747 citations · 2k across the 16 of their papers we have counts for
16 papers
Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX
ADMX Collaboration, G. Carosi, C. Cisneros +50
Axion dark matter can satisfy the conditions needed to account for all of the dark matter and solve the strong CP problem. The Axion Dark Matter eXperiment (ADMX) is a direct dark…
Improved Receiver Noise Calibration for ADMX Axion Search: 4.54 to 5.41 eV
M. Guzzetti, D. Zhang, C. Goodman +48
Axions are a well-motivated candidate for dark matter. The preeminent method to search for axion dark matter is known as the axion haloscope, which makes use of the conversion of a…
Search for non-virialized axions with 3.3-4.2 eV mass at selected resolving powers
A. T. Hipp, A. Quiskamp, T. J. Caligiure +65
The Axion Dark Matter eXperiment is sensitive to narrow axion flows, given axions compose a fraction of the dark matter with a non-negligible local density. Detecting these low-vel…
Axion Dark Matter eXperiment around 3.3 μeV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability
C. Goodman, M. Guzzetti, C. Hanretty +46
We report the results of a QCD axion dark matter search with discovery ability for Dine Fischler Srednicki Zhitnitsky (DFSZ) axions using an axion haloscope. Sub-Kelvin noise tempe…
The Data Acquisition System of the LZ Dark Matter Detector: FADR
J. Aalbers, D. S. Akerib, A. K. Al Musalhi +213
The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MH…
Axion Dark Matter eXperiment: Run 1A Analysis Details
C. Boutan, B. H. LaRoque, E. Lentz +48
The ADMX collaboration gathered data for its Run 1A axion dark matter search from January to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-…
Non-Virialized Axion Search Sensitive to Doppler Effects in the Milky Way Halo
C. Bartram, T. Braine, R. Cervantes +53
The Axion Dark Matter eXperiment (ADMX) has previously excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions between 680-790 MHz under the assumption that the dark matter is des…
Low Frequency (100-600 MHz) Searches with Axion Cavity Haloscopes
S. Chakrabarty, J. R. Gleason, Y. Han +44
We investigate reentrant and dielectric loaded cavities for the purpose of extending the range of axion cavity haloscopes to lower masses, below the range where the Axion Dark Matt…
Search for a dark-matter induced Cosmic Axion Background with ADMX
ADMX Collaboration, T. Nitta, T. Braine +45
We report the first result of a direct search for a Cosmic Background (CB) - a relativistic background of axions that is not dark matter - performed with the axion…
First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment
J. Aalbers, D. S. Akerib, C. W. Akerlof +344
The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dak…
Dark Matter Axion Search Using a Josephson Traveling Wave Parametric Amplifier
C. Bartram, T. Braine, R. Cervantes +48
We present a new exclusion bound of axion-like particle dark matter with axion-photon couplings above over the frequency range 4796.7--4799.…
Search for "Invisible" Axion Dark Matter in the eV Mass Range
ADMX Collaboration, C. Bartram, T. Braine +49
We report the results from a haloscope search for axion dark matter in the eV mass range. This search excludes the axion-photon coupling predicted by one of the b…
Axion Dark Matter eXperiment: Run 1B Analysis Details
ADMX Collaboration, C. Bartram, T. Braine +45
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 eV, corresponding to the frequency range 680--…
Extended Search for the Invisible Axion with the Axion Dark Matter Experiment
T. Braine, R. Cervantes, N. Crisosto +39
This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range - . This search excludes the full range of axion-phot…
Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment
D. S. Akerib, C. W. Akerlof, S. K. Alsum +175
LUX-ZEPLIN (LZ) is a next generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, So…
Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches
D. S. Akerib, C. W. Akerlof, D. Yu. Akimov +202
The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. Th…