{"id":22669868,"url":"https://github.com/astrobarker/tovpy","last_synced_at":"2025-03-29T11:15:34.500Z","repository":{"id":215136960,"uuid":"738211152","full_name":"AstroBarker/tovpy","owner":"AstroBarker","description":"Python based Tolman–Oppenheimer–Volkoff (TOV) solver","archived":false,"fork":false,"pushed_at":"2024-01-28T21:12:01.000Z","size":24,"stargazers_count":0,"open_issues_count":0,"forks_count":0,"subscribers_count":1,"default_branch":"main","last_synced_at":"2025-02-04T10:56:40.345Z","etag":null,"topics":[],"latest_commit_sha":null,"homepage":null,"language":"Python","has_issues":true,"has_wiki":null,"has_pages":null,"mirror_url":null,"source_name":null,"license":"gpl-3.0","status":null,"scm":"git","pull_requests_enabled":true,"icon_url":"https://github.com/AstroBarker.png","metadata":{"files":{"readme":"README.md","changelog":null,"contributing":null,"funding":null,"license":"LICENSE","code_of_conduct":null,"threat_model":null,"audit":null,"citation":null,"codeowners":null,"security":null,"support":null,"governance":null,"roadmap":null,"authors":null,"dei":null,"publiccode":null,"codemeta":null}},"created_at":"2024-01-02T17:33:42.000Z","updated_at":"2024-01-02T17:45:02.000Z","dependencies_parsed_at":"2024-01-02T18:47:21.207Z","dependency_job_id":"294f011a-5cab-43c8-bd45-87db6dee1e47","html_url":"https://github.com/AstroBarker/tovpy","commit_stats":null,"previous_names":["astrobarker/tovpy"],"tags_count":0,"template":false,"template_full_name":null,"repository_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/AstroBarker%2Ftovpy","tags_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/AstroBarker%2Ftovpy/tags","releases_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/AstroBarker%2Ftovpy/releases","manifests_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories/AstroBarker%2Ftovpy/manifests","owner_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners/AstroBarker","download_url":"https://codeload.github.com/AstroBarker/tovpy/tar.gz/refs/heads/main","host":{"name":"GitHub","url":"https://github.com","kind":"github","repositories_count":246174609,"owners_count":20735417,"icon_url":"https://github.com/github.png","version":null,"created_at":"2022-05-30T11:31:42.601Z","updated_at":"2022-07-04T15:15:14.044Z","host_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub","repositories_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repositories","repository_names_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/repository_names","owners_url":"https://repos.ecosyste.ms/api/v1/hosts/GitHub/owners"}},"keywords":[],"created_at":"2024-12-09T15:41:50.318Z","updated_at":"2025-03-29T11:15:34.466Z","avatar_url":"https://github.com/AstroBarker.png","language":"Python","funding_links":[],"categories":[],"sub_categories":[],"readme":"# tovpy\nA Python based Tolman–Oppenheimer–Volkoff (TOV) solver for the structure of a simple neutron star.\nCan be used to produce mass radius plots.\nSupports both polytropic equation of state as well as tabulated nuclear equations of state.\nFor nuclear equations of state, use tables from [StellarCollapse](https://stellarcollapse.org/microphysics.html)\n\nWith the nuclear equation of state, we assume a cold neutron star (minimum temperature of the table) and beta equilibrium.\n\nIncludes forward Euler and RK4 temporal integration.\n\n## Dependencies\n - numpy\n - matplotlib\n - astropy\n - numba\n","project_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fastrobarker%2Ftovpy","html_url":"https://awesome.ecosyste.ms/projects/github.com%2Fastrobarker%2Ftovpy","lists_url":"https://awesome.ecosyste.ms/api/v1/projects/github.com%2Fastrobarker%2Ftovpy/lists"}