We use our recent electric dipole moment (EDM) measurement data to constrain the possibility that the HfF+ EDM oscillates in time due to interactions with candidate dark matter axionlike particles (ALPs). We employ a Bayesian analysis method which accounts for both the look-elsewhere effect and the uncertainties associated with stochastic density fluctuations in the ALP field. We find no evidence of an oscillating EDM over a range spanning from 27 nHz to 400 mHz, and we use this result to constrain the ALP-gluon coupling over the mass range 10-22-10-15 eV. This is the first laboratory constraint on the ALP-gluon coupling in the 10-17-10-15 eV range, and the first laboratory constraint to properly account for the stochastic nature of the ALP...
The amplitude of the pseudoscalar (axion) or scalar field fluctuates on a time scale of order of mil...
Abstract Adding an axion-like particle (ALP) to the Standard Mod...
Recently there has been a surge of new experimental proposals to search for ultralight axion dark ma...
We use our recent electric dipole moment (EDM) measurement data to constrain the possibility that th...
Axion-like particles (ALPs) could mix with photons in the presence of astrophysical magnetic fields,...
In this work we revisit five different point sources within or behind galaxy clusters in order to co...
Several laboratory experiments have published limits on axionlike particles (ALPs) with feeble coupl...
Ultralight axion-like particles are well-motivated relics that might compose the cosmological dark m...
Ultralight axion-like particles can contribute to the dark matter near the Sun, leading to a distinc...
Ultralight axionlike particles (ALPs) are compelling dark matter candidates because of their potenti...
In the non-relativistic limit, two types of dark matter axion interactions with fermions are thought...
Axion-like particles (ALPs), which are gauge-singlets under the Standard Model (SM), appear in many ...
String theory compactifications may generate many light axion-like particles (ALPs) with weak coupli...
Despite the great successes achieved by the Standard Model (SM) in explaining and predicting the beh...
Searches for dark matter decaying into photons constrain its lifetime to be many orders of magnitude...
The amplitude of the pseudoscalar (axion) or scalar field fluctuates on a time scale of order of mil...
Abstract Adding an axion-like particle (ALP) to the Standard Mod...
Recently there has been a surge of new experimental proposals to search for ultralight axion dark ma...
We use our recent electric dipole moment (EDM) measurement data to constrain the possibility that th...
Axion-like particles (ALPs) could mix with photons in the presence of astrophysical magnetic fields,...
In this work we revisit five different point sources within or behind galaxy clusters in order to co...
Several laboratory experiments have published limits on axionlike particles (ALPs) with feeble coupl...
Ultralight axion-like particles are well-motivated relics that might compose the cosmological dark m...
Ultralight axion-like particles can contribute to the dark matter near the Sun, leading to a distinc...
Ultralight axionlike particles (ALPs) are compelling dark matter candidates because of their potenti...
In the non-relativistic limit, two types of dark matter axion interactions with fermions are thought...
Axion-like particles (ALPs), which are gauge-singlets under the Standard Model (SM), appear in many ...
String theory compactifications may generate many light axion-like particles (ALPs) with weak coupli...
Despite the great successes achieved by the Standard Model (SM) in explaining and predicting the beh...
Searches for dark matter decaying into photons constrain its lifetime to be many orders of magnitude...
The amplitude of the pseudoscalar (axion) or scalar field fluctuates on a time scale of order of mil...
Abstract Adding an axion-like particle (ALP) to the Standard Mod...
Recently there has been a surge of new experimental proposals to search for ultralight axion dark ma...