622 citations · 1.9k across the 22 of their papers we have counts for
22 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…
First Axion-Like Particle Results from a Broadband Search for Wave-Like Dark Matter in the 44 to 52 eV Range with a Coaxial Dish Antenna
Gabe Hoshino, Stefan Knirck, Mohamed H. Awida +16
We present the results from the first axion-like particle search conducted using a dish antenna. The experiment was conducted at room temperature and sensitive to axion-like partic…
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…
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…
First Results from a Broadband Search for Dark Photon Dark Matter in the to eV range with a coaxial dish antenna
Stefan Knirck, Gabe Hoshino, Mohamed H. Awida +25
We present first results from a dark photon dark matter search in the mass range from 44 to 52 () using a room-temperature dish antenna setup ca…
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…
Broadband solenoidal haloscope for terahertz axion detection
Jesse Liu, Kristin Dona, Gabe Hoshino +18
We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program. This haloscope plans to search for bosonic dark matter across the…
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.…
Design and performance of a multi-terahertz Fourier transform spectrometer for axion dark matter experiments
Kristin Dona, Jesse Liu, Noah Kurinsky +4
Dedicated spectrometers for terahertz radiation with [0.3, 30] THz frequencies using traditional optomechanical interferometry are substantially less common than their infrared and…
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--…
Axion Dark Matter eXperiment: Detailed Design and Operations
R. Khatiwada, D. Bowring, A. S. Chou +48
Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in…
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…
Piezoelectrically Tuned Multimode Cavity Search for Axion Dark Matter
C. Boutan, M. Jones, B. H. LaRoque +31
The eV axion is a well-motivated extension to the standard model. The Axion Dark Matter eXperiment (ADMX) collaboration seeks to discover this particle by looking for the resona…
A Search for Invisible Axion Dark Matter with the Axion Dark Matter Experiment
N. Du, N. Force, R. Khatiwada +25
This Letter reports results from a haloscope search for dark matter axions with masses between 2.66 and 2.81 eV. The search excludes the range of axion-photon couplings predicte…
Quantum Sensing for High Energy Physics
Zeeshan Ahmed, Yuri Alexeev, Giorgio Apollinari +113
Report of the first workshop to identify approaches and techniques in the domain of quantum sensing that can be utilized by future High Energy Physics applications to further the s…
US Cosmic Visions: New Ideas in Dark Matter 2017: Community Report
Marco Battaglieri, Alberto Belloni, Aaron Chou +248
This white paper summarizes the workshop "U.S. Cosmic Visions: New Ideas in Dark Matter" held at University of Maryland on March 23-25, 2017.
Bubble Chambers for Experiments in Nuclear Astrophysics
B. DiGiovine, D. Henderson, R. J. Holt +7
A bubble chamber has been developed to be used as an active target system for low energy nuclear astrophysics experiments. Adopting ideas from dark matter detection with superheate…
First determination of an astrophysical cross section with a bubble chamber: the 15N(α,γ)19F reaction
C. Ugalde, B. DiGiovine, D. Henderson +7
We have devised a technique for measuring some of the most important nuclear reactions in stars which we expect to provide considerable improvement over previous experiments. Adapt…