Formation of bound states in quintessence alternative theories.

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Title: Formation of bound states in quintessence alternative theories.
Authors: Koutsoumbas, George1 (AUTHOR) kutsubas@central.ntua.gr, Machattou, Andri1 (AUTHOR) andrimachattou@hotmail.com, Papantonopoulos, Eleftherios1 (AUTHOR) lpapa@central.ntua.gr
Source: European Physical Journal C -- Particles & Fields. Jun2026, Vol. 86 Issue 6, p1-10. 10p.
Subjects: Black holes, Phase transitions, Helmholtz free energy, Heat capacity, Hawking radiation
Abstract: We study RNAdS black holes in the presence of quintessence matter. We find that the presence of quintessence influences significantly the metric function and the Hawking temperature. For this kind of black holes phase transitions are present. We spot the phase transition points using the corresponding heat capacities, as well as the Helmholtz free energy for the canonical thermodynamic ensemble. Calculating the Regge and Wheeler potential for scalar perturbations, we find out that no bound states are present for stable RNAdS black holes in the presence of quintessence matter. [ABSTRACT FROM AUTHOR]
Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature 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: <searchLink fieldCode="JN" term="%22European+Physical+Journal+C+--+Particles+%26+Fields%22">European Physical Journal C -- Particles & Fields</searchLink>. Jun2026, Vol. 86 Issue 6, p1-10. 10p.
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  Data: <searchLink fieldCode="DE" term="%22Black+holes%22">Black holes</searchLink><br /><searchLink fieldCode="DE" term="%22Phase+transitions%22">Phase transitions</searchLink><br /><searchLink fieldCode="DE" term="%22Helmholtz+free+energy%22">Helmholtz free energy</searchLink><br /><searchLink fieldCode="DE" term="%22Heat+capacity%22">Heat capacity</searchLink><br /><searchLink fieldCode="DE" term="%22Hawking+radiation%22">Hawking radiation</searchLink>
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  Data: We study RNAdS black holes in the presence of quintessence matter. We find that the presence of quintessence influences significantly the metric function and the Hawking temperature. For this kind of black holes phase transitions are present. We spot the phase transition points using the corresponding heat capacities, as well as the Helmholtz free energy for the canonical thermodynamic ensemble. Calculating the Regge and Wheeler potential for scalar perturbations, we find out that no bound states are present for stable RNAdS black holes in the presence of quintessence matter. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of European Physical Journal C -- Particles & Fields is the property of Springer Nature 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: 10.1140/epjc/s10052-026-15863-1
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        Text: English
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        Type: general
      – SubjectFull: Phase transitions
        Type: general
      – SubjectFull: Helmholtz free energy
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      – SubjectFull: Heat capacity
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      – SubjectFull: Hawking radiation
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      – TitleFull: Formation of bound states in quintessence alternative theories.
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              M: 06
              Text: Jun2026
              Type: published
              Y: 2026
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