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Hossein Sadeghi

Researcher at Arak University

Publications -  248
Citations -  1761

Hossein Sadeghi is an academic researcher from Arak University. The author has contributed to research in topics: Salinity & Effective field theory. The author has an hindex of 18, co-authored 212 publications receiving 1322 citations. Previous affiliations of Hossein Sadeghi include Ferdowsi University of Mashhad & University of California, San Diego.

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Resonant Nano-particles Spheres as a Component of Nano-circuits

TL;DR: In this article, the effective permittivity for a material with two types of inclusions having two different electric polarizabilities have been calculated, and the effect of these inclusions on the permittivities has been analyzed.

Thermonuclear reaction rate of the 3 He (α, γ ) 7 Be process

TL;DR: In this paper , the reaction rate of the 3 He − α radiation capture process has been calculated in astrophysical energies using the pionless Effective Field Theory (EFT) and applying the Faddeev equation approach up to Next-to Leading Order (NLO) while taking Coulomb interaction into account.
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An update of the variant spectrum of the APC gene in Iranian familial adenomatous polyposis patients.

TL;DR: In this article , the authors evaluated pathogenic variants in exons of the APC gene in Iranian patients with FAP and found that the studying of APC alone for diagnosing FAP disease is not sufficient, and considering other genes are completely rational in the case of sequencing and studying the variants.
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Tunable Localized Resonances of Spherical Composite Particles at Optical and Near-Infrared Frequencies

TL;DR: In this article, the authors report on the design of spherical composite particles (SCPs) which consist of a homogeneous distribution of metal nano-particles (Ag) in a dielectric matrix.
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$$^{3}\hbox{He} - \alpha $$ 3 He - α

TL;DR: In this article , the amplitude, cross-section, and S-factor for the radiative capture reaction using the pionless Effective Field Theory (EFT) were computed using the Faddeev equation approach up to Next-to Leading Order in the astrophysical energy range.