Кондратьев В.Н., Коровина Ю.В. «Универсальная статистика мягких повторяющихся гамма(МПГ)-всплесков» Физика элементарных частиц и атомного ядра, 49, № 1, с. 183-189 (2018)

Soft gamma-ray repeating (SGR) bursts are considered as a release of magnetic energy stored in the baryon degrees of freedom of magnetar crust. It is shown that such an interpretation allows one to systemize all the observations of such bursts, reveal and explain the universal statistical properties.

Панасюк М.И., Липунов В.М., Пак Ил, Свертилов С.И., Богомолов В.В., Горбовской Е.С., Амелюшкин А.М., Богомолов А.В., Июдин А.Ф., Кузнецова Е.А., Петров В.Л., Рожков Г.В., Яшин И.В. «Комплекс приборов для исследования космических гамма-всплесков на спутнике «Ломоносов»» Физика элементарных частиц и атомного ядра, 49, № 1, с. 190-196 (2018)

The scientific instruments on board “Lomonosov” satellite include a set of detectors designed to study gamma-ray and optical emission of cosmic gamma-ray bursts (GRB). Gamma spectrometer BDRG provides GRB trigger production and study of GRB spectral and temporal properties in the energy range 10–3000 keV as well as determining of the GRB source location by comparison of the readings of three differently directed detectors with an accuracy of a few degrees. Wide-field SHOK optical cameras have a field of view of ∼2×40 deg. They fix by the GRB trigger a set of images with a frequency of about 5 frames per second prior to the trigger and following it. UFFO instrument incorporates UBAT telescope with coding mask for measurements in hard X rays and soft gamma rays and optical telescope with a rotating mirror SMT, directed to the GRB source for ∼1 s to measure GRB prompt emission at the early stages.

Петков В.Б. «Изотропный поток нейтрино от взрывов сверхновых звезд во Вселенной» Физика элементарных частиц и атомного ядра, 49, № 1, с. 197-203 (2018)

The neutrinos of all types from core-collapse supernova explosions are accumulated in the Universe throughout the galaxies evolution. Isotropic and time-independent flux of such neutrinos is a guaranteed steady source of supernova neutrinos, which can give information about the supernovae dynamics and the supernovae redshift distribution. The current upper limits on the isotropic neutrino flux and prospects for the present and future experiments are discussed.

Покровский Ю.Е. «Компактные сгустки темной материи вблизи поверхности Солнца» Физика элементарных частиц и атомного ядра, 49, № 1, с. 204 (2018)

The solar surface oscillations observed at the Crimean Astrophysical Observatory (CrAO) at the frequency of 104.1890 μHz and at the Solar and Heliospheric Observatory (SoHO) at 220.72 Hz are considered as a result of existence of Compact Clumps of Dark Matter (CCDM) at orbits near the solar surface. These CCDM have to emit Gravitational Waves (GW) which are estimated to be the most intensive ones expected in the vicinity of the Earth and can be easily detected in the near future by means of the Evolved Laser Interferometer Space Antenna (eLISA). In addition to CCDM_CrAO and CCDM_SoHO, some other CCDM may exist in the solar structure. It is shown that GW radiated by most of these CCDM could be detected by eLISA even if the respective solar surface oscillations are too small to be observed.

Учайкин В.В., Сибатов Р.. «О пропагаторах нелокальной релятивистской диффузии галактических космических лучей» Физика элементарных частиц и атомного ядра, 49, № 1, с. 205-213 (2018)

Some propagators of cosmic rays (CR) in the Galaxy in view of qualitative features of the trajectories generated by them are discussed. Inconsistencies of known models with the relativistic principle of limited speed and with large-scale turbulence of the interstellar medium are indicated. Analytical expressions for propagators of the nonlocal transport theory being free from these shortcomings are presented.