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              <text>Suhasini, K.; Ravi Kiran, G.; Kavya, N.S; Varsha, C.S.; Venkatesha, V.</text>
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              <text>Geometric aspects of noncommutative wormholes with conformal symmetry</text>
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              <text>Physica Scripta;Volume;101;Issue;18;Article No.;185003;</text>
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              <text>&lt;a href="https://doi.org/10.1088/1402-4896/ae648c" target="_blank" rel="noreferrer noopener"&gt;https://doi.org/10.1088/1402-4896/ae648c&lt;/a&gt; &lt;br /&gt;&lt;br /&gt;&lt;a href="https://www.scopus.com/pages/publications/105038145075?origin=resultslist" target="_blank" rel="noreferrer noopener"&gt;https://www.scopus.com/pages/publications/105038145075?origin=resultslist&lt;/a&gt;</text>
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              <text>Suhasini K., Department of Mathematics, SR University, Ananthasagar, Hasanparthy, Telangana, Warangal, 506371, India; Ravi Kiran G., Department of Mathematics, SR University, Ananthasagar, Hasanparthy, Telangana, Warangal, 506371, India; Kavya N.S., Centre for Mathematical Needs, Department of Mathematics, CHRIST (Deemed to be University), Bengaluru, 560029, India; Varsha C.S., Department of P.G. Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shivamogga, 577451, India; Venkatesha V., Department of P.G. Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shivamogga, 577451, India</text>
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              <text>This paper investigates traversable wormhole solutions within the framework of (Formula presented) f(Q,T) gravity by incorporating conformal symmetry and employing a Lorentzian distribution to model the matter sources. The study considers different equations of state, such as traceless and barotropic forms, to explore their impact on the viability of wormhole solutions. A comprehensive analysis of the effects of the model parameters on the wormhole geometry and its physical properties is carried out. The findings reveal that the resulting shape function satisfies all the necessary wormhole conditions. Importantly, certain scenarios are identified where the wormhole can be supported by non-exotic matter, highlighting the physical plausibility of such solutions within modified gravity.  2026 IOP Publishing Ltd. All rights, including for text and data mining, AI training, and similar technologies, are reserved. This article is available under the terms of the https://publishingsupport.iopscience.iop.org/iop-standard/v1.</text>
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              <text>barotropic fluid; conformal symmetry; energy conditions; lorentzian distribution; non-commutative geometry; traceless fluid; traversable wormhole</text>
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              <text>Institute of Physics</text>
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              <text>ISSN: 318949; CODEN: PHSTB</text>
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              <text>Restricted Access; Hardcopy may be available in the library</text>
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