Field-theoretic versus data-driven evaluations of electromagnetic corrections to hadronic vacuum polarization in $(g-2)_μ$
Eur.Phys.J.C, 2026, 86 (5), pp.497. (10.1140/epjc/s10052-026-15521-6)
Superfluid Dark Matter
Phys.Rept., 2026, 1172, pp.1-72. (10.1016/j.physrep.2026.02.001)
Euclid preparation: LXXVIII. Full-shape modelling of two-point and three-point correlation functions in real space
Astron.Astrophys., 2026, 707, pp.A228. (10.1051/0004-6361/202556177)
Possible Explanation of $F_2^n/F_2^p$ at Large $x$ Using Quantum Statistical Mechanics
Nucl.Phys.A, 2026, 1067, pp.123300. (10.1016/j.nuclphysa.2025.123300)
On the contribution from the light quarks to $H\toγγ, γZ$
Phys.Lett.B, 2026, 872, pp.140058. (10.1016/j.physletb.2025.140058)
Euclid preparation. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution
Astron.Astrophys., 2026, 708, pp.A105. (10.1051/0004-6361/202556642)
Moving superfluids in the rotating universe
JCAP, 2026, 05, pp.069. (10.1088/1475-7516/2026/05/069)
Time as a test-field: the no-boundary universe in motion and a smooth radiation bounce
Class.Quant.Grav., 2026, 43 (5), pp.055007. (10.1088/1361-6382/ae49de)
Gaussian Processes for Inferring Parton Distributions
JHEP, 2026, 04, pp.182. (10.1007/JHEP04(2026)182)
Black Hole Spectroscopy and Tests of General Relativity with GW250114
Phys.Rev.Lett., 2026, 136 (4), pp.041403. (10.1103/6c61-fm1n)