ARC Centre of Excellence for Dark Matter Particle Physics
Aims and Vision Nodes and Partners Media and Communcation Outreach and Education Equity, Diversity and Inclusion Publications Jobs and Opportunities Contact Code of Conduct Videos Stawell Underground Physics Laboratory
Executive Committee Chief Investigators Partner Investigators Associate Investigators Postdoctoral Researchers Academic Staff Professional and Technical Staff Students Research Committee Advisory Board International Scientific Advisory Committee Women in STEM Meet the Researcher
Introduction Direct Detection Large Hadron Collider Precision Metrology Theory
Media Releases Events Centre News Annual Reports
The Centre Aims and Vision Nodes and Partners Media and Communcation Outreach and Education Equity, Diversity and Inclusion Publications Jobs and Opportunities Contact Code of Conduct Videos Stawell Underground Physics Laboratory People Executive Committee Chief Investigators Partner Investigators Associate Investigators Postdoctoral Researchers Academic Staff Professional and Technical Staff Students Research Committee Advisory Board International Scientific Advisory Committee Women in STEM Meet the Researcher Research themes Introduction Direct Detection Large Hadron Collider Precision Metrology Theory News Media Releases Events Centre News Annual Reports
ARC Centre of Excellence for Dark Matter Particle Physics
 

Publications

 
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Featured
Theory
Jul 31, 2025
Dark Matter in the Coma cluster
Theory
Jul 31, 2025
Theory
Jul 31, 2025
Theory
Jul 28, 2025
Tidal adaptive softening and artificial fragmentation in cosmological simulations
Theory
Jul 28, 2025
Theory
Jul 28, 2025
Jul 28, 2025
Euclid: IV. The NISP Calibration Unit
Jul 28, 2025
Jul 28, 2025
Theory
Jun 28, 2025
Ending the Hubble tension
Theory
Jun 28, 2025
Theory
Jun 28, 2025
Theory
Apr 30, 2025
Dark matter genesis
Theory
Apr 30, 2025
Theory
Apr 30, 2025
Apr 28, 2025
Euclid preparation: LXVI. Impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties: insights from hydrodynamic simulations
Apr 28, 2025
Apr 28, 2025
Apr 28, 2025
Euclid preparation: LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey
Apr 28, 2025
Apr 28, 2025
Apr 28, 2025
Euclid preparation
Apr 28, 2025
Apr 28, 2025
Mar 28, 2025
Euclid preparation: LXIX. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey
Mar 28, 2025
Mar 28, 2025
Direct Detection
Feb 28, 2025
The SABRE South Experiment at the Stawell Underground Physics
Direct Detection
Feb 28, 2025
Direct Detection
Feb 28, 2025
Theory
Feb 28, 2025
Euclid preparation: LX. The use of HST images as input for weak-lensing image simulations
Theory
Feb 28, 2025
Theory
Feb 28, 2025
Theory
Feb 28, 2025
Euclid: Detecting Solar System objects in Euclid images and classifying them using Kohonen self-organising maps
Theory
Feb 28, 2025
Theory
Feb 28, 2025
Feb 28, 2025
Euclid: V. The Flagship galaxy mock catalogue: A comprehensive simulation for the Euclid mission
Feb 28, 2025
Feb 28, 2025
Metrology
Feb 10, 2025
A cosmogenic 10Be anomaly during the late Miocene as independent time marker for marine archives
Metrology
Feb 10, 2025
Metrology
Feb 10, 2025
Theory
Jan 31, 2025
Constraints on the U ( 1 ) B - L model from global QCD analysis
Theory
Jan 31, 2025
Theory
Jan 31, 2025
Theory
Jan 28, 2025
The Hubble Constant
Theory
Jan 28, 2025
Theory
Jan 28, 2025
Theory
Dec 31, 2024
Is there a scalar or pseudoscalar at 95 GeV?
Theory
Dec 31, 2024
Theory
Dec 31, 2024
Direct Detection
Dec 31, 2024
Time-dependent Aharonov-Bohm effect for electromagnetic and gravitational scalar potentials
Direct Detection
Dec 31, 2024
Direct Detection
Dec 31, 2024
Direct Detection
Dec 25, 2024
Two-neutrino double electron capture of 124Xe in the first LUX-ZEPLIN exposure
Direct Detection
Dec 25, 2024
Direct Detection
Dec 25, 2024
Theory
Dec 24, 2024
Neutrino portals to MeV WIMPs with s-channel mediators
Theory
Dec 24, 2024
Theory
Dec 24, 2024
Direct Detection
Dec 6, 2024
Level attraction in a quasiclosed cavity: Antiresonance in magnonic devices
Direct Detection
Dec 6, 2024
Direct Detection
Dec 6, 2024
Theory
Nov 30, 2024
Challenges in the extraction of physics beyond the Standard Model from electron scattering
Theory
Nov 30, 2024
Theory
Nov 30, 2024
Metrology
Nov 30, 2024
Upconversion of phonon modes into microwave photons in a lithium niobate bulk acoustic wave resonator coupled to a microwave cavity
Metrology
Nov 30, 2024
Metrology
Nov 30, 2024
Metrology
Nov 6, 2024
9th Symposium on Frequency Standards and Metrology 16/10/2023 - 20/10/2023 Kingscliff, Australia
Metrology
Nov 6, 2024
Metrology
Nov 6, 2024
Theory, Direct Detection
Nov 4, 2024
Time evolution of the reheating equation of state and its impact on the inflationary tensor perturbation spectrum
Theory, Direct Detection
Nov 4, 2024
Theory, Direct Detection
Nov 4, 2024
Direct Detection
Oct 31, 2024
Optimising an array of Cherenkov telescopes in Australia for the detection of TeV gamma-ray transients
Direct Detection
Oct 31, 2024
Direct Detection
Oct 31, 2024
Direct Detection
Oct 31, 2024
Metalized 3-D Printed Plastic Resonator Demonstrating Superconductivity Below 4 K
Direct Detection
Oct 31, 2024
Direct Detection
Oct 31, 2024
Theory, Direct Detection
Oct 31, 2024
Prospects for Light Dark Matter Searches at Large-Volume Neutrino Detectors
Theory, Direct Detection
Oct 31, 2024
Theory, Direct Detection
Oct 31, 2024
Direct Detection, Metrology
Oct 26, 2024
Precision multi-mode microwave spectroscopy of paramagnetic and rare-earth ion spin defects in single crystal calcium tungstate
Direct Detection, Metrology
Oct 26, 2024
Direct Detection, Metrology
Oct 26, 2024
Theory
Oct 26, 2024
Using dust to constrain dark matter models
Theory
Oct 26, 2024
Theory
Oct 26, 2024
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The ARC Centre of Excellence for Dark Matter Particle Physics is funded by the Australian Research Council

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The ARC Centre of Excellence for Dark Matter Particle Physics acknowledges the Traditional Custodians of the lands and waters on which we work. We acknowledge and pay respects to the Elders and Traditional Owners of the land on which our Australian nodes stand. We pay our respects to their Elders, past, present, and emerging.

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The ARC Centre of Excellence for Dark Matter Particle Physics recognises the richness diversity brings and we pride ourselves on fostering and promoting a diverse and inclusive learning and working environment free from discrimination, harassment, vilification, or victimisation based on individual identity and experience.


 

​© 2024 The ARC Centre of Excellence for Dark Matter Particle Physics