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oai:docta.ucm.es:20.500.14352/181642023-08-27T20:46:34Zcom_20.500.14352_14col_20.500.14352_15

Llanes Estrada, Felipe José 2023-06-17T22:10:11Z 2023-06-17T22:10:11Z 2017 2100-014X 10.1051/epjconf/201713701013 https://hdl.handle.net/20.500.14352/18164 http://dx.doi.org/10.1051/epjconf/201713701013 https://www.epj-conferences.org The finding of Gravitational Waves (GW) by the aLIGO scientific and VIRGO collaborations opens opportunities to better test and understand strong interactions, both nuclear-hadronic and gravitational. Assuming General Relativity holds, one can constrain hadron physics at a neutron star. But precise knowledge of the Equation of State and transport properties in hadron matter can also be used to constrain the theory of gravity itself. I review a couple of these opportunities in the context of modified f(R) gravity, the maximum mass of neutron stars, and progress in the Equation of State of neutron matter from the chiral effective field theory of QCD. eng https://creativecommons.org/licenses/by/3.0/es/ open access Atribución 3.0 España Constraining gravity with hadron physics: neutron stars, modified gravity and gravitational waves journal article