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Publications

1) B. Mirza, M. Zarei; Noncommutative Quantum Mechanics and the Aharonov-Casher Effect,Eur.Phys.J. C 32 (2004) 583, arXiv:hep-th/0311222v1.

2) B. Mirza, M. Zarei; Cancellation of Soft and Collinear Divergences in Noncommutative QED, Phys.Rev. D 74 (2006) 065019, arXiv:hep-th/0609181.

3) B. Mirza, R. Narimani, M. Zarei; Aharonov-Casher Effect for Spin One Particles in a Noncommutative Space, Eur.Phys.J. C 48 (2006) 641, arXiv:hep-th/0610323.

4) B. Mirza, M. Zarei; Effective Field Theory of a Locally Noncommutative Space-Time and Extra Dimensions, IJMPA, Vol. 23, Nos. 16 & 17 (2008) 2613 , : arXiv:0803.0232 [hep-th].

5) B. Mirza, M. Zarei; Wilsonian Effective Action for Noncommutative Gauge Theories Without UV/IR Mixing , Commun. Theor. Phys. (Beijing, China) 54 (2010) pp. 308–316.

6) M. Zarei, Short Distance Physics and Initial State Effects on the CMB Power, Phys. Rev. D 78, 123502 (2008), arXiv:0809.4312 [hep-th].

7) E. Bavarsad, M. Haghighat, Z. Rezaei, R. Mohammadi, I. Motie and M. Zarei, Generation of circular polarization of the CMB, Phys. Rev. D 81, 084035 (2010), arXiv:0912.2993 [hep-th].

8) M. Zarei, B. Mirza, Minimal Uncertainty in Momentum: The Effects of IR Gravity on Quantum Mechanics, Phys. Rev. D 79, 125007 (2009), arXiv:0901.1930 [hep-th].

9) R. Emami, H. Firouzjahi, S. M. Sadegh Movahed and M. Zarei, Anisotropic Inflation from Charged Scalar Fields, JCAP 1102 (2011) 005, arXiv:1010.5495v2 [astro-ph.CO] .

10) A. Maleknejad, M. Zarei, Slow-roll trajectories in Chromo-Natural and Gauge-flation Models, an exhaustive analysis, Phys. Rev. D 88 (2013) 043509, arXiv:1212.6760 [hep-th].

11)H. Firouzjahi, A. Green, K. Malik and M. Zarei, The Effect of Curvaton Decay on the Primordial Power Spectrum, PRD87 (2013) 103502, arXiv:1209.2652 [astro-ph.CO].

12) R. Emami, H. Firouzjahi and M. Zarei, Anisotropic Inflation with the non-Vacuum Initial State, PRD 90 (2014) 023504, arXiv:1401.4406 [hep-th].

13) M. Zarei, On the running of the spectral index to all orders: a new approach to constrain the inflationary models, arXiv:1408.6467v2 [astro-ph.CO].