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Significant progress has been made in recent years in constraining thedensity dependence of nuclear symmetry energy using terrestrial nuclearlaboratory data. Around and below the nuclear matter saturation density, theexperimental constraints start to merge in a relatively narrow region. Atsupra-saturation densities, there are, however, still large uncertainties.After summarizing the latest experimental constraints on the density dependenceof nuclear symmetry energy, we highlight a few recent studies examiningimprints of nuclear symmetry energy on the binding energy, energy releaseduring hadron-quark phase transitions as well as the $w$-mode frequency anddamping time of gravitational wave emission of neutron stars.

Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars