COSMICWISPers - (other cosmicwispers conferences)
5-14 September, 2023
Bari and Lecce, Italy
published April 23, 2024
Bari and Lecce, Italy
published April 23, 2024
COSMIC WISPers is a COST Action CA21106 (https://www.cost.eu/actions/CA21106/) focusses on very weakly interacting slim (m
The first General Meeting of the COSMIC WISPers Action [https://agenda.infn.it/event/34125/] took place in Bari (Italy) from 5th to 8th September 2023. The objective of the meeting was to review the status of the activities performed by the different Working Groups and to discuss the further directions of investigations. There were plenary sessions and 4 parallel sessions corresponding to the different Working Groups:
• WG1: Theory and Model Building
• WG2: Dark Matter and Cosmology
• WG3: Astrophysics
• WG4: Direct Searches
After the General Meeting, the COST Action CA21106 1st Training School was held in Lecce (Italy) (https://agenda.infn.it/event/34190/) from 11st to 14th September 2023. The goal was to start training a generation of young scientists in the interdisciplinary expertise on WISPs, ranging from theoretical and experimental approaches to multi-messenger astroparticle physics and cosmology.
There were four lectures on different topics corresponding to the Working Groups 1—4 and several students talks.
Editorial Board
Pierluca Carenza (pierluca.carenza@fysik.su.se)
Stockholm University, Sweden
Valentina Danieli (vdanieli@sissa.it)
SISSA - International School for Advanced Studies, Trieste, Italy
Raffaele Di Vora (divora@pd.infn.it)
INFN, Laboratori Nazionali di Legnaro, Italy
Alessandro Mirizzi (alessandro.mirizzi@ba.infn.it)
Bari University & INFN Bari, Italy
Daniele Montanino (daniele.montanino@le.infn.it)
Lecce University and INFN Lecce, Italy
Mario Reig (mario.reiglopez@physics.ox.ac.uk)
University of Oxford, United Kingdom
Alessio Rettaroli (alessio.rettaroli@lnf.infn.it)
INFN, Laboratori Nazionali di Frascati, Italy
Ville Vaskonen (ville.vaskonen@pd.infn.it)
Padova University and INFN Padova, Italy
| Sessions |
|---|
| Wg1 |
| Wg2 |
| Wg3 |
| Wg4 |
| Training School Lectures |
| Training School Talks |
| Wg1 |
|---|
|
Out of the dark: WISPs in String Theory and the Early Universe
|
|
Uncovering axion and BSM CP violations with EDMs
|
|
Prospects to scrutinise or smash SM*A*S*H
|
|
Axions and Festina Lente
|
|
Testing BSM Physics with Gravitational Waves
|
|
Low-scale leptogenesis with Dirac phase CP-violation
|
| Wg2 |
|
Axion Star Explosions and the Reionization History of the Universe
|
|
Probing ultralight and degenerate dark matter with galactic dynamics
|
|
Birefringence in CMB anisotropies due to cosmological pseudoscalar fields
|
|
Photon to axion conversion during BBN
|
|
Cosmological defects
|
|
Radiation from Axion Strings with Adaptive Mesh Refinement: Periodic and Burst Signals
|
| Wg3 |
|
The Growth and Evolution of Axion Clouds around Pulsars
|
|
ALPs, high-energy gamma-rays and magnetic fields
|
|
Formation of ultralight dark matter solar halos
|
|
Glowing Axion Stars at Radio Frequencies
|
| Wg4 |
|
CAST and more than CAST; A Dark Sector Probe for 20+ Years
|
|
Status of the VMB@CERN experiment
|
|
Axion-like particle searches at the LHC
|
|
Probing the Dark Sector with NA64 and POKER at CERN SPS
|
|
High energy resolution x-ray detectors for IAXO: advantages in pre- and post-discovery phases
|
| Training School Lectures |
|
Axion theory and model building
|
|
Cosmology of axion dark matter
|
|
Astrophysical Axion Bounds: The 2024 Edition
|
| Training School Talks |
|
In search of new particles with PADME
|
|
Axion Dark Matter Simulations with Adaptive Mesh Refinement
|
|
Using gravitational waves to detect axion miniclusters and axion stars
|
|
Axion field tomography: cosmic birefringence from the epochs of recombination and reionization
|
|
Supernova bounds on nucleonphilic ALPs
|
|
Constraining Ultra-Light Scalar Dark Matter with Pulsars
|
|
Massive Gravitons in Very Special Relativity: Theory and Observations
|
|
Simulations for direct dark matter searches using ALPS II's TES detection system
|
|
Plasmonic resonant detection of WIMP
|