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I in collaboration with Todd Thompson's group have been doing non-relativistic PNS spindown simulations. See https://ui.adsabs.harvard.edu/search/fq=%7B!type%3Daqp%20v%3D%24fq_database%7D&fq_database=(database%3Aastronomy%20OR%20database%3Aphysics)&q=author%3A%22thompson%2C%20t%22%20author%3A%22%20Coleman%2C%20m%22&sort=date%20desc%2C%20bibcode%20desc&p_=0 The primary reason that we haven't gone relativistic yet is there is no support for the general EOS module in GR. I am the author of the EOS module, and I'm no longer a full time researcher; I'm now part of the HPC team at Princeton University (but I still get time for research). I'm only willing to share code/input files with my collaborators okay. But that discussion can be started after I get back from vacation. |
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Hi everyone,
I'm a researcher at Phenikaa University working in the field of gravitational-wave data analysis, particularly with ground-based detectors.
We're currently exploring the use of Athena++ to simulate magnetars, with the goal of building on the work by Ankan Sur et al. (2021) to create a gravitational-wave catalog informed by GRMHD simulations.
Given how crucial the input file configuration is to running Athena++ simulations effectively, I'm reaching out to ask if anyone has experience or suggestions for setting up an initial input file suitable for simulating the dynamics of a magnetized, spinning neutron star. Any tips, examples, or starting points would be greatly appreciated.
If anyone is open to discussing this further (perhaps over a Zoom call), I’d be happy to coordinate a time that works for you.
Thanks in advance for your help!
Best,
Peter
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