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Chiara Capelli (University of Zurich)03/11/2025 11:30
The QROCODILE (Quantum Resolution-Optimized Cryogenic Observatory for Dark matter Incident at Low Energy) experiment uses superconducting nanowire single-photon detectors (SNSPDs) to search for scattering and absorption of dark matter (DM) candidates with masses as low as 30 keV. We conducted a first measurement at the University of Zurich with a WSi SNSPD placed on a Si/SiO2 substrate, and we...
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Robert Smith03/11/2025 12:00
The QUEST-DMC experiment uses a superfluid helium-3 target, cooled to less than 200 microkelvin, to search for interactions with sub-GeV mass dark matter candidates with recoil energies in the keV scale and below. Nanoelectromechanical resonators (NEMS) are submerged in the superfluid target and read out using low-noise quantum sensors to achieve the low energy thresholds required to probe...
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Silvia Scorza03/11/2025 14:30
The Modane Underground Laboratory is the deepest tunnel-access underground laboratory in Europe. The experimental site is protected by a 4800 m.w.e. overburden that reduce the muon flux to 5 muons/m2/day, and is thus ideal for a wide range of applications requiring ultra-low radioactivity levels. I will present the evolution of this facility and of its science program in the domain of dark...
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Javier Tiffenberg04/11/2025 09:30
Over the past decade, Skipper Charge-Coupled Devices (Skipper-CCDs) have transformed the landscape of rare-event detection by enabling ionization measurements with sub-electron resolution and unprecedented low dark-counts. This capability has opened new windows into the search for low-mass dark matter, coherent neutrino scattering, exotic neutrino interactions, and milli-charged particles. In...
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Santiago Perez04/11/2025 10:00
Millicharged particles (mCPs) appear in many extensions of the standard model. They are characterized by having a fractional electric charge and can be a compelling DM candidate or part of a dark sector that could solve anomalies in both particle physics and cosmology. If mCPs exist, they could be created through meson decays in accelerator facilities. Taking advantage of the low ionization...
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Nicolás AVALOS (LPNHE - IN2P3 - CNRS)04/11/2025 10:30
DAMIC-M (DArk Matter in CCDs at Modane) is an ongoing dark matter (DM) direct detection experiment located at the Modane Underground Laboratory (LSM). The very low energy threshold of Skipper CCDs allows us to test unexplored regions of the DM parameter space, in particular MeV-scale particles which interact with electrons via a U(1) mediator. Using a prototype detector and an exposure of ~1.2...
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04/11/2025 11:00
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Julien BILLARD (CNRS - IP2I)04/11/2025 11:45
TESSERACT (Transition Edge Sensor with Sub-Ev Resolution and Cryogenic Targets) is a future Light Dark Matter experiment to be installed in the Laboratoire Souterrain de Modane. Several cryogenic targets will be used in order to be sensitive to different DM interactions, allowing to explore both Electronic Recoils Dark Matter (ERDM) and Nuclear Recoils Dark Matter (NRDM) in the sub-GeV range,...
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Matthew Stukel (SNOLAB)04/11/2025 12:15
Located 2km underground at SNOLAB, the SuperCDMS (Cryogenic
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Dark Matter Search) experiment will focus on the detection of low-mass
(<10 GeV/c2) dark matter particles. The experiment utilizes 6 silicon and
18 germanium cryogenic calorimeters arranged in 4 detector towers.
There are two types of individual detectors; HV and iZIP. The HV detectors
are instrumented with phonon sensors, and... -
Paolo Gorla04/11/2025 12:45
The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) experiment, located in Laboratori Nazionali del Gran Sasso - INFN in Italy, aims to directly detect light dark matter (DM) particles. Scintillating CaWO_4 crystals, equipped with Transition Edge Sensor (TES), are operated as cryogenic detectors at mK temperatures, as target material for DM-nucleus scattering. CRESST...
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Jelle Aalbers05/11/2025 09:30
Liquid xenon detectors currently provide the most sensitive constraints on a broad range of dark matter candidates. Thanks to progress in detector technology and analysis methods, including ionization-only searches and the Migdal effect, xenon detectors are also effective at constraining several light dark matter models. This talk will overview the status, future prospects and limitations of...
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Davide Franco05/11/2025 10:00
Liquid argon (LAr) technology has emerged as one of the most widely used detection media in astroparticle physics, offering exceptional scalability and outstanding scintillation and ionization yields. Its versatility enables a broad scientific program ranging from neutrino physics and dark matter searches to future applications in MeV gamma astronomy. The intrinsic purity, self-shielding...
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Marie-Cecile Piro05/11/2025 10:30
The New Experiments With Sphere-Gas (NEWS-G) uses spherical proportional counters filled with light noble gas to directly detect light dark matter particles. The detector consists of a large sphere of 135 cm diameter, equipped with a high-voltage multi-anode sensor, “ACHINOS”, developed to ensure a sufficiently strong electric field at large radii while maintaining the capacity to achieve high...
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Shaobo Wang05/11/2025 11:30
Large scale liquid xenon (LXe) detectors located deep underground have unique
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advantages in searching for rare physics signals, including dark matter (DM) and
neutrinos. PandaX-4T is one of the big three LXe experiments for DM searches. We are
running the PandaX-4T detector with 4-ton xenon in the sensitive volume, the
commissioning run0 data and physical run 1 data have push the... -
Knut Moraa05/11/2025 12:00
Searches for dark matter below 1 GeV using solid detectors face challenging backgrounds associated with minuscule strains and stresses in the detector target and mounting. Alongside low mass and high radiopurity this makes superfluid 4He a unique target material. The TESSERACT multi-target dark matter search has demonstrated a superfluid He detector prototype which is sensitive to both...
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Laurent Chevalier06/11/2025 09:30
The DAWA (Dark Matter Axion Wideband Approach) experiment aims to detect
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axion-photon conversions in the 10–40 GHz frequency range, with sensitivity
to axion-photon couplings on the order of 10⁻¹¹ [GeV⁻¹].
The experimental setup consists of a spherical metallic surface magnetized
by permanent magnets, generating an average magnetic field of
approximately 0.8 T, over an area of about 1... -
Esther Ferrer Ribas (IRFU - Université Paris-Saclay)06/11/2025 10:00
The International Axion Observatory (IAXO) and its prototype, BabyIAXO, are next-generation helioscopes designed to search for axions and axion-like particles (ALPs) with unprecedented sensitivity. A key element of the project is the detector development program, which aims to achieve ultra-low background levels and high X-ray detection efficiency. BabyIAXO serves as a technological pathfinder...
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Gabe Hoshino06/11/2025 10:30
BREAD is a reflector-based axion detection concept which seeks to perform broadband searches for axions and axion-like particles at frequencies which are not accessible to resonant cavity experiments due to scaling limitations at small wavelengths. We present recent results from GigaBREAD, a gigahertz pilot experiment which probed axion-like particles and dark photons in the $\sim 50 ...
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David Leppla-Weber06/11/2025 11:30
The nature of dark matter is one of the biggest open questions in physics today.
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One possible answer is the axion, which was originally predicted as a solution
to the strong CP problem but also makes for an excellent cold dark matter can-
didate. The MAgnetized Disk and Mirror Axion eXperiment (MADMAX) aims
at detecting axions from the galactic dark matter halo in the theoretically... -
Ed Daw06/11/2025 12:00
The Axion Dark Matter eXperiment, sited at The University of Washington, Seattle, utilises a Sikivie type electromagnetic resonator to search for QCD axion dark matter. Joined in the last couple of years by the CAPP collaboration, ADMX continues to search for local halo axions at levels commensurate with the DFSZ model in a mass range 2.9 to 5.4 micro electron volts. QSHS is a new...
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Andreas Ringwald07/11/2025 09:30
The nature of dark matter remains one of the central puzzles in physics. Beyond traditional WIMPs, weakly interacting slim particles (WISPs) — such as axions, axion-like particles, dilatons, dark photons, and dark gravitons — emerge naturally in theories beyond the Standard Model, including string theory and modified gravity. Their ultra-light masses make them compelling wave-like dark matter...
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Prof. Yann Mambrini (CNRS, IJCLab, Université Paris-Saclay)07/11/2025 10:00
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Marco Cirelli07/11/2025 10:30
Light DM, intended as having a mass between 1 MeV and about 1 GeV, is an intriguing possibe alternative to the more traditional WIMP Dark Matter. It is interesting both theoretically and phenomenologically. Testing it via Indirect Detection is more challenging than WIMPs, but X-ray measurements provide a very powerful handle. They currently impose stringent constraints, and allow in...
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07/11/2025 11:30
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Sebastian A. R. Ellis, Valerie Domcke10/11/2025 15:00
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Lucien Heurtier12/11/2025 08:30
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Marcos Garcia12/11/2025 08:50
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Nabeen Bhusal12/11/2025 09:10
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Simon Cléry12/11/2025 09:30
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Mathieu Gross12/11/2025 10:20
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Jong-Hyun Yoon12/11/2025 10:40
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Riajul Haque12/11/2025 11:00
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Wenqi Ke12/11/2025 11:20
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Oleg Lebedev12/11/2025 13:30
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Stephen Henrich12/11/2025 13:50
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Sreemanti Chakraborti12/11/2025 14:10
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Hyun Min Lee12/11/2025 15:00
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Debaprasad Maity12/11/2025 15:20
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Alejandro Ibarra12/11/2025 15:40
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Kunio Kaneta12/11/2025 16:30
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Hyungjin Kim12/11/2025 16:50
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Tony Gherghetta13/11/2025 10:00
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Luca Scotto13/11/2025 14:30
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17/11/2025 11:00
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Panni Margot17/11/2025 13:30
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Reshmi Mukherjee (Barnard College, Columbia University)17/11/2025 14:00
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Julie McEnery17/11/2025 15:00
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MATTEO CERRUTI (Université de Paris / APC)17/11/2025 16:30
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Jeff Scargle17/11/2025 17:00
How would you like an algorithm that
Takes in time series you suspect, or know, contain periodic signals
Handles any data mode — time-tagged photons, fluxes, etc.
Returns estimates , for any sinusoidal signals present, of their
Amplitude
Phase
Frequency
Separates sinusoid pairs even closer in frequency than the Rayleigh criterion (Super Resolution)These properties of a new...
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Floriane Cangemi17/11/2025 17:30
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Werner Hofmann18/11/2025 09:00
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Sophie Aerdker18/11/2025 10:00
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Greg Madejski18/11/2025 11:00
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Andrii Neronov18/11/2025 12:00
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Jürgen Knödlseder (IRAP)18/11/2025 14:00
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Régis TERRIER (APC (CNRS/Université Paris Cité))18/11/2025 15:00
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Martin LEMOINE (Institut d'Astrophysique de Paris)19/11/2025 09:00
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Marianne LEMOINE-GOUMARD (CENBG, Univ. Bordeaux, CNRS-IN2P3)19/11/2025 10:00
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Guillaume DUBUS (IPAG)19/11/2025 11:00
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François Brun (CEA Saclay (IRFU/DPHP))19/11/2025 12:00
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Frédéric DAIGNE (Institut d'Astrophysique de Paris - Sorbonne University)19/11/2025 15:00
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Anna Franckowiak19/11/2025 16:30
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David Smith19/11/2025 17:30
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Helene Sol19/11/2025 18:00
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Pablo Saz Parkinson20/11/2025 09:00
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Foteini Oikonomou (Norwegian University of Science and Technology (NTNU))20/11/2025 10:00
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Sera Markoff20/11/2025 11:00
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Phil Uttley20/11/2025 12:00
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Janneth Valverde20/11/2025 15:30
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Fabian Schüssler (IRFU / CEA Paris-Saclay)20/11/2025 16:00
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Jean-François Glicenstein (IRFU, CEA Saclay)20/11/2025 16:30
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David Sanchez (LAPP/IN2P3/CNRS)21/11/2025 10:00
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Julien Peloton (CNRS-IJCLab)21/11/2025 11:00
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Deirdre HORAN (LLR / Ecole Polytechnique / CNRS / IN2P3), Jonathan Biteau (Université Paris-Saclay, CNRS/IN2P3, IJCLab), Stephen FEGAN (LLR/Ecole Polytechnique)21/11/2025 11:30
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Lucien Heurtier
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