


Том 167, № 1 (2025)
ATOMS, MOLECULES, OPTICS
O VREMENAKh ZhIZNI KVAZISTATsIONARNYKh UROVNEY PRI TUNNELIROVANII V REZONANSNO-TUNNEL'NOY STRUKTURE
Аннотация



INDUTsIROVANNYE VUF-IMPUL'SOM KANALY GENERATsII IZLUChENIYa ATOMOM V INTENSIVNOM LAZERNOM IK-POLE
Аннотация



NUCLEI, PARTICLES, FIELDS, GRAVITY AND ASTROPHYSICS
OTSKOK V NEMINIMAL'NOY EFFEKTIVNOY MODELI SKALYaRNO-TENZORNOY GRAVITATsII
Аннотация



SPINOR FIELD IN FLRW COSMOLOGY: SPHERICALLY SYMMETRIC CASE
Аннотация
Within the scope of a spherically symmetric FLRW cosmological model we have studied the role of nonlinear spinor field in evolution of the universe. It is found that if the FLRW model given by the spherical coordinates the energy-momentum tensor (EMT) of the spinor field possesses nontrivial non-diagonal components. These non-diagonal components of EMT neither depend on the spinor field nonlinearity nor on the value of parameter k defining the type of curvature of the FLRW model. The presence of such components imposes some restrictions on the spinor field. The problem is studied for open, flat and close geometries. In doing so we exploited the spinor description of sources such as perfect fluid and dark energies. Some qualitative numerical solutions are given.






SOLIDS AND LIQUIDS
KANALIROVANIE NEYTRONOV V MAGNITNOM PLOSKOM VOLNOVODE
Аннотация



DIAELASTIChESKIY EFFEKT V ALYuMINII POSLE VOZDEYSTVIYa NANOSEKUNDNYMI LAZERNYMI IMPUL'SAMI UL'TRAFIOLETOVOGO DIAPAZONA
Аннотация



ORDER, DISORDER AND PHASE TRANSITIONS IN CONDENSED MATTER
DVUMERNYE MAGNITOPLAZMONY V POLOSE KONEChNOY ShIRINY
Аннотация



KVANTOVYY SU(Z)-FERRIMAGNETIK NA TREUGOL'NOY REShETKE V MAGNITNOM POLE
Аннотация



STATsIONARNYY I NESTATsIONARNYY TOK V KONEChNYKh TsEPOChKAKh KITAEVA
Аннотация



STATISTICAL AND NONLINEAR PHYSICS, PHYSICS OF "SOFT" MATTER
SUPRATHERMAL ELECTRON TRANSPORT IN WEAKLY AND STRONGLY MAGNETIZED ASTROPHYSICAL PLASMAS INCLUDING COULOMB COLLISIONAL EFFECTS
Аннотация
This study examines electron transport in astrophysical plasmas mediated by Coulomb collisions and collisionless wave-particle interactions, using a kinetic transport model that incorporates spectral evolutions through these interactions. It investigates the transport of suprathermal electrons via whistler turbulence and the effects of plasma magnetization. Key findings indicate that in strongly magnetized plasmas, diffusion timescales in pitch angle space become saturated at large pitch angles, independent of increasing magnetic field strength. Conversely, in weakly magnetized plasmas, these timescales decrease with decreasing magnetic field strength, enhancing electron transport in velocity space. The study also identifies minimum conditions for resonant scattering, dominated by wave-particle interactions over Coulomb collisions, which depend on Coulomb collision effects and the power-law slope of the whistler turbulence spectrum. These findings have applications in weakly magnetized astrophysical plasmas, from the relatively strong magnetic fields of the interplanetary medium to the very weak magnetic fields of the intracluster medium.



REZONANSNYE VOLNOVODNYE POTERI LYuMINESTsENTsII V SLOE ZhIDKOGO KRISTALLA, OGRANIChENNOGO ITO-ELEKTRODAMI
Аннотация


