Tidal effects in the vicinity of rotating ModMax black hole.

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Title: Tidal effects in the vicinity of rotating ModMax black hole.
Authors: Asgher, M.1 (AUTHOR) m.asgher145@gmail.com, Abbas, G.1 (AUTHOR) ghulamabbas@iub.edu.pk, Güdekli, Ertan2 (AUTHOR) gudekli@istanbul.edu.tr, Nazar, H.3 (AUTHOR) hamad.nazar@khazar.org, Mannanova, Shakhida4 (AUTHOR) sh.mannanova@tsue.uz
Source: International Journal of Geometric Methods in Modern Physics. Sep2025, Vol. 22 Issue 10, p1-18. 18p.
Subjects: Tidal forces (Mechanics), Geodesic motion, Angular momentum (Mechanics), Kerr black holes, Tangential force, Black holes
Abstract: In this paper, we study the radial and angular tidal forces in the vicinity of rotating ModMax black hole. The radial tidal forces intensify with an increase in charge but diminish as the ModMax parameter, γ , increases. Consequently, the angular tidal forces become less effective as the charge increases and become substantially stronger as the γ parameter increases. Furthermore, we analyze the behavior of the geodesic deviation vectors η 1 ̂ and η î in the radial and angular direction, respectively. Increasing the magnitude of charge causes the radial geodesic deviation vector η 1 ̂ to move toward the center of the black hole. In contrast, the deviation increases as the value of the spin parameter increases. The radial geodesic deviation vector compresses to certain range before stretching continuously, as the values of radial coordinate r and γ grow rapidly. [ABSTRACT FROM AUTHOR]
Copyright of International Journal of Geometric Methods in Modern Physics 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: Tidal effects in the vicinity of rotating ModMax black hole.
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  Data: <searchLink fieldCode="AR" term="%22Asgher%2C+M%2E%22">Asgher, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> m.asgher145@gmail.com</i><br /><searchLink fieldCode="AR" term="%22Abbas%2C+G%2E%22">Abbas, G.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> ghulamabbas@iub.edu.pk</i><br /><searchLink fieldCode="AR" term="%22Güdekli%2C+Ertan%22">Güdekli, Ertan</searchLink><relatesTo>2</relatesTo> (AUTHOR)<i> gudekli@istanbul.edu.tr</i><br /><searchLink fieldCode="AR" term="%22Nazar%2C+H%2E%22">Nazar, H.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<i> hamad.nazar@khazar.org</i><br /><searchLink fieldCode="AR" term="%22Mannanova%2C+Shakhida%22">Mannanova, Shakhida</searchLink><relatesTo>4</relatesTo> (AUTHOR)<i> sh.mannanova@tsue.uz</i>
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  Data: <searchLink fieldCode="JN" term="%22International+Journal+of+Geometric+Methods+in+Modern+Physics%22">International Journal of Geometric Methods in Modern Physics</searchLink>. Sep2025, Vol. 22 Issue 10, p1-18. 18p.
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  Data: <searchLink fieldCode="DE" term="%22Tidal+forces+%28Mechanics%29%22">Tidal forces (Mechanics)</searchLink><br /><searchLink fieldCode="DE" term="%22Geodesic+motion%22">Geodesic motion</searchLink><br /><searchLink fieldCode="DE" term="%22Angular+momentum+%28Mechanics%29%22">Angular momentum (Mechanics)</searchLink><br /><searchLink fieldCode="DE" term="%22Kerr+black+holes%22">Kerr black holes</searchLink><br /><searchLink fieldCode="DE" term="%22Tangential+force%22">Tangential force</searchLink><br /><searchLink fieldCode="DE" term="%22Black+holes%22">Black holes</searchLink>
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  Data: In this paper, we study the radial and angular tidal forces in the vicinity of rotating ModMax black hole. The radial tidal forces intensify with an increase in charge but diminish as the ModMax parameter, γ , increases. Consequently, the angular tidal forces become less effective as the charge increases and become substantially stronger as the γ parameter increases. Furthermore, we analyze the behavior of the geodesic deviation vectors η 1 ̂ and η î in the radial and angular direction, respectively. Increasing the magnitude of charge causes the radial geodesic deviation vector η 1 ̂ to move toward the center of the black hole. In contrast, the deviation increases as the value of the spin parameter increases. The radial geodesic deviation vector compresses to certain range before stretching continuously, as the values of radial coordinate r and γ grow rapidly. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
  Group: Ab
  Data: <i>Copyright of International Journal of Geometric Methods in Modern Physics 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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RecordInfo BibRecord:
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    Identifiers:
      – Type: doi
        Value: 10.1142/S0219887825400249
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      – Code: eng
        Text: English
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      Pagination:
        PageCount: 18
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    Subjects:
      – SubjectFull: Tidal forces (Mechanics)
        Type: general
      – SubjectFull: Geodesic motion
        Type: general
      – SubjectFull: Angular momentum (Mechanics)
        Type: general
      – SubjectFull: Kerr black holes
        Type: general
      – SubjectFull: Tangential force
        Type: general
      – SubjectFull: Black holes
        Type: general
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      – TitleFull: Tidal effects in the vicinity of rotating ModMax black hole.
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            – D: 15
              M: 09
              Text: Sep2025
              Type: published
              Y: 2025
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