Events1st Electronic Conference on Universe
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This submission belongs to the session S7. Deep-Space Probes of the event 1st Electronic Conference on Universe
Published date
22 Feb, 2021
Citation
David Lucchesi, Luciano Anselmo, Massimo Bassan, Marco Lucente, Carmelo Magnafico, Carmen Pardini, Roberto Peron, Giuseppe Pucacco, Massimo Visco, Testing General Relativity vs. Alternative Theories of Gravitation with the SaToR-G Experiment, in Proceedings of 1st Electronic Conference on Universe, 22 February–28 February 2021, MDPI: Basel, Switzerland, doi: 10.3390/ECU2021-09274
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Testing General Relativity vs. Alternative Theories of Gravitation with the SaToR-G Experiment

Luciano Anselmo 3
image
Carmen Pardini 3
Massimo Visco 2,5
1. National Institute for Astrophysics (INAF/IAPS), Via Fosso del Cavaliere n. 100, 00133 Tor Vergata, Roma, Italy, Italy
2. Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, Via della Ricerca Scientifica n. 1, 00133 Roma, Italy
3. Istituto di Scienza e Tecnologie dell’Informazione (ISTI)—Consiglio Nazionale delle Ricerche, Via G. Moruzzi n. 1, 56124 Pisa, Italy
4. Dipartimento di Fisica, Università di Roma Tor Vergata, Via della Ricerca Scientifica n. 1, 00133 Roma, Italy
5. National Institute for Astrophysics (INAF/IAPS), Via Fosso del Cavaliere n. 100, 00133 Tor Vergata, Roma, Italy
Abstract

SaToR-G (Satellites Tests of Relativistic Gravity) is a new experiment of gravitation that aims to test the gravitational interaction beyond the predictions of General Relativity (GR) in search for effects foreseen by other alternative theories of gravitation and possibly connected with “new physics”. SaToR-G is financed by the Astroparticle Physics Experiments of the Italian “Istituto Nazionale di Fisica Nucleare” (INFN) and takes advantage of the improved dynamical model of the two LAGEOS laser-ranged satellites and of the LARES one achieved within the previous experiment LARASE (LAser RAnged Satellites Experiment). The improvements mainly concern the modeling of the non-conservative forces (NCF) acting on the surface of the satellites considered and that of the Earth's gravitational field during their precise orbit determination (POD). Regarding the NCF, the main efforts were in the development of a model for the spin of the satellites (LASSOS: LArase Satellites Spin mOdel Solutions) and a model for thermal thrust forces (LATOS: LArase Thermal mOdel Solutions). For the gravitational field, the monthly solutions of the GRACE mission have been implemented in the code used for the POD. After a summary of the main results obtained by LARASE in the field of gravitation the main objectives of SaToR-G and the planned strategy for achieving them will be presented.

Keywords
General Relativity
Alternative theories of gravitation
LAGEOS satellites
Satellite Laser Ranging
Non-conservative forces
GRACE mission
Manuscript
Poster
Lucchesi_et_al_Sator-g_Deep-Space_Probes.pdf
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