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This paper presents an estimate for the spectral properties of the stochastic background of gravitational waves emitted by a population of hot, young, rapidly rotating neutron stars throughout the Universe undergoing $f$-mode instabilities, formed through either core-collapse supernova explosions or the merger of binary neutron star systems.
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Pnigouras, P. & Kokkotas, K. D. 2015, Phys. Rev. D, 92, 084018
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Pnigouras, P. & Kokkotas, K. D. 2016, in preparation
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