collaborators

6 papers

hep-ph2026

Chemical evolution of antimatter domains in early Universe

A. I. Dembitskaia, Stephane Weiss, M. Yu. Khlopov +1

According to modern physics, our Universe is baryon-asymmetric. That phenomenon can not be described in the frameworks of the Standard Model of particle physics. Globally, the Univ…

astro-ph.CO2026

Particle production and Higgs reheating

Aarav Shah, Kanabar Jay, Maxim Khlopov +2

Reheating is essential for transforming the cold, vacuum dominated Universe at the end of inflation into the hot thermal bath required by the Standard Model. In many well motivated…

hep-ph2025

Probing Lorentz Invariance Violation at High-Energy Colliders via Intermediate Massive Boson Mass Measurements: Z Boson Example

Z. Kepuladze, J. Jejelava

Lorentz invariance (LI) is a foundational principle of modern physics, yet its possible violation (LIV) remains an intriguing window to physics beyond the Standard Model. While str…

physics.gen-ph2025

How to present and interpret the Feynman diagrams in this theory describing fermion and boson fields in a unique way, in comparison with the Feynman diagrams so far presented and interpreted?

N. S. Mankoč Borštnik, H. B. Nielsen

Although the internal spaces describing spins and charges of fermions' and bosons' second-quantised fields have such different properties, yet we can all describe them equivalently…

gr-qc2025

Inferring the Merger History of Primordial Black Holes from Gravitational-Wave data and the Stochastic Signatures

Sourav Roy Chowdhury, Aritra Basak, Maxim Khlopov +1

Primordial black holes (PBHs) are well-motivated candidates for cold dark matter and may also account for a fraction of the binary black hole mergers observed by the LIGO-Virgo-KAG…

hep-ph2025

Strong primordial inhomogeneities induced by axion-like scalar field

Maxim A. Krasnov, Maxim Yu. Khlopov, Oem Trivedi

Our goal is to consider Axion-like particle (ALP) model to investigate the behaviour of space-time in the vicinity of the domain wall, induced by axion-like field. Here we present…