activity
20042026
most citedExperimental Searches for the Axion and Axion-like Particles

690 citations · 10.7k across the 91 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

hep-ph2020★ 55 cited

Dark Energy Radiation

Kim V. Berghaus, Peter W. Graham, David E. Kaplan +2

We show that if dark energy evolves in time, its dynamical component could be dominated by a bath of dark radiation. Within current constraints this radiation could have up to $\si…

gr-qc2020★ 28 cited

Gravity Gradient Noise from Asteroids

Michael A. Fedderke, Peter W. Graham, Surjeet Rajendran

The gravitational coupling of nearby massive bodies to test masses in a gravitational wave (GW) detector cannot be shielded, and gives rise to 'gravity gradient noise' (GGN) in the…

gr-qc2020★ 38 cited

Gravity Probe Spin: Prospects for measuring general-relativistic precession of intrinsic spin using a ferromagnetic gyroscope

Pavel Fadeev, Tao Wang, Y. B. Band +4

An experimental test at the intersection of quantum physics and general relativity is proposed: measurement of relativistic frame dragging and geodetic precession using intrinsic s…

hep-ph2020★ 78 cited

Exploring the robustness of stellar cooling constraints on light particles

William DeRocco, Peter W. Graham, Surjeet Rajendran

Stellar cooling arguments place strict restrictions on a wide variety of models of new physics. In this paper, we argue that mechanisms to evade these constraints are restricted by…

hep-ph2020★ 61 cited

Storage Ring Probes of Dark Matter and Dark Energy

Peter W. Graham, Selcuk Haciomeroglu, David E. Kaplan +3

We show that proton storage ring experiments designed to search for proton electric dipole moments can also be used to look for the nearly dc spin precession induced by dark energy…

hep-ph2020★ 124 cited

Muons in supernovae: implications for the axion-muon coupling

Robert Bollig, William DeRocco, Peter W. Graham +1

The high temperature and electron degeneracy attained during a supernova allow for the formation of a large muon abundance within the core of the resulting proto-neutron star. If n…