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<doi_batch_id>-3dc97f3d182b6b0ed3d-437a</doi_batch_id>
<timestamp>20221010191122488</timestamp>
<depositor>
  <depositor_name>hyperscienceij@gmail.com:rcrl</depositor_name> 
  <email_address>hyperscienceij@gmail.com</email_address>
</depositor>
<registrant>WEB-FORM</registrant> 
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<journal>
<journal_metadata>   <full_title>Hyperscience International Journals</full_title>   <abbrev_title>HIJ</abbrev_title>   <issn media_type='electronic'>28213300</issn> </journal_metadata> <journal_issue>  <publication_date media_type='online'>     <month>09</month>     <year>2022</year>   </publication_date>   <journal_volume>     <volume>2</volume>   </journal_volume>   <issue>3</issue> </journal_issue><!-- ============== --> <journal_article publication_type='full_text'>   <titles>     <title>Lagrangian Solution of Schwarzschild-like Metric for an ‎Elliptical Object</title>   </titles>   <contributors>      <organization sequence='first' contributor_role='author'>Department of Physics, Islamic Azad University (IAU)-Varamin-Pishva Branch, Varamin, Iran</organization>    <person_name sequence='first' contributor_role='author'>      <given_name>Bijan</given_name>      <surname>Nikouravan</surname>      <ORCID>https://orcid.org/0000-0003-4308-1632</ORCID>    </person_name>    <person_name sequence='additional' contributor_role='author'>       <given_name>Misha</given_name>       <surname>Nikouravan</surname>       <ORCID>https://orcid.org/0000-0003-1976-8848</ORCID>     </person_name>     <organization sequence='additional' contributor_role='author'>Department of Engineering, Sharif University, Tehran, Iran</organization>   </contributors>    <jats:abstract xml:lang='en'>         <jats:p>Lagrangian method applied as well as tensor method, for a linear transformed geodesic line element of Schwarzschild-like The ‎Lagrangian method was applied for a linearly transformed geodesic line element of a Schwarzschild-like solution instead of ‎the tensor method. The solution shows that it is not only valid for spherical objects but also it is more comprehensive for ‎elliptical celestial objects. Two types of kinetic and potential energy are the basis of the calculation. Hamiltonian and ‎Lagrangian equality show that the problem has no potential energy. With this transformed geodesic line element, we obtained ‎a new coefficient for the meridional advance of an experimental particle in Schwarzschild spacetime in terms of period, ‎eccentricity, and mean distance. This new perigee equation is not only valid for the Schwarzschild metric (for a spherical ‎object), but also more accurate for the Schwarzschild-like metric (for elliptical objects).‎</jats:p>     </jats:abstract>  <publication_date media_type='online'>     <month>09</month>     <year>2022</year>   </publication_date>   <pages>     <first_page>209</first_page>     <last_page>216</last_page>   </pages>   <doi_data>     <doi>10.55672/hij2022pp209-216</doi>     <resource>https://hscience.org/index.php/hij/article/view/59</resource>   </doi_data> </journal_article>
</journal>
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