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 spectrumSokolova-Lapa E.,
Gornostaev M.,
Wilms J.,
Ballhausen R.,
Falkner S.,
Postnov K.,
Thalhammer P.,
Fürst F.,
García J.A.,
Shakura N.,
Becker P.A.,
Wolff M.T.,
Pottschmidt K.,
Härer L.,
Malacaria C. 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
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 targetsGostishchev, N. A.,
Kubankin, A. S.,
Nasonov, N. N.,
Polyanskii, V. V.,
Sergienko, V. I.,
Khablo, V. A. The spectra of the
polarization bremsstrahlung (PB) in the X-ray range induced by 7-MeV electrons