papers

Publications (23)

hep-ph2025

The model meets the new data and muon neutrino trident scattering

Ming-Wei Li, Xiao-Gang He, Andrew Cheek +1

The Muon collaboration at Fermilab has announced their final result of the anomalous magnetic moment of the muon. By adopting the lattice-QCD evaluation of the leading-order…

hep-ph2025

Using to constrain preferred axion model dark matter

Andrew Cheek, Ui Min

Preferred axion models are minimal realizations of the Peccei-Quinn solution to the strong CP problem while providing a dark matter candidate. These models invoke new heavy quarks…

astro-ph.CO2025

Axion Dark Matter Archaeology with Primordial Gravitational Waves

Andrew Cheek, Anish Ghoshal, Debarun Paul

We investigate the complementary information to be gained from inflationary gravitational wave (IGW) signals and searches for QCD axion dark matter. We focus on post-inflationary P…

hep-ph2025

Testing the dark origin of neutrino masses with oscillation experiments

Andrew Cheek, Luca Visinelli, Hong-Yi Zhang

The origin of neutrino masses remains unknown to date. One popular idea involves interactions between neutrinos and ultralight dark matter, described as fields or particles with ma…

hep-ph2023

A Direct Detection View of the Neutrino NSI Landscape

Dorian W. P. Amaral, David Cerdeno, Andrew Cheek +1

In this article, we study the potential of direct detection experiments to explore the parameter space of general non-standard neutrino interactions (NSI) via solar neutrino scatte…

hep-ph2024

Gemini Dark Matter

Andrew Cheek, Yu-Cheng Qiu, Liang Tan

The tension in the large scale structure can be explained by decaying dark matter with an almost degenerate spectrum and small enough decay width. Here we propose the Ge…

hep-ph2023

Extending preferred axion models via heavy-quark induced early matter domination

Andrew Cheek, Jacek K. Osiński, Leszek Roszkowski

We examine the cosmological consequences of the heavy quarks in KSVZ-type axion models. We find that their presence often causes an early matter domination phase, altering the evol…

hep-ph2023

Dark matter production through a non-thermal flavon portal

Andrew Cheek, Jacek K. Osiński, Leszek Roszkowski +1

The Froggatt-Nielsen (FN) mechanism provides an attractive way of generating the determined fermion mass hierarchy and quark mixing matrix elements in the Standard Model (SM). Here…

hep-ph2026

Earth rotation turns event timing into a geometric probe of UHE neutrino origin

Andrew Cheek, João Paulo Pinheiro, Jordi Salvado

It has been proposed that the ultra-high-energy (UHE) event detected by KM3NeT could be explained by dark matter (DM) decay. Prima facie this seems unlikely becau…

astro-ph.CO2023

Redshift Effects in Particle Production from Kerr Primordial Black Holes

Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez +1

When rotating primordial black holes evaporate via Hawking radiation, their rotational energy and mass are dissipated with different dynamics. We investigate the effect of these dy…

hep-ph2023

Isospin-violating dark matter at liquid noble detectors: new constraints, future projections, and an exploration of target complementarity

Andrew Cheek, Darren D. Price, Ellen M. Sandford

There is no known reason that dark matter interactions with the Standard Model should couple to neutrons and protons in the same way. This isospin violation can have large conseque…

hep-ph2026

: Solar Neutrinos for Direct Detection

Dorian W. P. Amaral, David Cerdeño, Andrew Cheek +2

We introduce Solar Neutrinos for Direct Detection (): an open-source Python package that enables the computation of the solar neutrino rate spectrum at direct detec…

hep-ph2022

Primordial Black Hole Evaporation and Dark Matter Production: II. Interplay with the Freeze-In/Out Mechanism

Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez +1

We study how the evaporation of primordial black holes (PBHs) can affect the production of dark matter (DM) particles through thermal processes. We consider fermionic DM interactin…

astro-ph.GA2020

The dark matter component of the Gaia radially anisotropic substructure

Nassim Bozorgnia, Azadeh Fattahi, Carlos S. Frenk +5

We study the properties of the dark matter component of the radially anisotropic stellar population recently identified in the Gaia data, using magneto-hydrodynamical simulations o…

hep-ph2026

Probing Dark Matter annihilation in the Galactic Centre with TRIDENT

Yingwei Wang, Xinhui Chu, Andrew Cheek +7

We determine the future sensitivity of the TRIDENT neutrino telescope to dark matter annihilation in the Galactic Centre. By applying the full detector design we show that TRIDENT…

hep-ph2026

Quality control for axions and ALPs

Andrew Cheek, Andrew Fowlie, Gonzalo Herrera

Axions and axion-like particles (ALPs) are protected by Peccei-Quinn (PQ) symmetries that quantum gravity is expected to break. Modeling quantum gravity by Planck-suppressed PQ-bre…

hep-ph2023

Primordial Black Holes Are True Vacuum Nurseries

Louis Hamaide, Lucien Heurtier, Shi-Qian Hu +1

The Hawking evaporation of primordial black holes (PBH) reheats the Universe locally, forming hot spots that survive throughout their lifetime. We propose to use the temperature pr…

hep-ph2023

Evaporation of Primordial Black Holes in the Early Universe: Mass and Spin Distributions

Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez +1

Many cosmological phenomena lead to the production of primordial black holes in the early Universe. These phenomena often create a population of black holes with extended mass and…

hep-ph2021

Light and Darkness: consistently coupling dark matter to photons via effective operators

Chiara Arina, Andrew Cheek, Ken Mimasu +1

We revise the treatment of fermionic dark matter interacting with photons via dimension-5 and -6 effective operators. We show how the application of the effective operators beyond…

hep-ph2025

Sub-GeV Dark Matter Under Pressure from Direct Detection

Andrew Cheek, Pablo Figueroa, Gonzalo Herrera +1

The DAMIC-M collaboration recently reported impressive bounds on sub-GeV dark matter, robustly testing both thermal and non-thermal models for the very first time. In this work we…

hep-ph2025

Dark photon dark matter from flattened axion potentials

Hong-Yi Zhang, Paola Arias, Andrew Cheek +3

Dark photons can be resonantly produced in the early universe via their coupling to an oscillating axion field. However, this mechanism typically requires large axion--dark photon…

hep-ph2022

Primordial Black Hole Evaporation and Dark Matter Production: I. Solely Hawking radiation

Andrew Cheek, Lucien Heurtier, Yuber F. Perez-Gonzalez +1

Hawking evaporation of black holes in the early Universe is expected to copiously produce all kinds of particles, regardless of their charges under the Standard Model gauge group.…

hep-ph2018

Opening the energy window on direct dark matter detection

Nassim Bozorgnia, David G. Cerdeno, Andrew Cheek +1

In this article we investigate the benefits of increasing the maximum nuclear recoil energy analysed in dark matter (DM) direct detection experiments. We focus on elastic DM-nucleu…