Bracketing the soliton-halo relation of ultralight dark matter

(2025)

Authors:

Kfir Blum, Marco Gorghetto, Edward Hardy, Luca Teodori

QSHS: An Axion Dark Matter Resonant Search Apparatus

(2025)

Authors:

A Alsulami, I Bailey, G Carosi, G Chapman, B Chakraborty, EJ Daw, N Du, S Durham, J Esmenda, J Gallop, T Gamble, T Godfrey, G Gregori, J Halliday, L Hao, E Hardy, EA Laird, P Leek, J March-Russell, PJ Meeson, CF Mostyn, Yu A Pashkin, SO Peatain, M Perry, M Piscitelli, M Reig, EJ Romans, S Sarkar, PJ Smith, A Sokolov, N Song, A Sundararajan, B-K Tan, SM West, S Withington

Instability in N=4 supersymmetric Yang-Mills theory at finite density

Physical Review D American Physical Society (APS) 111:8 (2025) 086030

Authors:

Liam Gladden, Victor Ivo, Pavel Kovtun, Andrei O Starinets

F -extremization determines certain large- N CFTs

Journal of High Energy Physics Springer 2025:4 (2025) 85

Authors:

Ludo Fraser-Taliente, John Wheater

Abstract:

We show that the conformal data of a range of large-N CFTs, the melonic CFTs, are specified by constrained extremization of the universal part of the sphere free energy F = − log ZSd, called F~. This family includes the generalized SYK models, the vector models (O(N), Gross-Neveu, etc.), and the tensor field theories. The known F and a-maximization procedures in SCFTs are therefore extended to these non-supersymmetric CFTs in continuous d. We establish our result using the two-particle irreducible (2PI) effective action, and, equivalently, by Feynman diagram resummation. The universal part of F~ interpolates in continuous dimension between the known C-functions, so we can interpret this result as an extremization of the number of IR degrees of freedom, in the spirit of the generalized c, F, a-theorems. The outcome is a complete classification of the melonic CFTs: they are the conformal mean field theories which extremize the universal part of the sphere free energy, subject to an IR marginality condition on the interaction Lagrangian.

Dark matter attenuation effects: sensitivity ceilings for spin-dependent and spin-independent interactions

Journal of Cosmology and Astroparticle Physics IOP Publishing 2025:4 (2025) 017

Authors:

N Darvishi, J Smirnov, S Autti, L Bloomfield, A Casey, N Eng, P Franchini, Rp Haley, Pj Heikkinen, A Jennings, A Kemp, E Leason, J March-Russell, A Mayer, Jocelyn Monroe, D Münstermann, Mt Noble, Jr Prance, X Rojas, T Salmon, J Saunders, R Smith, Md Thompson, A Thomson, A Ting, V Tsepelin, Sm West, L Whitehead, De Zmeev

Abstract:

Direct detection experiments aimed at uncovering the elusive nature of dark matter (DM) have made significant progress in probing ever lower cross-sections for DM-nucleon interactions. At the same time, an upper limit in the cross-section sensitivity region is present due to DM scattering in the Earth and atmosphere and as a result never reaching the detector. We investigate the impact of this effect for both spin-dependent and spin-independent interactions. In contrast to previous studies that assume a straight line path for DM scattering we employ a semi-analytic diffusion model that takes into account the impact of potentially large angle deviations prevalent for light DM masses. We find that for sufficiently low energy thresholds, this difference in modelling impacts the DM interaction cross-section sensitivity. This study evaluates the impact in the context of the QUEST-DMC experiment, which utilises surface-based detectors with superfluid Helium-3 bolometers to search for sub-GeV DM exploiting low energy threshold. At masses below 1 GeV/c^2 the deviation between the two frameworks becomes pronounced. The ceiling sensitivity limit for QUEST-DMC on spin-dependent DM-neutron cross-sections is ∼ 3 × 10^-24cm^2 using the diffusive framework and approximately doubles with the straight-line path DM scattering. Similarly, for spin-independent DM-nucleon cross-sections, the ceiling limit is ∼ 7.5 × 10^-27cm^2 under the diffusive framework and also increases about a factor of two with the straight-line path approximation, within the mass range of 0.025–5 GeV/c^2.