Astrophysics

    

Nachweis Der Kontinuierlichen Gravitationswelle Von HM Cancri (Detection of the Continuous Gravitational Wave of HM Cancri)

Authors: Herbert Weidner

HM Cancri ist möglicherweise die intensivste Quelle kontinuierlicher GW in unserer Galaxie. Trotz bekannter Frequenz konnte die Strahlung mangels geeigneter Sensoren bisher nicht nachgewiesen werden. Ein neuartiges Verfahrens kann die Phasenmodulation kompensieren und diese CGW in den Aufzeichnungen supraleitender Gravimeter zweifelsfrei nachweisen. Diese neuartige Beobachtungsfenster wird ein tieferes Verständnis des rätselhaften Sternsystems ermöglichen.

HM Cancri is expected to be one of the brightest sources of gravitational waves in our galaxy. Despite its known frequency, the radiation could not be detected so far. A new technique can compensate for the phase modulation and detect this CGW in the records of supraconducting gravimeters beyond doubt. This novel observational window will allow a deeper understanding of the enigmatic stellar system.

Comments: 10 Pages.

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Submission history

[v1] 2022-01-25 19:47:55

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