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The gravitational-wave detections of binary black hole mergers suggest the possibility of detecting gravitational waves from binaries consisting of compact stars in the near future. During the merger, the compact stars leave their footprints on the gravitational-wave signals through their tidal deformability. Therefore the detections of these signals can constrain the equation of state of ultra-dense matter. We present the prospects of constraining the nuclear equation of state with gravitational-wave signals in the Advanced detector era and beyond.

Prospects of Constraining the Nuclear Equation of State with Gravitational-Wave Signals in the Advanced Detector Era and Beyond