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Decay orbital period of the binary system on gravitational waves’ detection
Sagita P.Y.D.a, Suroso A.b,c, Zen F.P.b,c
a Department of Physics, Faculty of Mathematics and Natural Sciences, Billfath University of Lamongan, Indonesia
b Department of Physics, Faculty of Mathematics and Natural Sciences, Bandung Institute of Technology, Indonesia
c Indonesia Center for Theoretical and Mathematical Physics (ICTMP), Indonesia, Indonesia
[vc_row][vc_column][vc_row_inner][vc_column_inner][vc_separator css=”.vc_custom_1624529070653{padding-top: 30px !important;padding-bottom: 30px !important;}”][/vc_column_inner][/vc_row_inner][vc_row_inner layout=”boxed”][vc_column_inner width=”3/4″ css=”.vc_custom_1624695412187{border-right-width: 1px !important;border-right-color: #dddddd !important;border-right-style: solid !important;border-radius: 1px !important;}”][vc_empty_space][megatron_heading title=”Abstract” size=”size-sm” text_align=”text-left”][vc_column_text]© Published under licence by IOP Publishing Ltd.Gravitational Waves had been fifth detected which is on PSR 1913+16 at 1974 until 1981 by Arecibo Telescope, on GW150914, GW151226, and GW170104 by LIGO and the last is on GW170814 by LIGO and VIRGO. The research made a binary system dynamic modeling by using linearization theorem and post-Newtonian formalism. This modeling is a binary system with two mass identically orbiting each other on the center of circular orbit. By this modelling will get decay orbital period of system for the fifth data of gravitational waves’ detection is -1,073 x 10-12 for PSR 1913+16, -81,956 x 10-12 for GW150914, -2,56 x 10-12 for GW151226, -73,73 x 10-12 for GW170104, and -44,94 x 10-12 for GW170814. The result can inform us about time which using system to combine be a more massive system (a black hole or a pulsar).[/vc_column_text][vc_empty_space][vc_separator css=”.vc_custom_1624528584150{padding-top: 25px !important;padding-bottom: 25px !important;}”][vc_empty_space][megatron_heading title=”Author keywords” size=”size-sm” text_align=”text-left”][vc_column_text]Binary systems,Black holes,Circular orbit,Massive systems,Newtonians,Orbital periods[/vc_column_text][vc_empty_space][vc_separator css=”.vc_custom_1624528584150{padding-top: 25px !important;padding-bottom: 25px !important;}”][vc_empty_space][megatron_heading title=”Indexed keywords” size=”size-sm” text_align=”text-left”][vc_column_text][/vc_column_text][vc_empty_space][vc_separator css=”.vc_custom_1624528584150{padding-top: 25px !important;padding-bottom: 25px !important;}”][vc_empty_space][megatron_heading title=”Funding details” size=”size-sm” text_align=”text-left”][vc_column_text][/vc_column_text][vc_empty_space][vc_separator css=”.vc_custom_1624528584150{padding-top: 25px !important;padding-bottom: 25px !important;}”][vc_empty_space][megatron_heading title=”DOI” size=”size-sm” text_align=”text-left”][vc_column_text]https://doi.org/10.1088/1742-6596/1171/1/012009[/vc_column_text][/vc_column_inner][vc_column_inner width=”1/4″][vc_column_text]Widget Plumx[/vc_column_text][/vc_column_inner][/vc_row_inner][/vc_column][/vc_row][vc_row][vc_column][vc_separator css=”.vc_custom_1624528584150{padding-top: 25px !important;padding-bottom: 25px !important;}”][/vc_column][/vc_row]