activity
20172025
most citedDetermining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8

144 citations · 152 across the 7 of their papers we have counts for

collaborators

7 papers

physics.ins-det2025

The real-time data processing and acquisition system for Project 8 Phase II

A. Ashtari Esfahani, A. Banducci, S. Böser +36

In Phase II of the Project 8 neutrino mass experiment, electrons from the decays of tritium or Kr are detected via their 26 GHz cyclotron radiation whil…

physics.ins-det2025

Project 8 Apparatus for Cyclotron Radiation Emission Spectroscopy with Kr and Tritium

A. Ashtari Esfahani, D. M. Asner, S. Böser +53

Cyclotron Radiation Emission Spectroscopy (CRES) is a novel technique for the precise measurement of relativistic electron energy. This technique is being employed by the Project~8…

astro-ph.CO2024

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…

physics.ins-det2024★ 3 cited

Deep Learning Based Event Reconstruction for Cyclotron Radiation Emission Spectroscopy

A. Ashtari Esfahani, S. Böser, N. Buzinsky +48

The objective of the Cyclotron Radiation Emission Spectroscopy (CRES) technology is to build precise particle energy spectra. This is achieved by identifying the start frequencies…

hep-ex2023

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-…

astro-ph.CO2023★ 5 cited

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…

physics.ins-det2017★ 144 cited

Determining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8

Ali Ashtari Esfahani, David M. Asner, Sebastian Böser +41

The most sensitive direct method to establish the absolute neutrino mass is observation of the endpoint of the tritium beta-decay spectrum. Cyclotron Radiation Emission Spectroscop…