Hi Nisa,
This can be done using the set of routines available in Lorene/Codes/Bin_star. Running the codes init_bin and coal should make the ID file resu.d and some description of the NSs (calcul.d). There are several parameters that can be tweaked to obtain the BNS ID you need exactly.
The process is also described in this tutorial posted on ET's youtube channel.(Starting at about 15:30) https://www.youtube.com/watch?v=-NUD-piBeek&t=932s.
There is also some documentation we prepared for the ET workshop last year and it links to several other useful resources. https:// docs.google.com/document/d/1NniHTBucMjE14uPBj_YinBE0XvPUgcGAKyVdQXLuJSk/edit?usp=sharing
Let us know if this helps or if you have any questions.
Atul
On Sun, Mar 13, 2022 at 5:54 PM Nisa Amir nisaamir@math.qau.edu.pk wrote:
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How can i reproduce initial data file (e.g G2_I12vs12_D4R33T21_45km.resu https://secure-web.cisco.com/1WIFY2aC5ZNWiXmYUlWn-ewBFDiuNUptTNvmGHxlC5Ak_zyrqMI0g0VDQCb0p9ciigUu2964WJF_4YpjLes30EmIEcan5tRZeSHREM7lzVPDv1fwAPbuSheWWVeDp-D6lfoHiVWBAE5xFigtgT5kFAYriDFfNPOpAlGf8uVwOqVnDyG2orPChO4lYfE8AxRg7K_Tz55vIxcEbTFUwJEQuJ-Ijz_zfVYVOwOXvmnK2FjnX8dBatNCFSZrSym-A2WsI_HDWtUmXQIj8-o2xx6T8dUk2RFzVGpAx-ZKfFqzOwnTsmJ9DFwnzPU6Aubhx0iLGKrivxmO5byvMvQRMbN0mcPAFckU0tvv9m6wbqk8i3FsbCmQe0EBG-BpR5JiDs_qIUHMpN_ELwFECJAcJ5IkYL-Os9MxGtV32MwDtfVqFrhc/https%3A%2F%2Feinsteintoolkit.org%2Fgallery%2Fbns%2FG2_I12vs12_D4R33T21_45km.resu.xz) for a new neutron star parameters with LORENE code?
I have already installed and compiled the LORENE, but do not know what to do afterwards.
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