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271. M. Sadegh, R. Mohammadi and I. Motie,
Generation of circular polarization in CMB radiation via nonlinear photon-photon interaction,
Phys. Rev. D 97(2018),   [abstract]   
Code: IPM/A-2017/53    
 
272. E. . Yusofi and M. . Mohsenzadeh,
Non-minimal Particle Creation from Asymptotic-de Sitter Inflation,
Springer 57(2018), 1622â??1630  [abstract]   
Code: IPM/A-2017/51    
 
273. Y. Wang, Y. Aimuratov, R. Moradi, M. Peresano, R. Ruffini and S. Shakeri,
Revisiting the Statistics of X-ray Flares in Gamma-ray Bursts,
THESEUS Workshop 2017 (2018),   [abstract]   
Code: IPM/A-2017/23    
 
274. R. Moradi, R. Ruffini, C. L. Bianco, Y.-C. Chen, M. Karlica, J. D. Melon Fuksman, D. Primorac, J. A. Rueda, S. Shakeri, Y. Wang and S. S. Xue,
Relativistic Behavior and Equitemporal Surfaces in Ultra-Relativistic Prompt Emission Phase of Gamma-Ray Bursts,
Springer 62(2018),   [abstract]   
Code: IPM/A-2018/38    
 
275. Seyed A. Hashemi, A. Javadi and J Th. van Loon,
From evolved stars to the evolution of IC1613,
MNRAS 483(2018),   [abstract]   
Code: IPM/A-2018/37    
 
276. N. Bartolo, A. Hoseinpour, G. Orlando, S. Matarrese and M. Zarei,
Photon-graviton scattering: A new way to detect anisotropic gravitational waves?,
Phys. Rev. D 98(2018),   [abstract]   
Code: IPM/A-2018/36    
 
277. H. He, H. Wang, M. Zhang, A. Mehrabi, Y. Yan and D. Yun,
Phase difference between long-term magnetic feature activity and flare activity of solar-type stars,
IAU 13(2018), 217-220  [abstract]   
Code: IPM/A-2018/35    
 
278. H. He, H. Wang, M. Zhang, A. Mehrabi, Y. Yan and D. Yun,
Activity Analyses for Solar-type Stars Observed with Kepler. II. Magnetic Feature versus Flare Activity,
Astrophysical Journal 236(2018),   [abstract]   
Code: IPM/A-2018/34    
 
279. S. Shakeri and A. Allahyari,
Circularly polarized EM radiation from GW binary sources,
JCAP 2018(2018),   [abstract]   
Code: IPM/A-2018/32    
 
280. S. Sheikhnezami,
Disk-outflow interaction: exchange of mass and angular momentum,
ZENODO (2018),   [abstract]   
Code: IPM/A-2018/30    
 

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