output
20172026
most citedHydrostatic-pressure effects on the pseudogap in slightly doped YBa2Cu3O7-δ single crystals

46 citations

14 papers

cond-mat.supr-con2026

Hydrostatic pressure effect on the pseudogap in Y0.77Pr0.23Ba2Cu3O7-δsingle crystals

A. L. Solovjov, L. V. Bludova, A. S. Kolesnik +6

We studied the changes of resistivity , superconducting transition temperature , fluctuation conductivity , and pseudogap of …

astro-ph.HE2026

The contribution to Galactic Centre γ-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations

M. Kalambay, M. Ishchenko, D. Kuvatova +2

The Galactic Centre γ-ray excess (GCE), observed by Fermi-LAT around Sgr A*, exceeds expectations from standard cosmic-ray models and is commonly attributed either to dark matter a…

astro-ph.GA2026

Evolution of fractality in centrally concentrated young clusters

Almat Akhmetali, Adilkhan Assilkhan, Mordecai-Mark Mac Low +6

We investigate the structural evolution of young star clusters forming within centrally concentrated molecular clouds. Our simulations use the Torch framework, which integrates the…

cond-mat.supr-con2025★ 6 cited

Study of fluctuation conductivity in YBaCuO-- films in strong magnetic fields

E. V. Petrenko, L. V. Omelchenko, Yu. A. Kolesnichenko +4

We report the effect of the \emph{ab}-plane magnetic field up to on the resistivity and fluctuation conductivity in YBaCuO thin f…

gr-qc2025★ 4 cited

Thermal properties of Klein-Gordon Oscillator in the Context of Amelino-Camelia and Magueijo-Smolin Doubly Special Relativity (DSR) frameworks

Abdelmalek Boumali, Nosratollah Jafari, Bekdaulet Shukirgaliyev +1

We examine the thermal and statistical properties of the one dimensional Klein-Gordon oscillator within two prominent Doubly Special Relativity (DSR) frameworks: Amelino-Camelia an…

astro-ph.GA2025★ 2 cited

Dynamical model of Praesepe and its tidal tails

L. Weis, C. West, A. Just +5

Context. The dynamical evolution of open clusters in the tidal field of the Milky Way and the feeding of the disc field star population depend strongly on the initial conditions at…