Geodesic motion of a test particle around a noncommutative Schwarzchild Anti-de Sitter black hole.

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Title: Geodesic motion of a test particle around a noncommutative Schwarzchild Anti-de Sitter black hole.
Authors: Larbi, Mohamed Aimen1,2 (AUTHOR) mohamedaimen.larbi@univ-batna.dz, Zaim, Slimane2 (AUTHOR) zaim69slimane@yahoo.com, Touati, Abdellah3 (AUTHOR) touati.abph@gmail.com
Source: Modern Physics Letters A. 6/28/2025, Vol. 40 Issue 19/20, p1-15. 15p.
Subjects: Noncommutative geometry, Geodesic motion, Geodesic equation, Pseudopotential method, Black holes, Geodesics
Abstract: In this work, we derive non-commutative corrections to the Schwarzschild-Anti-de Sitter solution up to the first and second orders of the noncommutative parameter Θ. Additionally, we obtain the corresponding deformed effective potentials and the non-commutative geodesic equations for massive particles. Through the analysis of time-like noncommutative geodesics for various values of Θ , we demonstrate that the circular geodesic orbits of the noncommutative Schwarzschild-Anti-de Sitter black hole exhibit greater stability compared to those of the commutative one. Furthermore, we derive corrections to the perihelion deviation angle per revolution as a function of Θ. By applying this result to the perihelion precession of Mercury and utilizing experimental data, we establish a new upper bound on the noncommutative parameter, estimated to be on the order of 1 0 − 6 6 m 2 . [ABSTRACT FROM AUTHOR]
Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Geodesic motion of a test particle around a noncommutative Schwarzchild Anti-de Sitter black hole.
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  Data: <searchLink fieldCode="AR" term="%22Larbi%2C+Mohamed+Aimen%22">Larbi, Mohamed Aimen</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<i> mohamedaimen.larbi@univ-batna.dz</i><br /><searchLink fieldCode="AR" term="%22Zaim%2C+Slimane%22">Zaim, Slimane</searchLink><relatesTo>2</relatesTo> (AUTHOR)<i> zaim69slimane@yahoo.com</i><br /><searchLink fieldCode="AR" term="%22Touati%2C+Abdellah%22">Touati, Abdellah</searchLink><relatesTo>3</relatesTo> (AUTHOR)<i> touati.abph@gmail.com</i>
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  Data: <searchLink fieldCode="JN" term="%22Modern+Physics+Letters+A%22">Modern Physics Letters A</searchLink>. 6/28/2025, Vol. 40 Issue 19/20, p1-15. 15p.
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  Data: <searchLink fieldCode="DE" term="%22Noncommutative+geometry%22">Noncommutative geometry</searchLink><br /><searchLink fieldCode="DE" term="%22Geodesic+motion%22">Geodesic motion</searchLink><br /><searchLink fieldCode="DE" term="%22Geodesic+equation%22">Geodesic equation</searchLink><br /><searchLink fieldCode="DE" term="%22Pseudopotential+method%22">Pseudopotential method</searchLink><br /><searchLink fieldCode="DE" term="%22Black+holes%22">Black holes</searchLink><br /><searchLink fieldCode="DE" term="%22Geodesics%22">Geodesics</searchLink>
– Name: Abstract
  Label: Abstract
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  Data: In this work, we derive non-commutative corrections to the Schwarzschild-Anti-de Sitter solution up to the first and second orders of the noncommutative parameter Θ. Additionally, we obtain the corresponding deformed effective potentials and the non-commutative geodesic equations for massive particles. Through the analysis of time-like noncommutative geodesics for various values of Θ , we demonstrate that the circular geodesic orbits of the noncommutative Schwarzschild-Anti-de Sitter black hole exhibit greater stability compared to those of the commutative one. Furthermore, we derive corrections to the perihelion deviation angle per revolution as a function of Θ. By applying this result to the perihelion precession of Mercury and utilizing experimental data, we establish a new upper bound on the noncommutative parameter, estimated to be on the order of 1 0 − 6 6 m 2 . [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of Modern Physics Letters A is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1142/S0217732325500609
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      – Code: eng
        Text: English
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      Pagination:
        PageCount: 15
        StartPage: 1
    Subjects:
      – SubjectFull: Noncommutative geometry
        Type: general
      – SubjectFull: Geodesic motion
        Type: general
      – SubjectFull: Geodesic equation
        Type: general
      – SubjectFull: Pseudopotential method
        Type: general
      – SubjectFull: Black holes
        Type: general
      – SubjectFull: Geodesics
        Type: general
    Titles:
      – TitleFull: Geodesic motion of a test particle around a noncommutative Schwarzchild Anti-de Sitter black hole.
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            NameFull: Larbi, Mohamed Aimen
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            NameFull: Zaim, Slimane
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            NameFull: Touati, Abdellah
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            – D: 28
              M: 06
              Text: 6/28/2025
              Type: published
              Y: 2025
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              Value: 19/20
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