Search Publications

Space test of the equivalence principle: first results of the MICROSCOPE mission
DOI: 10.1088/1361-6382/ab4707 Bibcode: 2019CQGra..36v5006T

Bergé, Joel; Chhun, Ratana; Métris, Gilles +31 more

The weak equivalence principle (WEP), stating that two bodies of different compositions and/or mass fall at the same rate in a gravitational field (universality of free fall), is at the very foundation of general relativity. The MICROSCOPE mission aims to test its validity to a precision of 10-15, two orders of magnitude better than cur…

2019 Classical and Quantum Gravity
MICROSCOPE 72
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
Measuring fN force variations in the presence of constant nN forces: a torsion pendulum ground test of the LISA Pathfinder free-fall mode
DOI: 10.1088/1361-6382/aaa00f Bibcode: 2018CQGra..35c5017R

Russano, G.; Cavalleri, A.; Cesarini, A. +11 more

LISA Pathfinder is a differential accelerometer with the main goal being to demonstrate the near perfect free-fall of reference test masses, as is needed for an orbiting gravitational wave observatory, with a target sensitivity of 30 fm s-2 Hz-1/2 at 1 mHz. Any lasting background differential acceleration between the two test…

2018 Classical and Quantum Gravity
LISAPathfinder 10
Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski functionals
DOI: 10.1088/1361-6382/aa5ce2 Bibcode: 2017CQGra..34i4002B

Buchert, Thomas; France, Martin J.; Steiner, Frank

Despite the wealth of Planck results, there are difficulties in disentangling the primordial non-Gaussianity of the Cosmic Microwave Background (CMB) from the secondary and the foreground non-Gaussianity (NG). For each of these forms of NG the lack of complete data introduces model-dependences. Aiming at detecting the NGs of the CMB temperature an…

2017 Classical and Quantum Gravity
Planck 43
Constraints on LISA Pathfinder’s self-gravity: design requirements, estimates and testing procedures
DOI: 10.1088/0264-9381/33/23/235015 Bibcode: 2016CQGra..33w5015A

Mendes, L.; Madden, S.; Russano, G. +96 more

LISA Pathfinder satellite was launched on 3 December 2015 toward the Sun-Earth first Lagrangian point (L1) where the LISA Technology Package (LTP), which is the main science payload, will be tested. LTP achieves measurements of differential acceleration of free-falling test masses (TMs) with sensitivity below 3× {10}-14 {{m}} {{{s}}}

2016 Classical and Quantum Gravity
LISAPathfinder 23
On the running of the spectral index to all orders: a new model-dependent approach to constrain inflationary models
DOI: 10.1088/0264-9381/33/11/115008 Bibcode: 2016CQGra..33k5008Z

Zarei, Moslem

In conventional model-independent approaches, the power spectrum of primordial perturbations is characterized by such free parameters as the spectral index, its running, the running of running, and the tensor-to-scalar ratio. In this work we show that, at least for simple inflationary potentials, one can find the primordial scalar and tensor power…

2016 Classical and Quantum Gravity
Planck 21
Composite Inflation in the light of 2015 Planck data
DOI: 10.1088/0264-9381/33/15/157001 Bibcode: 2016CQGra..33o7001C

Channuie, Phongpichit

In this work, we examine cosmological constraints on models of composite inflation based on the slow-roll approximation by using the recent Planck measurement. We compare the spectral index of curvature perturbation (and its running) and the tensor-to-scalar ratio predicted by such models with Planck 2015 data. We find that the predictions of tech…

2016 Classical and Quantum Gravity
Planck 4
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