papers

Publications (14)

hep-ph2026

-Dwarfs: White Dwarfs probe Quadratically Coupled Scalars

Kai Bartnick, Konstantin Springmann, Stefan Stelzl +1

We study ultralight scalar fields with quadratic couplings to Standard-Model fermions and derive strong constraints from white-dwarf mass-radius data. Such couplings source scalar…

astro-ph.HE2026

New ultralight scalar particles and the mass-radius relation of white dwarfs -- the important role of Sirius B

Kai Bartnick, Detlev Koester, Rolf-Peter Kudritzki +3

We present the equation of state for two classes of new ultralight particles, a scalar field coupling to electrons and a light QCD axion field coupling to…

hep-ph2023

Heavy neutron stars from light scalars

Reuven Balkin, Javi Serra, Konstantin Springmann +2

We study how light scalar fields can change the stellar landscape by triggering a new phase of nuclear matter. Scalars coupled to nucleons can develop a non-trivial expectation val…

hep-ph2025

Momentum and Matter Matter for Axion Dark Matter Matters on Earth

Abhishek Banerjee, Itay M. Bloch, Quentin Bonnefoy +5

We investigate the implications of matter effects to searches for axion Dark Matter on Earth. The finite momentum of axion Dark Matter is crucial to elucidating the effects of Eart…

hep-ph2024

White dwarfs as a probe of exceptionally light QCD axions

Reuven Balkin, Javi Serra, Konstantin Springmann +2

We study the effects of exceptionally light QCD axions on the stellar configuration of white dwarfs. At finite baryon density, the non-derivative coupling of the axion to nucleons…

hep-ph2025

Natural Ultralight Dark Matter: The Quadratic Twin

Cédric Delaunay, Michael Geller, Zamir Heller-Algazi +2

Scalar ultralight dark matter (ULDM) is uniquely accessible to tabletop experiments such as clocks and interferometers, and its search has been the focus of a vast experimental eff…

hep-ph2021

The QCD Axion at Finite Density

Reuven Balkin, Javi Serra, Konstantin Springmann +1

We show how the properties of the QCD axion change in systems at finite baryonic density, such as neutron stars. At nuclear saturation densities, where corrections can be reliably…

hep-ph2026

The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles

Ariel Arza, Deniz Aybas, Shyam Balaji +124

Axions and other very weakly interacting slim particles (WISPs), with masses below 1 GeV, arise naturally in many extensions of the Standard Model of particle physics. In particula…

hep-ph2025

From Supernovae to Neutron Stars: A Systematic Approach to Axion Production at Finite Density

Konstantin Springmann, Michael Stadlbauer, Stefan Stelzl +1

We present a systematic study of QCD axion production in environments with finite baryon density and temperature, implying significant changes to axion phenomenology. Within heavy…

hep-ph2024

Constraining Light QCD Axions with Isolated Neutron Star Cooling

Antonio Gómez-Bañón, Kai Bartnick, Konstantin Springmann +1

The existence of light QCD axions, whose mass depends on an additional free parameter, can lead to a new ground state of matter, where the sourced axion field reduces the nucleon e…

hep-ph2025

On the sensitivity of nuclear clocks to new physics

Andrea Caputo, Doron Gazit, Hans-Werner Hammer +4

The recent demonstration of laser excitation of the eV isomeric state of Thorium-229 is a significant step towards a nuclear clock. The low excitation energy likely res…

hep-ph2021

Runaway Relaxion from Finite Density

Reuven Balkin, Javi Serra, Konstantin Springmann +2

Finite density effects can destabilize the metastable vacua in relaxion models. Focusing on stars as nucleation seeds, we derive the conditions that lead to the formation and runaw…

hep-ph2025

A Universal Bound on QCD Axions from Supernovae

Konstantin Springmann, Michael Stadlbauer, Stefan Stelzl +1

We identify a new production channel for QCD axions in supernova environments that contributes to axion emissivity for all models solving the strong CP problem. This channel arises…

hep-ph2021

Density Induced Vacuum Instability

Reuven Balkin, Javi Serra, Konstantin Springmann +2

We consider matter density effects in theories with a false ground state. Large and dense systems, such as stars, can destabilize a metastable minimum and allow for the formation o…