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Wiggly whipped inflationMotivated by BICEP2 results on the CMB polarization B-mode which imply primordial gravitational

X-ray emission from magnetized neutron star atmospheres at low mass-accretion rates: I. Phase-averaged spectrum excitations of electrons. The strongly polarized emitted spectrum has a double-hump shape that is observed

Influence of Compton scattering on the broad-band X-ray spectra of intermediate polars the observed X-ray spectrum of intermediate polars. Methods. We construct the model of the post-shock region

Effective spectrum width of the synchrotron radiation to the ultrarelativistic limit of SR, the effective width of the spectrum is calculated for the polarization components

DEFECTS IN CHOLESTERIC LIQUID CRYSTALS

Wiggly whipped inflationMotivated by BICEP2 results on the CMB polarization B-mode which imply primordial gravitational

Polarization exchange of optical eigenmode pair in twisted-nematic Fabry-Pérot resonatorThe polarization exchange effect in a twisted-nematic Fabry-Pérot resonator is experimentally

Influence of Compton scattering on the broad-band X-ray spectra of intermediate polars the observed X-ray spectrum of intermediate polars. Methods. We construct the model of the post-shock region

Spectral and polarization properties of a ‘cholesteric liquid crystal—phase plate—metal’ structure. The nonreciprocal transmission of polarized light propagating in the forward and backward directions is established

Angular dependence of the coherent peak position in the polarization bremsstrahlung spectrum of relativistic electrons in polycrystalline targetsThe spectra of the polarization bremsstrahlung (PB) in the X-ray range induced by 7-MeV electrons

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