output
19922026
most citedDirect Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

3k citations

Showing 2022 · hep-phShow all

7 papers · 2 filters

hep-ph2022★ 11 cited

Supermassive black hole seeds from sub-keV dark matter

Avi Friedlander, Sarah Schon, Aaron C. Vincent

Quasars observed at redshifts are powered by supermassive black holes which are too large to have grown from early stellar remnants without efficient super-Eddington…

hep-ph2022★ 18 cited

Dark Matter from Monogem

Christopher V. Cappiello, Neal P. Avis Kozar, Aaron C. Vincent

As a supernova shock expands into space, it may collide with dark matter particles, scattering them up to velocities more than an order of magnitude larger than typical dark matter…

hep-ph2022★ 13 cited

New Constraints on Macroscopic Dark Matter Using Radar Meteor Detectors

Pawan Dhakal, Steven Prohira, Christopher V. Cappiello +3

We show that dark-matter candidates with large masses and large nuclear interaction cross sections are detectable with terrestrial radar systems. We develop our results in close co…

hep-ph2022★ 5 cited

Diffuse X-Ray and Gamma-Ray Limits on Boson Stars that Interact with Nuclei

Javier F. Acevedo, Amit Bhoonah, Joseph Bramante

Light bosonic dark matter can form gravitationally bound states known as boson stars. In this work, we explore a new signature of these objects interacting with the interstellar me…

hep-ph2022★ 181 cited

The Present and Future Status of Heavy Neutral Leptons

Asli M. Abdullahi, Pablo Barham Alzas, Brian Batell +42

The existence of non-zero neutrino masses points to the likely existence of multiple SM neutral fermions. When such states are heavy enough that they cannot be produced in oscillat…

hep-ph2022★ 49 cited

Snowmass2021 Cosmic Frontier White Paper: Ultraheavy particle dark matter

Daniel Carney, Nirmal Raj, Yang Bai +25

We outline the unique opportunities and challenges in the search for "ultraheavy" dark matter candidates with masses between roughly and the Planck scale $m_{\rm pl}…