Search Publications

In the realm of the Hubble tension-a review of solutions
DOI: 10.1088/1361-6382/ac086d Bibcode: 2021CQGra..38o3001D

Riess, Adam G.; Di Valentino, Eleonora; Melchiorri, Alessandro +6 more

The simplest ΛCDM model provides a good fit to a large span of cosmological data but harbors large areas of phenomenology and ignorance. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the 4σ to 6σ disagreem…

2021 Classical and Quantum Gravity
Gaia 1554
Light propagation in 2PN approximation in the field of one moving monopole II. Boundary value problem
DOI: 10.1088/1361-6382/aaeb4c Bibcode: 2019CQGra..36a5007Z

Zschocke, Sven

In this investigation the boundary value problem of light propagation in the gravitational field of one arbitrarily moving body with monopole structure is considered in the second post-Newtonian approximation. The solution of the boundary value problem comprises a set of altogether three transformations: , , and . Analytical solutions of these tra…

2019 Classical and Quantum Gravity
Gaia 7
Gaia-like astrometry and gravitational waves
DOI: 10.1088/1361-6382/aa9f57 Bibcode: 2018CQGra..35d5005K

Klioner, Sergei A.

This paper discusses the effects of gravitational waves on high-accuracy astrometric observations such as those delivered by Gaia. Depending on the frequency of gravitational waves, two regimes for the influence of gravitational waves on astrometric data are identified: the regime when the effects of gravitational waves directly influence the deri…

2018 Classical and Quantum Gravity
Gaia 43
Light propagation in 2PN approximation in the field of one moving monopole I. Initial value problem
DOI: 10.1088/1361-6382/aa9976 Bibcode: 2018CQGra..35e5013Z

Zschocke, Sven

In this investigation the light propagation in the gravitational field of one arbitrarily moving body with monopole structure is considered in the second post-Newtonian approximation. It is found that the light trajectory depends on the acceleration of the body. Some of these acceleration terms are important in order to get well-defined logarithmi…

2018 Classical and Quantum Gravity
Gaia 10
The ray tracing analytical solution within the RAMOD framework. The case of a Gaia-like observer
DOI: 10.1088/0264-9381/32/16/165008 Bibcode: 2015CQGra..32p5008C

Lattanzi, M. G.; Crosta, M.; Vecchiato, A. +1 more

This paper presents the analytical solution of the inverse ray tracing problem for photons emitted by a star and collected by an observer located in the gravitational field of the Solar System. This solution has been conceived to suit the accuracy achievable by the ESA Gaia satellite (launched on 19 December 2013) consistently with the measurement…

2015 Classical and Quantum Gravity
Gaia 10
Time transfer functions as a way to validate light propagation solutions for space astrometry
DOI: 10.1088/0264-9381/31/1/015021 Bibcode: 2014CQGra..31a5021B

Bertone, Stefano; Crosta, Mariateresa; Vecchiato, Alberto +3 more

Given the extreme accuracy of modern space astrometry, a precise relativistic modeling of observations is required. Concerning light propagation, the standard procedure is the solution of the null-geodesic equations. However, another approach based on the time transfer functions (TTF) has demonstrated its capability to give access to key quantitie…

2014 Classical and Quantum Gravity
Gaia 24