Search Publications
Pulsar-based map of galactic acceleration
Moran, Abigail; Mingarelli, Chiara M. F.; Van Tilburg, Ken +1 more
Binary pulsars can be used to probe Galactic potential gradients through calculating their line-of-sight accelerations. We present the first data release of direct line-of-sight acceleration measurements for 29 binary pulsars. We validate these data with a local acceleration model, and compare our results to those from earlier works. We find evide…
Constraining the stochastic gravitational wave background using the future lunar seismometers
Zhang, Fan; Chen, Xian; Shao, Lijing +3 more
Motivated by the old idea of using the Moon as a resonant gravitational wave (GW) detector, as well as the recent updates in modeling the lunar response to GWs, we reevaluate the feasibility of using a network of lunar seismometers to constrain the stochastic GW background (SGWB). In particular, using the updated model of the lunar response, we de…
Sensor noise in L I S A P a t h f i n d e r : Laser frequency noise and its coupling to the optical test mass readout
Mendes, L.; Russano, G.; Sanjuan, J. +84 more
The LISA Pathfinder (LPF) mission successfully demonstrated the feasibility of the technology needed for the future space borne gravitational wave observatory LISA. A key subsystem under study was the laser interferometer, which measured the changes in relative distance in between two test masses (TMs). It achieved a sensitivity of 32.0-1.7
Violation of the equivalence principle induced by oscillating rest mass and transition frequency, and its detection in atom interferometers
Wolf, Peter; Gué, Jordan; Hees, Aurélien
We present a theoretical investigation of the expected experimental signals produced by freely falling atoms with time oscillating mass and transition frequency. These oscillations could be produced in a variety of models, in particular, models of scalar dark matter nonuniversally coupled to the standard matter such as axionlike particles and dila…
Nano-Newton electrostatic force actuators for femto-Newton-sensitive measurements: System performance test in the LISA Pathfinder mission
Mendes, L.; Russano, G.; Nofrarias, M. +89 more
Electrostatic force actuation is a key component of the system of geodesic reference test masses (TM) for the LISA orbiting gravitational wave observatory and in particular for performance at low frequencies, below 1 mHz, where the observatory sensitivity is limited by stray force noise. The system needs to apply forces of order 10-9 N …
Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
Wang, Yue; Gong, Yungui; Wang, Zhongkai +1 more
Primordial black holes (PBHs) generated in the early Universe are considered as one of the candidates for dark matter. To produce PBHs with sufficient abundance, the primordial scalar power spectrum needs to be enhanced to the order of 0.01. Considering the third-order polynomial potential with polynomial attractors, we show that PBHs with a mass …
Constraints on the fuzzy dark matter mass window from high-redshift observables
Kovetz, Ely D.; Lazare, Hovav; Flitter, Jordan
We use a combination of high-redshift observables to extract the strongest constraints to date on the fraction of axion fuzzy dark matter (FDM) in the mass window
Probing a scale dependent gravitational slip with galaxy strong lensing systems
Mörtsell, Edvard; Guerrini, Sacha
Observations of galaxy-scale strong gravitational lensing systems enable unique tests of departures from general relativity at the kilo- to megaparsec scale. In this work, the gravitational slip parameter γPN, measuring the amplitude of a hypothetical fifth force, is constrained using 130 elliptical galaxy lens systems. We implement a l…
Detection of gravitational waves in circular particle accelerators II. Response analysis and parameter estimation using synthetic data
Brüggen, Marcus; Rao, Suvrat; Baumgarten, Julia +1 more
We simulate the response of a Storage Ring Gravitational Wave Observatory (SRGO) to astrophysical millihertz (mHz) gravitational waves (GWs), numerically obtaining its sensitivity curve and optimal choices for some controllable experiment parameters. We also generate synthetic noisy GW data and use Markov Chain Monte Carlo methods to perform param…
Tilt-to-length coupling in LISA Pathfinder: Long-term stability
Mendes, L.; Russano, G.; Sanjuan, J. +75 more
The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular time spans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by