activity
20152025
most citedA facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case

782 citations · 1.7k across the 40 of their papers we have counts for

collaborators

41 papers

astro-ph.CO2025

3D matter power spectrum correspondence to 1D Lyman-alpha flux power spectrum

Ivan Ridkokasha, Andres Aramburo-Garcia, Kyrylo Bondarenko +3

The 3D distribution of matter at small scales encodes valuable information about the nature of dark matter and other fundamental physics. A prominent probe of such scales outside g…

hep-ex2024★ 4 cited

Reconstruction of 400 GeV/c proton interactions with the SHiP-charm project

SHiP Collaboration

The SHiP-charm project was proposed to measure the associated charm production induced by 400 GeV/c protons in a thick target, including the contribution from cascade production. A…

astro-ph.CO2024

Dark photon constraints from CMB temperature anisotropies

Andres Aramburo-Garcia, Kyrylo Bondarenko, Alexey Boyarsky +6

The resonant conversion, within the inter-galactic medium, of regular photons into dark photons amplifies the anisotropy observed in the CMB, thereby imposing stringent constraints…

astro-ph.CO2024★ 1 cited

Probing intergalactic intergalactic magnetic fields with LOFAR LoTSS DR2 data

Kyrylo Bondarenko, Alexey Boyarsky, Anastasia Sokolenko +1

We use Faraday rotation measurements from the latest catalog LoTSS DR2 from LOFAR to probe intergalactic magnetic fields. To identify the extragalactic component of the observed ro…

hep-ph2023★ 1 cited

Unveiling new physics with discoveries at Intensity Frontier

Oleksii Mikulenko, Kyrylo Bondarenko, Alexey Boyarsky +1

The idea of feebly interacting particles (FIPs) has emerged as an important approach to address challenges beyond the Standard Model. The next generation of Intensity Frontier expe…

hep-ph2023

New physics at the Intensity Frontier: how much can we learn and how?

Oleksii Mikulenko, Kyrylo Bondarenko, Alexey Boyarsky +1

Intensity Frontier experiments are often evaluated by the smallest coupling it can probe, irrespective of what particle can be found or the scientific significance of its detection…

hep-ph2023

Sensitivities to feebly interacting particles: public and unified calculations

Maksym Ovchynnikov, Jean-Loup Tastet, Oleksii Mikulenko +1

The increasing interest in Long-Lived Particles (LLPs) has led to numerous proposed experiments in order to search for them. However, the sensitivity estimates published by these e…

hep-ph2023

Best-case scenarios for neutrino capture experiments

Kyrylo Bondarenko, Alexey Boyarsky, Josef Pradler +1

A direct discovery of the cosmic neutrino background would bring to a closure the searches for relic left-over radiation predicted by the Hot Big Bang cosmology. Recently, the KATR…

hep-ph2023★ 37 cited

Sensitivities to feebly interacting particles: public and unified calculations

Maksym Ovchynnikov, Jean-Loup Tastet, Oleksii Mikulenko +1

The idea that new physics could take the form of feebly interacting particles (FIPs) - particles with a mass below the electroweak scale, but which may have evaded detection due to…

hep-ph2023★ 6 cited

Towards the optimal beam dump experiment to search for feebly interacting particles

Kyrylo Bondarenko, Alexey Boyarsky, Oleksii Mikulenko +2

Future searches for new physics beyond the Standard Model are without doubt in need of a diverse approach and experiments with complementary sensitivities to different types of cla…

hep-ph2022★ 14 cited

Sensitivity of the FACET experiment to Heavy Neutral Leptons and Dark Scalars

Maksym Ovchynnikov, Viktor Kryshtal, Kyrylo Bondarenko

We analyze the potential of the recently proposed experiment FACET (Forward-Aperture CMS ExTension) to search for new physics. As an example, we consider the models of Higgs-like s…

astro-ph.CO2022★ 7 cited

The contribution of magnetized galactic outflows to extragalactic Faraday rotation

Andres Aramburo-Garcia, Kyrylo Bondarenko, Alexey Boyarsky +3

Galactic outflows driven by star formation and active galactic nuclei blow bubbles into their local environments, causing galactic magnetic fields to be carried into intergalactic…

astro-ph.CO2022★ 11 cited

Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation

Andres Aramburo-Garcia, Kyrylo Bondarenko, Alexey Boyarsky +3

Previously derived Faraday rotation constraints on the volume-filling intergalactic magnetic field (IGMF) have used analytic models that made a range of simplifying assumptions abo…

hep-ph2022

Neutron stars as photon double-lenses: constraining resonant conversion into ALPs

Kyrylo Bondarenko, Alexey Boyarsky, Josef Pradler +1

Axion-photon conversion is a prime mechanism to detect axion-like particles that share a coupling to the photon. We point out that in the vicinity of neutron stars with strong magn…

physics.ins-det2021★ 2 cited

Track reconstruction and matching between emulsion and silicon pixel detectors for the SHiP-charm experiment

SHiP Collaboration

In July 2018 an optimization run for the proposed charm cross section measurement for SHiP was performed at the CERN SPS. A heavy, moving target instrumented with nuclear emulsion…

physics.ins-det2021

The SHiP experiment at the proposed CERN SPS Beam Dump Facility

SHIP Collaboration

The Search for Hidden Particles (SHiP) Collaboration has proposed a general-purpose experimental facility operating in beam-dump mode at the CERN SPS accelerator to search for ligh…

hep-ph2021★ 3 cited

Production of Chern-Simons bosons in decays of mesons

Yuliia Borysenkova, Pavlo Kashko, Mariia Tsarenkova +2

We consider the effective interaction of quarks with a new GeV-scale vector particle that couples to electroweak gauge bosons by the so-called effective Chern-Simons interaction. W…

astro-ph.CO2021★ 19 cited

Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields

Kyrylo Bondarenko, Alexey Boyarsky, Alexander Korochkin +3

Intergalactic magnetic fields in the voids of the large-scale structure can be probed via measurements of secondary gamma-ray emission from gamma-ray interactions with extragalacti…

astro-ph.HE2021★ 16 cited

Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field

Andres Aramburo Garcia, Kyrylo Bondarenko, Alexey Boyarsky +3

The origin and composition of ultra-high energy cosmic rays (UHECRs) remain a mystery. The common lore is that UHECRs are deflected from their primary directions by the Galactic an…

hep-ph2021★ 42 cited

An allowed window for heavy neutral leptons below the kaon mass

Kyrylo Bondarenko, Alexey Boyarsky, Juraj Klaric +4

The extension of the Standard Model with two gauge-singlet Majorana fermions can simultaneously explain two beyond-the-Standard-model phenomena: neutrino masses and oscillations, a…

astro-ph.CO2020★ 7 cited

Probing sub-eV Dark Matter decays with PTOLEMY

Kyrylo Bondarenko, Alexey Boyarsky, Marco Nikolic +2

When the Dark Matter mass is below the eV-scale, its cosmological occupation number exceeds the ones of photons from the cosmic microwave background as well as of relic neutrinos.…

astro-ph.CO2020★ 42 cited

Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles

Andres Aramburo Garcia, Kyrylo Bondarenko, Alexey Boyarsky +3

We study the effects of galaxy formation physics on the magnetization of the intergalactic medium (IGM) using the IllustrisTNG simulations. We demonstrate that large-scale regions…

hep-ph2020★ 56 cited

New Constraints on the Mass of Fermionic Dark Matter from Dwarf Spheroidal Galaxies

James Alvey, Nashwan Sabti, Victoria Tiki +7

Dwarf spheroidal galaxies are excellent systems to probe the nature of fermionic dark matter due to their high observed dark matter phase-space density. In this work, we review, re…

astro-ph.CO2020★ 20 cited

From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass

Kyrylo Bondarenko, Anastasia Sokolenko, Alexey Boyarsky +3

In this paper we study the density profiles of self-interacting dark matter (SIDM) haloes spanning the full observable mass range, from dwarf galaxies to galaxy clusters. Using rea…