The values of mass function according to the constant <i>H</i> and
<p>The values of mass function according to the constant <i>H</i> and </p>
محفوظ في:
| المؤلف الرئيسي: | |
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| مؤلفون آخرون: | , , , |
| منشور في: |
2025
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| الموضوعات: | |
| الوسوم: |
إضافة وسم
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| _version_ | 1852020198107774976 |
|---|---|
| author | A. Zahra (19484713) |
| author2 | S. A. Mardan (19484716) Sana Saleem (3551681) Muhammad Bilal Riaz (14341552) Tomas Kozubek (21395600) |
| author2_role | author author author author |
| author_facet | A. Zahra (19484713) S. A. Mardan (19484716) Sana Saleem (3551681) Muhammad Bilal Riaz (14341552) Tomas Kozubek (21395600) |
| author_role | author |
| dc.creator.none.fl_str_mv | A. Zahra (19484713) S. A. Mardan (19484716) Sana Saleem (3551681) Muhammad Bilal Riaz (14341552) Tomas Kozubek (21395600) |
| dc.date.none.fl_str_mv | 2025-05-20T18:02:07Z |
| dc.identifier.none.fl_str_mv | 10.1371/journal.pone.0321111.t001 |
| dc.relation.none.fl_str_mv | https://figshare.com/articles/dataset/The_values_of_mass_function_according_to_the_constant_i_H_i_and/29113643 |
| dc.rights.none.fl_str_mv | CC BY 4.0 info:eu-repo/semantics/openAccess |
| dc.subject.none.fl_str_mv | Biophysics Biotechnology Evolutionary Biology Ecology Marine Biology Inorganic Chemistry Science Policy Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified necessary energy conditions modified chaplygin equation maxwell field equations matter distribution within several compact objects relativistic stellar objects hydrostatic equilibrium condition possibly exotic stars star &# 8217 relativistic charged spheres metric </ p buchdahl ansatz provides including neutron stars stellar equilibrium compact stars buchdahl ansatz xlink "> surface redshift static configurations results demonstrate realistic description psr j2215 psr j1614 psr j0952 psr j0740 psr j0030 pressure occur presented graphically physical viability maximum density gw 190814 gw 170817 electric charge charged sphere behaved throughout avoiding singularities anisotropic fluid adiabatic index 4u 1608 |
| dc.title.none.fl_str_mv | The values of mass function according to the constant <i>H</i> and |
| dc.type.none.fl_str_mv | Dataset info:eu-repo/semantics/publishedVersion dataset |
| description | <p>The values of mass function according to the constant <i>H</i> and </p> |
| eu_rights_str_mv | openAccess |
| id | Manara_f8bc2bbb7f8e62cb77a956ee0da3eb9d |
| identifier_str_mv | 10.1371/journal.pone.0321111.t001 |
| network_acronym_str | Manara |
| network_name_str | ManaraRepo |
| oai_identifier_str | oai:figshare.com:article/29113643 |
| publishDate | 2025 |
| repository.mail.fl_str_mv | |
| repository.name.fl_str_mv | |
| repository_id_str | |
| rights_invalid_str_mv | CC BY 4.0 |
| spelling | The values of mass function according to the constant <i>H</i> and A. Zahra (19484713)S. A. Mardan (19484716)Sana Saleem (3551681)Muhammad Bilal Riaz (14341552)Tomas Kozubek (21395600)BiophysicsBiotechnologyEvolutionary BiologyEcologyMarine BiologyInorganic ChemistryScience PolicyBiological Sciences not elsewhere classifiedPhysical Sciences not elsewhere classifiednecessary energy conditionsmodified chaplygin equationmaxwell field equationsmatter distribution withinseveral compact objectsrelativistic stellar objectshydrostatic equilibrium conditionpossibly exotic starsstar &# 8217relativistic charged spheresmetric </ pbuchdahl ansatz providesincluding neutron starsstellar equilibriumcompact starsbuchdahl ansatzxlink ">surface redshiftstatic configurationsresults demonstraterealistic descriptionpsr j2215psr j1614psr j0952psr j0740psr j0030pressure occurpresented graphicallyphysical viabilitymaximum densitygw 190814gw 170817electric chargecharged spherebehaved throughoutavoiding singularitiesanisotropic fluidadiabatic index4u 1608<p>The values of mass function according to the constant <i>H</i> and </p>2025-05-20T18:02:07ZDatasetinfo:eu-repo/semantics/publishedVersiondataset10.1371/journal.pone.0321111.t001https://figshare.com/articles/dataset/The_values_of_mass_function_according_to_the_constant_i_H_i_and/29113643CC BY 4.0info:eu-repo/semantics/openAccessoai:figshare.com:article/291136432025-05-20T18:02:07Z |
| spellingShingle | The values of mass function according to the constant <i>H</i> and A. Zahra (19484713) Biophysics Biotechnology Evolutionary Biology Ecology Marine Biology Inorganic Chemistry Science Policy Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified necessary energy conditions modified chaplygin equation maxwell field equations matter distribution within several compact objects relativistic stellar objects hydrostatic equilibrium condition possibly exotic stars star &# 8217 relativistic charged spheres metric </ p buchdahl ansatz provides including neutron stars stellar equilibrium compact stars buchdahl ansatz xlink "> surface redshift static configurations results demonstrate realistic description psr j2215 psr j1614 psr j0952 psr j0740 psr j0030 pressure occur presented graphically physical viability maximum density gw 190814 gw 170817 electric charge charged sphere behaved throughout avoiding singularities anisotropic fluid adiabatic index 4u 1608 |
| status_str | publishedVersion |
| title | The values of mass function according to the constant <i>H</i> and |
| title_full | The values of mass function according to the constant <i>H</i> and |
| title_fullStr | The values of mass function according to the constant <i>H</i> and |
| title_full_unstemmed | The values of mass function according to the constant <i>H</i> and |
| title_short | The values of mass function according to the constant <i>H</i> and |
| title_sort | The values of mass function according to the constant <i>H</i> and |
| topic | Biophysics Biotechnology Evolutionary Biology Ecology Marine Biology Inorganic Chemistry Science Policy Biological Sciences not elsewhere classified Physical Sciences not elsewhere classified necessary energy conditions modified chaplygin equation maxwell field equations matter distribution within several compact objects relativistic stellar objects hydrostatic equilibrium condition possibly exotic stars star &# 8217 relativistic charged spheres metric </ p buchdahl ansatz provides including neutron stars stellar equilibrium compact stars buchdahl ansatz xlink "> surface redshift static configurations results demonstrate realistic description psr j2215 psr j1614 psr j0952 psr j0740 psr j0030 pressure occur presented graphically physical viability maximum density gw 190814 gw 170817 electric charge charged sphere behaved throughout avoiding singularities anisotropic fluid adiabatic index 4u 1608 |