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Autor:
Samonin, V.1 (AUTHOR) samonin@lti-gti.ru, Morozova, V.1 (AUTHOR), Podvyaznikov, M.1 (AUTHOR), Reverberi, A.2 (AUTHOR), Meshalkin, V.3 (AUTHOR), Kulov, N.4 (AUTHOR), Garabadzhiu, A.1 (AUTHOR)
Publikováno v:
Theoretical Foundations of Chemical Engineering. Jun2023, Vol. 57 Issue 3, p338-349. 12p.
Autor:
Morozova, V., Piro, A. L., Renzo, M., Ott, C. D., Clausen, D., Couch, S. M., Ellis, J., Roberts, L. F.
We present the SuperNova Explosion Code (SNEC), an open-source Lagrangian code for the hydrodynamics and equilibrium-diffusion radiation transport in the expanding envelopes of supernovae. Given a model of a progenitor star, an explosion energy, and
Externí odkaz:
http://arxiv.org/abs/1505.06746
Publikováno v:
Astrophys Space Sci (2010) 330: 257-266
Plasma magnetosphere surrounding rotating magnetized neutron star in the braneworld has been studied. For the simplicity of calculations Goldreich-Julian charge density is analyzed for the aligned neutron star with zero inclination between magnetic f
Externí odkaz:
http://arxiv.org/abs/1004.4111
We study the magnetosphere of a slowly rotating magnetized neutron star subject to toroidal oscillations in the relativistic regime. Under the assumption of a zero inclination angle between the magnetic moment and the angular momentum of the star, we
Externí odkaz:
http://arxiv.org/abs/1004.1739
Autor:
Ahmedov, B. J., Morozova, V. S.
The notion of death line of rotating pulsars is applied to model of oscillating neutron stars. It is shown that the magnetosphere of typical non-rotating oscillating stars may not contain secondary plasma to support the generation of radio emission i
Externí odkaz:
http://arxiv.org/abs/0901.1008
We study magnetospheric structure surrounding rotating magnetized neutron star with nonvanishing NUT (Newman-Tamburino-Unti) parameter. For the simplicity of calculations Goldreich-Julian charge density is analyzed for the aligned neutron star with z
Externí odkaz:
http://arxiv.org/abs/0806.2376
Autor:
Morozova, V. S., Ahmedov, B. J.
Publikováno v:
Int.J.Mod.Phys.D18:107-118,2009
General relativistic quantum interference effects in the slowly rotating NUT space-time as the Sagnac effect and the phase shift effect of interfering particle in neutron interferometer are considered. It was found that in the case of the Sagnac effe
Externí odkaz:
http://arxiv.org/abs/0804.2786
Autor:
SPHINX Collaboration, Antipov, Yu., Artamonov, A., Batarin, V., Bezzubov, V., Eroshin, O., Golovkin, S., Gorin, Yu., Govorun, V., Isaev, A., Kolganov, V., Konstantinov, A., Kozhevnikov, A., Kubarovsky, V., Kurshetsov, V., Kushnirenko, A., Landsberg, L., Leontiev, V., Lomkatsi, G., Medinskiy, M., Medovikov, V., Molchanov, V., Morozova, V., Mukhin, V., Nilov, A., Patalakha, D., Petrenko, S., Petrukhin, A., Rykalin, V., Senko, V., Shalanda, N., Smolyankin, V., Sytin, A., Vaniev, V., Vavilov, D., Victorov, V., Yakimchuk, V., Zimin, S.
The paper describes the SPHINX facility which includes a wide-aperture magnetic spectrometer with scintillation counters and hodoscopes, proportional chambers and drift tubes, multichannel electromagnetic and hadron calorimeters, a guard system, a RI
Externí odkaz:
http://arxiv.org/abs/physics/0504035
Publikováno v:
Physics of Particles & Nuclei Letters; Aug2024, Vol. 21 Issue 4, p747-749, 3p