activity
19952025
most citedObservation of a New Narrow Charmonium State in Exclusive B+-->K+ pi+pi- J/psi Decays

2k citations · 20.9k across the 251 of their papers we have counts for

collaborators

248 papers

physics.ins-det2025

Quantum measurement systems and applications to particle physics and cosmology

Masashi Hazumi

There are new detector proposals and R&D that utilize quantum enhancements not previously adopted. Examples include superconducting quantum sensors, atom interferometry, and quantu…

astro-ph.IM2024

The Simons Observatory: Design, Integration, and Current Status of Small Aperture Telescopes

Aashrita Mangu, Lance Corbett, Sanah Bhimani +14

The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment located in the Atacama Desert in Chile at an elevation of 5200 meters, nominally consisting of…

astro-ph.IM2024

Commissioning the CMB polarization telescope GroundBIRD with the full set of detectors

Miku Tsujii, Jochem J. A. Baselmans, Jihoon Choi +39

GroundBIRD is a ground-based cosmic microwave background (CMB) experiment for observing the polarization pattern imprinted on large angular scales ( ) from the Teide Obse…

hep-ph2024★ 9 cited

Nuclear Spin Metrology with Nitrogen Vacancy Center in Diamond for Axion Dark Matter Detection

So Chigusa, Masashi Hazumi, Ernst David Herbschleb +3

We present a method to directly detect the axion dark matter using nitrogen vacancy centers in diamonds. In particular, we use metrology leveraging the nuclear spin of nitrogen to…

astro-ph.IM2024

The LiteBIRD mission to explore cosmic inflation

T. Ghigna, A. Adler, K. Aizawa +156

LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primord…

astro-ph.IM2024★ 1 cited

Development of the Low Frequency Telescope focal plane detector arrays for LiteBIRD

Tommaso Ghigna, Aritoki Suzuki, Benjamin Westbrook +12

LiteBIRD, a forthcoming JAXA mission, aims to accurately study the microwave sky within the 40-400 GHz frequency range divided into 15 distinct nominal bands. The primary objective…