LZ reports no WIMP detection in 60 live days with 5.5 t exposure and sets a new spin-independent limit of 9.2×10^{-48} cm² at 36 GeV/c².
collaboratiom, Physical Review Letters 131(4) (2023)
7 Pith papers cite this work. Polarity classification is still indexing.
7
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
roles
background 2representative citing papers
A nonlocal gravity model interpolates between MOND in bound systems and dark matter-like effects in cosmology.
Dark matter capture heats Planet 9 to ~200 K for certain interaction strengths, providing an infrared observational signature.
JWST TRGB distances to 10 SN Ia hosts update calibrations for 11 SNe yielding H0 of 68.4-69.6 km/s/Mpc and show modest shifts when combined with prior HST data.
Semi-supervised DL anomaly detector (VAE + classifier) for model-independent searches in DARWIN, outperforming classical likelihood tests on simulated WIMP injections while learning directly from raw high-dimensional outputs.
Interstellar objects may contribute enough baryonic mass to reduce the local dark matter halo density to 0.24 GeV/cm³.
citing papers explorer
-
First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
LZ reports no WIMP detection in 60 live days with 5.5 t exposure and sets a new spin-independent limit of 9.2×10^{-48} cm² at 36 GeV/c².
-
A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems
A nonlocal gravity model interpolates between MOND in bound systems and dark matter-like effects in cosmology.
-
Dark matter heating of Planet 9, and its observational implications
Dark matter capture heats Planet 9 to ~200 K for certain interaction strengths, providing an infrared observational signature.
-
The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch
JWST TRGB distances to 10 SN Ia hosts update calibrations for 11 SNe yielding H0 of 68.4-69.6 km/s/Mpc and show modest shifts when combined with prior HST data.
-
Model-independent searches of new physics in DARWIN with a semi-supervised deep learning pipeline
Semi-supervised DL anomaly detector (VAE + classifier) for model-independent searches in DARWIN, outperforming classical likelihood tests on simulated WIMP injections while learning directly from raw high-dimensional outputs.
-
Contribution of interstellar objects to local dark matter density
Interstellar objects may contribute enough baryonic mass to reduce the local dark matter halo density to 0.24 GeV/cm³.
- Search for Higgsinos in final states with low-momentum lepton-track pairs at 13 TeV