Galactic transient sources with the Cherenkov Telescope Array Observatory

Monthly Notices of the Royal Astronomical Society Oxford University Press 540:1 (2025) 205-238

Authors:

K Abe, S Abe, J Abhir, A Abhishek, F Acero, A Acharyya, R Adam, A Aguasca-Cabot, I Agudo, A Aguirre-Santaella, J Alfaro, R Alfaro, N Alvarez-Crespo, R Alves Batista, J-P Amans, E Amato, G Ambrosi, F Ambrosino, EO Angüner, LA Antonelli, C Aramo, C Arcaro, TTH Arnesen, K Asano

Abstract:

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exhibiting extreme variability as magnetars as well as pulsar-wind nebulae. Although most of them can show emission up to MeV and/or GeV energies, many have not yet been detected in the TeV domain by Imaging Atmospheric Cherenkov Telescopes. In this paper, we explore the feasibility of detecting new Galactic transients with the Cherenkov Telescope Array Observatory (CTAO) and the prospects for studying them with Target of Opportunity observations. We show that CTAO will likely detect new sources in the TeV regime, such as the massive microquasars in the Cygnus region, low-mass X-ray binaries with low-viewing angle, flaring emission from the Crab pulsar-wind nebula or other novae explosions, among others. Since some of these sources could also exhibit emission at larger time-scales, we additionally test their detectability at longer exposures. We finally discuss the multiwavelength synergies with other instruments and large astronomical facilities.

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.