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Efficiency of template banks for highly-eccentric gravitational-wave sources D NIEL B ARTA D NIEL B ARTA W IGNER R ESEARCH C ENTRE FOR P HYSICS , Budapest W IGNER R ESEARCH C ENTRE FOR P HYSICS , Budapest Ph.D. Student , E TVS L ORND U


  1. Efficiency of template banks for highly-eccentric gravitational-wave sources D ÁNIEL B ARTA D ÁNIEL B ARTA W IGNER R ESEARCH C ENTRE FOR P HYSICS , Budapest W IGNER R ESEARCH C ENTRE FOR P HYSICS , Budapest Ph.D. Student , E ÖTVÖS L ORÁND U NIVERSITY , Budapest Ph.D. Student , E ÖTVÖS L ORÁND U NIVERSITY , Budapest Annual NewCompStar Conference 15 th June 2015

  2. Adaptive stepsize int.  Parametric NDSolve: - Cut off, if the separation reaches 6M ⊙ (Schw. ISCO) - MaxSteps = 10 15 Waveform (2.5PN):

  3. Adaptive stepsize int.  Parametric NDSolve: - Cut off, if the separation reaches 6M ⊙ (Schw. ISCO) - MaxSteps = 10 15 Waveform (2.5PN):

  4. ε M 1 +M 2 0 0.3 0.6 30 M ⊙ Waveform Separation 40 M ⊙ 70 M ⊙

  5. Thank you for your kind attention! Dániel Barta E-mail: barta.daniel@wigner.mta.hu Acknowledgement: I would like to thank the assistance of M. Vasúth ( Wigner RCP ), to B. S. Sathyaprakash and M. Pürrer ( Cardiff University ) for the preliminary introduction to the field and that this work was supported by a STSM Grant of „ NewCompStar ” from the COST Action MP1304 .

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