P. Sikivie, and K. Zioutas, Annual Review of Nuclear and Particle Science, 56:293 (2006)
[71]	J. F. Navarro, C. S. Frenk, and S. D. M. White, ApJ, 490:493 (1997)
[72]	C. Giocoli, G. Tormen, R. K. Sheth, and F. C. van den Bosch, MNRAS, 404:502 (2010)
[73]	M. Maciejewski, M. Vogelsberger, S. D. M. White, and V. Springel, MNRAS, 415:2475 (2011)
[74]	G. R. Blumenthal and R. J. Gould, Reviews of Modern Physics, 42:237 (1970)
[75]	F. C. Jones, Physical Review, 167:1159 (1968)
[76]	S.-J. Lin, Q. Yuan, and X.-J. Bi, Phys. Rev. D, 91:063508 (2015)
[77]	S.-J. Lin, X.-J. Bi, P.-F. Yin, and Z.-H. Yu, arXiv:1504.07230
[78]	K. Hamaguchi, T. Moroi, and K. Nakayama, Physics Letters B, 747:523 (2015)
[79]	M. Ibe, S. Matsumoto, S. Shirai, and T. T. Yanagida, Phys. Rev. D, 91:111701 (2015)
[80]	C.-H. Chen, C.-W. Chiang, and T. Nomura, Physics Letters B, 747:495 (2015)
[81]	I. V. Moskalenko and A. W. Strong, ApJ, 493:694 (1998)
[82]	A. W. Strong and I. V. Moskalenko, ApJ, 509:212 (1998)
[83]	Y. Yang, L. Feng, X. Huang et al, J. Cosmology Astropart. Phys., 12:020 (2011)
[84]	K. Murase and J. F. Beacom, J. Cosmology Astropart. Phys., 10:043 (2012)
[85]	K. C. Y. Ng, R. Laha, S. Campbell et al, Phys. Rev. D, 89, 083001 (2014)

[1]	Hrishabh Bharadwaj , Ashok Goyal . Effective field theory approach to lepto-philic self-conjugate dark matter. Chinese Physics C, 2021, 45(2): 023114. doi: 10.1088/1674-1137/abce50
[2]	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
[3]	Guoli Liu , Fei Wang , Wenyu Wang , Jin-Min Yang . Explaining DAMPE results by dark matter with hierarchical lepton-specific Yukawa interactions. Chinese Physics C, 2018, 42(3): 035101. doi: 10.1088/1674-1137/42/3/035101
[4]	Andrea Addazi , Stephon Alexander , Yi-Fu Cai , Antonino Marcianó . Dark matter and baryogenesis in the Fermi-bounce curvaton mechanism. Chinese Physics C, 2018, 42(6): 065101. doi: 10.1088/1674-1137/42/6/065101
[5]	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
[6]	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
[7]	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
[8]	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
[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]	HU Jie , GONG Hao-Wei , LIN Qing , NI Kai-Xuan , TAN An-Di , WEI Yue-Huan , XIAO Meng-Jiao , XIAO Xiang , ZHAO Li . Development of the liquid level meters for the PandaX dark matter detector. Chinese Physics C, 2014, 38(5): 056002. doi: 10.1088/1674-1137/38/5/056002
[12]	YANG Jun . Have we found conclusive evidence for dark matter through direct detection experiments?. Chinese Physics C, 2014, 38(4): 045101. doi: 10.1088/1674-1137/38/4/045101
[13]	QIAO Qing-Peng , XU Bin . Dark-matter pair production at the ILC in the littlest Higgs model with T-parity. Chinese Physics C, 2013, 37(3): 033103. doi: 10.1088/1674-1137/37/3/033103
[14]	KANG Ke-Jun , YUE Qian , WU Yu-Cheng et al. (CDEX collaboration) and (TEXONO collaboration) . CDEX-1 1 kg point-contact germanium detector for low mass dark matter searches. Chinese Physics C, 2013, 37(12): 126002. doi: 10.1088/1674-1137/37/12/126002
[15]	CHEN Ya-Zheng , CHEN Jun-Mou , LUO Yan-An , SHEN Hong , LI Xue-Qian . Effects of nuclear deformation on the form factorfor direct dark matter detection. Chinese Physics C, 2012, 36(6): 505-512 . doi: 10.1088/1674-1137/36/6/005
[16]	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
[17]	TANG Zhi-Cheng , YUAN Qiang , BI Xiao-Jun , CHEN Guo-Ming . On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays. Chinese Physics C, 2011, 35(8): 725-734. doi: 10.1088/1674-1137/35/8/006
[18]	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
[19]	CAO Li-Gang . Superfluid nuclear matter in BCS theory and beyond. Chinese Physics C, 2009, 33(S1): 33-36. doi: 10.1088/1674-1137/33/S1/011
[20]	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

Access

Get Citation

null. Constraints on dark matter annihilation and decay from the isotropic gamma-ray background[J]. Chinese Physics C, 2017, 41(4): 045104. doi: 10.1088/1674-1137/41/4/045104

null. Constraints on dark matter annihilation and decay from the isotropic gamma-ray background[J]. Chinese Physics C, 2017, 41(4): 045104. doi: 10.1088/1674-1137/41/4/045104 shu

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2016-07-22
Revised: 2016-11-23

Fund

Supported by National Natural Science Foundation of China (11475189, 11475191, 11135009), 973 Program of China (2013CB837000), Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences (XDB09000000)

Article Metric

Article Views(1686)
PDF Downloads(31)
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, [email protected]

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Constraints on dark matter annihilation and decay from the isotropic gamma-ray background

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, [email protected]

Email This Article

Constraints on dark matter annihilation and decay from the isotropic gamma-ray background

HTML

目录