output
20032026
most citedStrongly correlated flat-band systems: The route from Heisenberg spins to Hubbard electrons

243 citations

Showing 2014Show all

16 papers · 1 filter

quant-ph201412 cited

Perturbation of the ns energy levels of the hydrogen atom in rotationally invariant noncommutative space

Kh. P. Gnatenko, Yu. S. Krynytskyi, V. M. Tkachuk

Noncommutative space which is rotationally invariant is considered. The hydrogen atom is studied in this space. We exactly find the leading term in the asymptotic expansion of the…

math.MG20143 cited

Coarse classification of abelian groups and amenable shift-homogeneous metric spaces

Taras Banakh, Matija Cencelj, Dušan Repovš +1

In this paper we classify countable locally finite-by-abelian groups up to coarse isomorphism. This classification is derived from a coarse classification of amenable shift-homogen…

cond-mat.str-el201414 cited

Frustrated diamond-chain quantum Heisenberg antiferromagnet in a magnetic field

Johannes Richter, Olesia Krupnitska, Taras Krokhmalskii +1

We consider the antiferromagnetic spin-1/2 Heisenberg model on a frustrated diamond-chain lattice in a - or -aligned external magnetic field. We use the strong-coupling…

astro-ph.HE20142 cited

Probing cluster environments of blazars through gamma-gamma absorption

Iurii Sushch, Markus Böttcher

Most blazars are known to be hosted in giant elliptic galaxies, but their cluster environments have not been thoroughly investigated. Cluster environments may contain radiation fie…

hep-th2014

Tunnelling of scalar and Dirac particles from squashed charged rotating Kaluza-Klein black holes

M. M. Stetsko

Thermal radiation of scalar particles and Dirac fermions from squashed charged rotating five-dimensional black holes is considered. To obtain temperature of the black holes we use…

astro-ph.HE2014

Pair Cascades in the Disk Environment of the Binary System PSR B1259-63/LS 2883

Iurii Sushch, Markus Böttcher

PSR B1259-63/LS 2883 is a very high energy (VHE; GeV) γ-ray emitting binary consisting of a 48 ms pulsar orbiting around a Be star with a period of years. The B…