\begin{document}$f(R,L_{m},T)$\end{document} gravity. The quark matter inside these stars is modeled as de-confined quarks and described by a color-flavor-locked equation of state. Using this equation of state, we numerically solve the modified Tolman-Oppenheimer-Volkoff (TOV) equation to obtain the mass and radius of quark stars. We analyze key properties of the quark star such as dynamical stability, compactness, and gravitational redshift. The results show that the modified gravitational theory has a significant impact on the properties of quark stars and is consistent with the observational data of massive pulsars."> Study of color-flavor locked quark stars in <inline-formula><tex-math id="M1">\begin{document}${\boldsymbol f(R,L_{m},T)}$\end{document}</tex-math></inline-formula> gravity using observational data -
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