activity
20232025
most citedLow energy effective theories of composite dark matter with real representations

1 citations · 1 across the 2 of their papers we have counts for

collaborators

6 papers

hep-ph2025

Sub-GeV dark matter and multi-decay signatures from dark showers at beam-dump experiments

Elias Bernreuther, Nicoline Hemme, Felix Kahlhoefer +2

In models of strongly-interacting dark sectors, the production of dark quarks at accelerators can give rise to dark showers with multiple dark mesons in the final state. If some of…

hep-ph2025

Surveying the theory space of pion dark matter

Anja Alfano, Nick Evans, Suchita Kulkarni +1

We use a holographic model to survey the space of strongly coupled SU(Nc) gauge dynamics with QCD-like chiral symmetry breaking pattern for quarks in the fundamental representation…

hep-ph2025

NLO observables for QCD-like theories and application to pion dark matter

Helena Kolešová, Daniil Krichevskiy, Suchita Kulkarni

QCD-like theories are of interest in various areas of beyond-Standard-Model phenomenology, including composite Higgs models or pionic dark matter. The effective field theories prov…

hep-ph2025

Strongly Interacting Dark Matter admixed Neutron Stars

Yannick Dengler, Suchita Kulkarni, Axel Maas +1

Dark matter may accumulate in neutron stars given its gravitational interaction and abundance. We investigate the influence of strongly-interacting dark matter, described by a QCD-…

hep-ph20241 cited

Low energy effective theories of composite dark matter with real representations

Joachim Pomper, Suchita Kulkarni

We consider pseudo Nambu-Goldstone bosons arising from Dirac fermions transforming in real representations of a confining gauge group as dark matter candidates. We consider a speci…

hep-ph2023

Dark matter relic density in strongly interacting dark sectors with light vector mesons

Elias Bernreuther, Nicoline Hemme, Felix Kahlhoefer +1

Stable dark matter particles may arise as pseudo-Goldstone bosons from the confinement of dark quarks interacting via a non-Abelian gauge force. Their relic abundance is determined…