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Abstract New strong non-spiralling-in gravitational wave (GW) source for LIGO/VIRGO detectors are proposed. Double O Ne–Mg white dwarf mergers can produce strong gravitational waves with frequencies in the several hundreds… Click to show full abstract
Abstract New strong non-spiralling-in gravitational wave (GW) source for LIGO/VIRGO detectors are proposed. Double O Ne–Mg white dwarf mergers can produce strong gravitational waves with frequencies in the several hundreds Hz range. Such events can be followed by a Super Nova type Ia.
Keywords:
gravitational waves;
double one;
source;
ligo virgo;
one white
Journal Title: New Astronomy
Year Published: 2017
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Journal Title: New Astronomy
Year Published: 2017
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!