PandaX limits on the light dark matter with a light mediator in the singlet extension of MSSM

[1]
T. Bringmann, J. Hasenkamp, and J. Kersten, arXiv: 1312.4947 [hep-ph].
[2]
A. A. Klypin, A. V. Kravtsov, O. Valenzuela et al., Astrophys. J., 522: 82 (1999)
[3]
A. V. Kravtsov, Adv. Astron., 2010: 281913 (2010)
[4]
J. Zavala et al., Astrophys. J., 700: 1779 (2009)
[5]
R. K. de Naray and K. Spekkens, Astrophys. J., 741: L29 (2011)
[6]
M. G. Walker and J. Penarrubia, Astrophys. J., 742: 20 (2011)
[7]
M. Boylan-Kolchin, J. S. Bullock, and M. Kaplinghat, Mon. Not. Roy. Astron. Soc., 415: L40 (2011)
[8]
M. Boylan-Kolchin, J. S. Bullock, and M. Kaplinghat, Mon. Not. Roy. Astron. Soc., 422: 1203 (2012)
[9]
J. L. Feng, H. Tu, and H. B. Yu, JCAP, 0810: 043 (2008), arXiv:0808.2318[hep-ph
[10]
R. Foot and S. Vagnozzi, Phys. Rev. D, 91: 023512 (2015), arXiv:1409.7174[hep-ph
[11]
M. Blennow, S. Clementz, and J. Herrero-Garcia, JCAP, 1703(03): 048 (2017), arXiv:1612.06681[hep-ph
[12]
S. Tulin, H. -B. Yu, and K. M. Zurek, Phys. Rev. Lett., 110: 111301 (2013)
[13]
S. Tulin, H. -B. Yu, and K. M. Zurek, Phys. Rev. D, 87: 115007 (2013)
[14]
P. Ko and Y. Tang, JCAP, 1405: 047 (2014)
[15]
P. Ko and Y. Tang, Phys. Lett. B, 739: 62 (2014)
[16]
R. Foot, Phys. Rev. D, 69: 036001 (2004), arXiv:hep-ph/0308254
[17]
T. Li, S. Miao, and Y. F. Zhou, JCAP, 1503(03): 032 (2015), arXiv:1412.6220[hep-ph
[18]
E. Del Nobile, M. Kaplinghat, and H. B. Yu, JCAP, 1510(10): 055 (2015), arXiv:1507.04007[hep-ph
[19]
F. Kahlhoefer, S. Kulkarni, and S. Wild, JCAP, 1711(11): 016 (2017), arXiv:1707.08571[hep-ph
[20]
X. Ren et al. (PandaX-II Collaboration), Phys. Rev. Lett., 121(2): 021304 (2018), arXiv:1802.06912[hep-ph
[21]
P. Fayet, Nucl. Phys. B, 90: 104 (1975)
[22]
P. Fayet, Phys. Lett. B, 69: 489 (1977)
[23]
For pheno studies of NMSSM, see, e.g., J. R. Ellis et al., Phys. Rev. D, 39: 844 (1989)
[24]
M. Drees, Int. J. Mod. Phys. A, 4: 3635 (1989)
[25]
P. N. Pandita, Phys. Lett. B, 318: 338 (1993)
[26]
P. N. Pandita, Phys. Rev. D, 50: 571 (1994)
[27]
S. F. King and P. L. White, Phys. Rev. D, 52: 4183 (1995)
[28]
B. Ananthanarayan and P. N. Pandita, Phys. Lett. B, 353: 70 (1995)
[29]
B. Ananthanarayan and P. N. Pandita, Phys. Lett. B, 371: 245 (1996)
[30]
W. Wang, Z. Xiong, and J. M. Yang, Phys. Lett. B, 680: 167 (2009)
[31]
J. Cao and J. M. Yang, Phys. Rev. D, 78: 115001 (2008)
[32]
A. Kaminska, G. G. Ross, K. Schmidt-Hoberg et al., arXiv: 1401.1816 [hep-ph]
[33]
H. M. Lee et al., Nucl. Phys. B, 850: 1 (2011) arXiv: 1102.3595 [hep-ph]
[34]
G. G. Ross and K. Schmidt-Hoberg, Nucl. Phys. B, 862: 710 (2012), arXiv: 1108.1284 [hep-ph]
[35]
A. Kaminska, G. G. Ross, and K. Schmidt-Hoberg, JHEP, 1311: 209 (2013)
[36]
G. G. Ross, K. Schmidt-Hoberg, and F. Staub, JHEP, 1208: 074 (2012)
[37]
K. Schmidt-Hoberg, F. Staub, and M. W. Winkler, JHEP, 1301: 124 (2013)
[38]
K. Schmidt-Hoberg and F. Staub, JHEP, 1210: 195 (2012)
[39]
J. Cao et al., JHEP, 1203: 086 (2012), arXiv:1202.5821[hep-ph
[40]
J. E. Kim and H. P. Nilles, Phys. Lett. B, 138: 150 (1984)
[41]
J. Cao et al., JHEP 1405: 056 (2014)
[42]
J. Cao et al., Phys. Lett. B, 703: 292 (2011)
[43]
J. Cao et al., JHEP, 1007: 044 (2010)
[44]
W. Wang, Z. Xiong, J. M. Yang et al., JHEP, 0911: 053 (2009)
[45]
D. Hooper and T. M. P. Tait, arXiv: 0906.0362 [hep-ph].
[46]
F. Wang, W. Wang, J. M. Yang et al., Phys. Rev. D, 90: 035028 (2014), arXiv:1404.6705[hep-ph
[47]
J. Cao et al., Phys. Rev. D, 82: 051701 (2010)
[48]
M. Abdughani, L. Wu, and J. M. Yang, Eur. Phys. J. C, 78(1): 4 (2018), arXiv: 1705.09164 [hep-ph]
[49]
M. Abdughani et al., JHEP, 1911: 095 (2019), arXiv: 1909.07792 [hep-ph]
[50]
F. Wang, W. Wang, and J. M. Yang, Eur. Phys. J. C, 74(10): 3121 (2014)
[51]
P. Draper et al., Phys. Rev. Lett., 106: 121805 (2011)
[52]
R. Bernabei et al. (DAMA and LIBRA Collaborations), Eur. Phys. J. C, 67: 39 (2010), arXiv:1002.1028[astro-ph.GA
[53]
J. Ren, L. Wu, J. M. Yang et al., Nucl. Phys. B, 943: 114613 (2019), arXiv: 1708.06615 [hep-ph]
[54]
M. Abdughani et al., Commun. Theor. Phys., 71: 955 (2019), arXiv: 1905.06047 [hep-ph]
[55]
U. Ellwanger, J. F. Gunion, and C. Hugonie, JHEP, 0502: 066 (2005)
[56]
http://www.sciops.esa.int/SA/PLANCK/docs/Planck 2013 results.
[57]
H. Jiang et al. (CDEX Collaboration), Phys. Rev. Lett., 120(24): 241301 (2018), arXiv:1802.09016[hep-ex
[58]
R. Agnese et al. (SuperCDMS Collaboration), Phys. Rev. Lett., 116(7): 071301 (2016), arXiv:1509.02448[astro-ph.CO
[59]
F. Petricca et al. (CRESST Collaboration), arXiv: 1711.07692 [astro-ph.CO]
[60]
D. S. Akerib et al. (LUX Collaboration), Phys. Rev. Lett., 118(2): 021303 (2017), arXiv:1608.07648[astro-ph.CO
[61]
E. Aprile et al. (XENON Collaboration), arXiv: 1805.12562 [astro-ph.CO]
[62]
M. Drees and M. Nojiri, Phys. Rev. D, 48: 3483 (1993)
[63]
G. Belanger, F. Boudjema, A. Pukhov et al., Comput. Phys. Commun., 180: 747 (2009)
[64]
W. Wang, M. Zhang, and J. Zhao, Int. J. Mod. Phys. A, 33(11): 1841002 (2018), arXiv:1604.00123[hep-ph
[65]
H. J. Kang and W. Wang, Commun. Theor. Phys., 65(4): 499 (2016), arXiv:1601.00373[hep-ph
[66]
T. Bringmann and M. Pospelov, Phys. Rev. Lett., 122(17): 171801 (2019), arXiv: 1810.10543 [hep-ph]
[67]
J. B. Dent, B. Dutta, J. L. Newstead et al., arXiv: 1907.03782 [hep-ph]
[68]
K. Bondarenko et al., arXiv: 1909.08632 [hep-ph]
[69]
W. Wang et al., arXiv: 1912.09904 [hep-ph]
[70]
G. Ambrosi et al. (DAMPE Collaboration), Nature, 552: 63 (2017)
[71]
See, e.g., G. H. Duan et al., JHEP, 1802: 107 (2018), arXiv: 1711.11012 [hep-ph]
[72]
G. H. Duan et al., Eur. Phys. J. C, 78(4): 323 (2018), arXiv: 1711.11563 [hep-ph]
[73]
G. L. Liu, F. Wang, W. Wang et al., Chin. Phys. C, 42(3): 035101 (2018), arXiv: 1712.02381 [hep-ph]