Search Publications

Test of general relativity during the BepiColombo interplanetary cruise to Mercury
DOI: 10.1103/PhysRevD.98.064059 Bibcode: 2018PhRvD..98f4059S

Schettino, Giulia; Serra, Daniele; Tommei, Giacomo +1 more

The theory of general relativity first introduced the concept that space-time is curved by the presence of masses. As a consequence, any signal between two sources passing by a massive body is deflected and therefore experiences a transmission time delay with respect to the straight-line propagation. In the parametrized Post-Newtonian formalism—wh…

2018 Physical Review D
Gaia 8
Effects of a caustic ring of dark matter on the distribution of stars and interstellar gas
DOI: 10.1103/PhysRevD.98.103009 Bibcode: 2018PhRvD..98j3009C

Chakrabarty, Sankha S.; Sikivie, Pierre

Caustic rings of dark matter with tricusp cross section were predicted to lie in the galactic disk. Their radii increase on cosmological time scales at a rate of order 1 kpc /Gyr . When a caustic ring passes through the orbit of a star, the orbit is strongly perturbed. We find that a star moving in a nearly circular orbit is first attracted toward…

2018 Physical Review D
Gaia 7
Closing in on the large-scale CMB power asymmetry
DOI: 10.1103/PhysRevD.97.063504 Bibcode: 2018PhRvD..97f3504C

Moss, A.; Scott, D.; Contreras, D. +2 more

Measurements of the cosmic microwave background (CMB) temperature anisotropies have revealed a dipolar asymmetry in power at the largest scales, in apparent contradiction with the statistical isotropy of standard cosmological models. The significance of the effect is not very high, and is dependent on a posteriori choices. Nevertheless, a number o…

2018 Physical Review D
Planck 7
Observational constraints on warm quasi-exponential inflation
DOI: 10.1103/PhysRevD.97.123503 Bibcode: 2018PhRvD..97l3503V

Videla, Nelson; Panotopoulos, Grigorios

In the present work, we study a warm inflationary model defined by a quasi-exponential inflaton potential and an inflaton decay rate proportional to the Hubble rate. The model is characterized by three free parameters. We compute the power spectrum, the scalar spectral index, as well as the tensor-to-scalar ratio within the framework of the model,…

2018 Physical Review D
Planck 7
Astrometric test of the weak equivalence principle
DOI: 10.1103/PhysRevD.98.021501 Bibcode: 2018PhRvD..98b1501X

Xie, Yi

Weak equivalence principle (WEP) is, for the first time, tested by astrometry on quasars in the sky measured in two wavelengths. Compared to previous WEP tests based on the Shapiro time delay of massless particles, this one has profound superiority that nearly 1 700 quasars with best measured positions commonly in the optical and radio bands are a…

2018 Physical Review D
Gaia 6
Gravitational wave effects on astrometric observables
DOI: 10.1103/PhysRevD.98.124036 Bibcode: 2018PhRvD..98l4036B

Bini, Donato; Geralico, Andrea

Observational data from the European Space Agency astrometric mission Gaia determining the positions of celestial objects within an accuracy of a few microarcseconds will be soon fully available. Other satellite-based space missions are currently planned to significantly improve such precision in the next years. The data reduction process needs hi…

2018 Physical Review D
Gaia 4
Strong lensing constraints on modified gravity models
DOI: 10.1103/PhysRevD.98.124027 Bibcode: 2018PhRvD..98l4027D

Dai, De-Chang; Stojkovic, Dejan; Starkman, Glenn D.

We impose the first strong-lensing constraints on a wide class of modified gravity models where an extra field that modifies gravity also couples to photons (either directly or indirectly through a coupling with baryons) and thus modifies lensing. We use the nonsingular isothermal ellipsoid profile as an effective potential which produces flat gal…

2018 Physical Review D
eHST 3