Search Publications

Testing gravity on cosmic scales: A case study of Jordan-Brans-Dicke theory
DOI: 10.1103/PhysRevD.105.043522 Bibcode: 2022PhRvD.105d3522J

Joudaki, Shahab; Ferreira, Pedro G.; Lima, Nelson A. +1 more

We provide an end-to-end exploration of a distinct modified gravitational theory in Jordan-Brans-Dicke (JBD) gravity, from an analytical and numerical description of the background expansion and linear perturbations, to the nonlinear regime captured with a hybrid suite of N -body simulations, to the cosmological constraints from existing probes of…

2022 Physical Review D
eHST 41
Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations
DOI: 10.1103/PhysRevD.106.023030 Bibcode: 2022PhRvD.106b3030B

Calore, F.; Serpico, P. D.; Siegert, T. +2 more

We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes …

2022 Physical Review D
INTEGRAL 39
Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA
DOI: 10.1103/PhysRevD.105.042002 Bibcode: 2022PhRvD.105d2002B

Baghi, Quentin; Korsakova, Natalia; Slutsky, Jacob +3 more

The LISA Pathfinder (LPF) mission succeeded outstandingly in demonstrating key technological aspects of future space-borne gravitational-wave detectors, such as the Laser Interferometer Space Antenna (LISA). Specifically, LPF demonstrated with unprecedented sensitivity the measurement of the relative acceleration of two free-falling cubic test mas…

2022 Physical Review D
LISAPathfinder 33
Galaxy luminosity function pipeline for cosmology and astrophysics
DOI: 10.1103/PhysRevD.105.043518 Bibcode: 2022PhRvD.105d3518S

Muñoz, Julian B.; Sabti, Nashwan; Blas, Diego

Observations of high-redshift galaxies have provided us with a rich tool to study the physics at play during the epoch of reionization. The luminosity function (LF) of these objects is an indirect tracer of the complex processes that govern galaxy formation, including those of the first dark-matter structures. In this work, we present an extensive…

2022 Physical Review D
eHST 31
Constraining the stochastic gravitational wave background with photometric surveys
DOI: 10.1103/PhysRevD.106.084006 Bibcode: 2022PhRvD.106h4006W

Doré, Olivier; Wang, Yijun; Pardo, Kris +1 more

The detection of the stochastic gravitational wave background (SGWB) is essential for understanding black hole populations, especially for supermassive black hole binaries. The recent promising results from various pulsar timing array (PTA) collaborations allude to an imminent detection. In this paper, we investigate the relative astrometric gravi…

2022 Physical Review D
Gaia 29
Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmography?
DOI: 10.1103/PhysRevD.106.123523 Bibcode: 2022PhRvD.106l3523P

Pourojaghi, S.; Zabihi, N. F.; Malekjani, M.

Using mock data for the Hubble diagrams of type Ia supernovae (SNIa) and quasars (QSOs) generated based on the standard model of cosmology, and using the least-squares method based on the Markov-Chain-Monte-Carlo (MCMC) algorithm, we first put constraints on the cosmographic parameters in the context of the various model-independent cosmographic m…

2022 Physical Review D
eHST 23
Transient acceleration events in LISA Pathfinder data: Properties and possible physical origin
DOI: 10.1103/PhysRevD.106.062001 Bibcode: 2022PhRvD.106f2001A

Mendes, L.; Russano, G.; Nofrarias, M. +79 more

We present an in depth analysis of the transient events, or glitches, detected at a rate of about one per day in the differential acceleration data of LISA Pathfinder. We show that these glitches fall in two rather distinct categories: fast transients in the interferometric motion readout on one side, and true force transient events on the other. …

2022 Physical Review D
LISAPathfinder 22
511 keV line constraints on feebly interacting particles from supernovae
DOI: 10.1103/PhysRevD.105.063026 Bibcode: 2022PhRvD.105f3026C

Calore, Francesca; Carenza, Pierluca; Giannotti, Maurizio +4 more

Feebly interacting particles with masses with O (10 - 100 ) MeV can be copiously produced by core-collapse supernovae (SNe). In this paper we consider the case of MeV-ish sterile neutrinos and dark photons mixed with ordinary neutrinos and photons, respectively. Furthermore, both sterile neutrinos and dark photons may decay into positrons on their…

2022 Physical Review D
INTEGRAL 21
Sensor noise in LISA Pathfinder: An extensive in-flight review of the angular and longitudinal interferometric measurement system
DOI: 10.1103/PhysRevD.106.082001 Bibcode: 2022PhRvD.106h2001A

Mendes, L.; Russano, G.; Sanjuan, J. +84 more

In a previous article [1], we have reported on the first subpicometer interferometer flown in space as part of ESA's LISA Pathfinder mission, and have shown the residual sensor noise to be on the level of 32.0-1.7+2.4 fm /√{Hz } . This review provides a deeper and more complete overview of the full system and its interferomet…

2022 Physical Review D
LISAPathfinder 19
Modeling intrinsic galaxy alignment in the MICE simulation
DOI: 10.1103/PhysRevD.106.123510 Bibcode: 2022PhRvD.106l3510H

Carretero, Jorge; Castander, Francisco J.; DES Collaboration +9 more

The intrinsic alignment (IA) of galaxies is potentially a major limitation in deriving cosmological constraints from weak lensing surveys. In order to investigate this effect, we assign intrinsic shapes and orientations to galaxies in the light-cone output of the MICE simulation, spanning ∼5000 deg2 and reaching redshift z =1.4 . This a…

2022 Physical Review D
eHST 19