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Autor:
Miller, Andrew, Astone, Pia, D'Antonio, Sabrina, Frasca, Sergio, Intini, Giuseppe, La Rosa, Iuri, Leaci, Paola, Mastrogiovanni, Simone, Muciaccia, Federico, Palomba, Cristiano, Piccinni, Ornella J., Signhal, Akshat, Whiting, Bernard F.
Publikováno v:
Phys. Rev. D (2018) 98, 102004
We describe a method to detect gravitational waves lasting $O(hours-days)$ emitted by young, isolated neutron stars, such as those that could form after a supernova or a binary neutron star merger, using advanced LIGO/Virgo data. The method is based
Externí odkaz:
http://arxiv.org/abs/1810.09784
