Dark-matter pair production at the ILC in the littlest Higgs model with <I>T</I>-parity

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Begeman K G, Broeils A H, Sanders R H. Mon. Not. Roy. Astron. Soc., 1991, 249: 523[2] Massey R et al. Nature, 2007, 445: 286[3] Roszkowski L. Phys. Lett. B, 1991 262: 59[4] Roszkowski L. arXiv:hepph/9903467[5] Primack J R. arXiv:astroph/0112255[6] Chen Pisin. arXiv:astroph/0303349[7] MA C P, Boylan-Kolchin M. Phys. Rev. Lett., 2004, 93: 021301[8] Bertone G, Hooper D, Silk J. Phys. Rept., 2005, 405: 279[9] Dreiner H K, Luhn C, Thormeier M. Phys. Rev. D, 2006, 73: 075007[10] Goldberg H. Phys. Rev. Lett., 1983, 50: 1419[11] Ellis J R, Hagelin J S, Nanopoulos D V et al. Nucl. Phys. B, 1984, 238: 453[12] CHENG H C, Low I. JHEP, 2004, 0408: 061[13] Low I. JHEP, 2004, 0410: 067[14] Skiba W, Terning J. Phys. Rev. D, 2003, 68: 075001[15] CHENG H C, Low I. JHEP, 2003, 0309: 051[16] Hubisz J, Meade P. Phys. Rev. D, 2005, 71: 035016[17] Birkedal A, Noble A, Perelstein M et al. Phys. Rev. D, 2006, 74: 035002[18] CHEN Ya-Zheng, LUO Yan-An, LI Lei et al. Commun. Theor. Phys., 2011, 55: 1059[19] QIAO Qing-Peng, TANG Jian, LI Xue-Qian. Commun. Theor. Phys., 2008, 50: 1211[20] CHEN Chian-Shu, Cheung Kingman, YUAN Tzu-Chiang. Phys. Lett. B, 2007, 644: 158[21] Cacciapaglia G, Deandrea A, Choudhury S R et al. Phys. Rev. D, 2010, 81: 075005[22] Nakamura K et al. J. Phys. G, 2010, 37: 075021[23] Khlopov M Y, Sakharov A S, Sudarikov A L. Grav. Cosmol., 1998, 4: S1[24] Belotsky K M, Khlopov M Y, Sakharov A S et al. Grav. Cosmol. Suppl., 1998, 4: 70[25] Bartl A, Fraas H, Majerotto W. Nucl. Phys. B, 1986, 278: 1[26] Carena M S, Freitas A. Phys. Rev. D, 2006, 74: 095004[27] Fayet P. Nucl. Phys. B, 1986, 263: 649[28] QIAO Qing-Peng, XU Bin. arXiv:hepph/1111.6155[29] Asakawa E, Asano M, Fujii K et al. Phys. Rev. D, 2009, 79: 075013