[1] Manuel Drees（Bonn U.）, Hoernisa Iminniyaz( 吾尔泥沙. 依明尼亚孜，Bonn U.& Xinjiang U. ) and Mitsuru Kakizaki（Bonn U.）,“ Abundance of cosmological relics in low-temperature scenarios”, Phys.Rev.D73: 123502, 2006
[2]Manuel Drees（Bonn U.）, Hoernisa Iminniyaz (吾尔泥沙.依明尼亚孜，，Bonn U. & Xinjiang U.) and Mitsuru Kakizaki(Bonn U.), “Constraints on the very early universe from thermal WIMP dark matter”, Phys.Rev.D76:103524, 2007
[3] Pavel Fileviez Perez（Wisconsin U.）, Hoernisa Iminniyaz (吾尔泥沙.依明尼亚孜，Xinjiang U.)， German Rodrigo（Valencia U.）, “Proton Stability, Dark Matter and Light Color Octet Scalars in Adjoint SU(5) Unification”, Phys. Rev. D78: 015013, 2008
[4]Pavel Fileviez Perez（Wisconsin U.）, Hoernisa Iminniyaz (吾尔泥沙.依明尼亚孜，Peking U.，CHEP & Xinjiang U.)， German Rodrigo（Valencia U.），Sogee Spinner（Wisconsin U.）, “Gauge Mediated SUSY Breaking via Seesaw”, Phys. Rev.D81: 095013, 2010
[5] Hoernisa Iminniyaz* (吾尔泥沙.依明尼亚孜,Peking U.，CHEP & Xinjiang U.), Mitsuru Kakizaki（Annecy，LAPTH）, “Thermal abundance of non-relativistic relics with Sommerfeld enhancement”， Nuclear Physics B， 851， 57， 2011
[6]Hoernisa Iminniyaz（吾尔尼沙.依明尼亚孜,Xinjiang U.）, Manuel Drees (Bonn U.), Xuelei Chen (Beijing Observ.),“Relic Abundance of Asymmetric Dark Matter”，Journal of Cosmology and Astroparticle Physics，07, 003, 2011
[7]Hoernisa Iminniyaz*（吾尔尼沙.依明尼亚孜,Xinjiang U.& Peking U., CHEP）, Xuelei Chen(Peking U.,CHEP & Beijing Observ.), Xiaojun Bi（Beijing, Inst.High Energy Phys.）,Sayipjamal Dulat(Xinjiang U.), “The effects of kinetic decoupling on the relic density with Sommerfeld enhancement”, Commun. Theor. Phys， 第56 卷，第5 期， 967， 2011
[8]Hoernisa Iminniyaz*（吾尔尼沙.依明尼亚孜, Xinjiang U.）,“Relic Density of WIMPs in Kination Models”, 星际APP官网学报（自然科学版），第29 卷, 第3 期, 313，2012
[9]Hoernisa Iminniyaz*（吾尔尼沙.依明尼亚孜, Xinjiang U.）, “Comments on 'Thermal relic abundances of particles with velocity-dependent interactions' ”, Physics Letters B,723, 255-256, 2013.
[10]Hoernisa Iminniyaz* ( 吾尔尼沙. 依明尼亚孜, Xinjiang U.), Xuelei Chen (Peking U.,CHEP & Beijing Observ.),“Relic Abundance of Asymmetric Dark Matter in Quintessence ”. Astropart.Phys. 54, 125-131, 2014.
[11]Shun-zhi Wang（Shanghai University of Engineering）, Hoernisa Iminniyaz*（吾尔尼沙.依明尼亚孜, Xinjiang U.,通讯作者），Mamatrishat Mamat（买买提热夏提，买买提，Xinjiang U.），“Relic Abundance of Asymmetric Dark Matter and the Scalar--Tensor Model”, Int.J.Mod.Phys. A31, no.07, 1650021, 2016.
[12]Haximjan Abdusattar（Xinjiang U.），Hoernisa Iminniyaz*（吾尔尼沙.依明尼亚孜,Xinjiang U., 通讯作者），“Abundance of Asymmetric Dark Matter in Brane World Cosmology”,Commun.Theor.Phys. 66, no.3, 363-368, 2016
[13]Hoernisa Iminniyaz*(吾尔尼沙.依明尼亚孜,Xinjiang U.)，“Asymmetric Dark Matter in the Shear-dominated Universe”，Phys.Lett.B765, 6-10, 2017.
[14]Guoliang Lü(Xinjiang U.), Chunhua Zhu (Xinjiang U.), Zhaojun Wang (Xinjiang U.), and Hoernisa Iminniyaz(吾尔尼沙.依明尼亚孜,Xinjiang U.)，“Effects of Irradiation on the Evolution of Ultracompact X-Ray Binaries”，The Astrophysical Journal, 847:62(7pp) 2017.
[15] Hoernisa Iminniyaz*(吾尔尼沙.依明尼亚孜,Xinjiang U.), B.Salai(博尔汗·沙来) and G.Lv,“Relic Density of Asymmetric Dark Matter in Modified Cosmological Scenarios”，Commun. Theor. Phys. 70， No.5, 602，2018 |
