%0 Journal Article %T Can the maximum mass of neutron stars rule out any equation of state of dense stellar matter before gravity is well understood? %A De-Hua Wen %A Bao-An Li %A Lie-Wen Chen %J Physics %D 2011 %I arXiv %X Probably No! As an example, using soft EOSs consistent with existing terrestrial nuclear laboratory experiments for hybrid neutron stars containing a quark core described with MIT bag model using reasonable parameters, we show that the recently discovered new holder of neutron star maximum mass PSR J1614-2230 of $1.97\pm0.04M_{\odot}$ can be well described by incorporating a Yukawa gravitational correction that is consistent with existing constraints from neutron-proton and neutron-lead scatterings as well as the spectroscopy of antiproton atoms. %U http://arxiv.org/abs/1101.1504v1