Wormhole Geometries Supported by Strange Quark Matter and Phantom-like Generalized Chaplygin gas within $f(Q)$ Gravity

Abstract

A crucial aspect of wormhole (WH) physics is the inclusion of exotic matter, which requires violating the null energy condition. Here, we explore the potential for WHs to be sustained by quark matter under conditions of extreme density along with the phantom-like generalized cosmic Chaplygin gas (GCCG) in symmetric teleparallel gravity. Theoretical and experimental studies on baryon structures indicate that strange quark matter, composed of u (up), d (down), and s (strange) quarks, represents the most energy-efficient form of baryonic matter. Drawing from these theoretical insights, we use the Massachusetts Institute of Technology (MIT) bag model equation of state to characterize ordinary quark matter. By formulating specific configurations for the bag parameter, we develop several WH models corresponding to different shape functions for the isotropic and anisotropic cases. Our analysis strongly suggests that an isotropic WH is not theoretically possible. Furthermore, we investigate traversable WH solutions utilizing a phantom-like GCCG, examining their feasibility. This equation of state, capable of violating the null energy condition, can elucidate late-time cosmic acceleration through various beneficial parameters. In this framework, we derive WH solutions for both constant and variable redshift functions. We have employed the volume integral quantifier (VIQ) method for both studies to assess the quantity of exotic matter. Furthermore, we have done the equilibrium analysis through the Tolman-Oppenheimer-Volkoff (TOV) equation, which supports the viability of our constructed WH model.

Physics of the Dark Universe published version

References in corpus (60)

• f(R) theories
• Extended Theories of Gravity
• Disappearing cosmological constant in f(R) gravity
• Coincident General Relativity
• Class of viable modified $f(R)$ gravities describing inflation and the onset of accelerated expansion
• Cosmology in $f(Q)$ geometry
• Wormholes supported by a phantom energy
• $f(Q,T)$ gravity
• Coupling matter in modified $Q$-gravity
• Teleparallel Theories of Gravity: Illuminating a Fully Invariant Approach
• Wormholes in Dilatonic Einstein-Gauss-Bonnet Theory
• Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models
• Testing $F(Q)$ gravity with redshift space distortions
• Fate of the first traversible wormhole: black-hole collapse or inflationary expansion
• Possible existence of wormholes in the galactic halo region
• Chaplygin traversable wormholes
• Black holes in $f(\mathbb{Q})$ Gravity
• Quark Matter in Strong Magnetic Field
• Wormhole solutions in symmetric teleparallel gravity
• Wormhole geometries in $f(Q)$ gravity and the energy conditions
• Lagrange formulation of the symmetric teleparallel gravity
• Traversable wormhole geometries in $f(Q)$ gravity
• Wormholes in viable $f(R)$ modified theories of gravity and Weak Energy Condition
• Thermodynamics, strange quark matter, and strange stars
• New asymptotically flat phantom wormhole solutions
• On wormhole formation in $f(\text{R},\text{T})$ gravity: varying Chaplygin gas and barotropic fluid
• Wormholes supported by polytropic phantom energy
• Evolving wormhole geometries
• The spectrum of symmetric teleparallel gravity
• Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of $f(Q)$ Gravity
• Maximum mass of neutron stars with a quark core
• Wormhole inspired by non-commutative geometry
• Casimir Wormholes in Modified Symmetric Teleparallel Gravity
• Tolman-Oppenheimer-Volkoff equations in presence of the Chaplygin gas: stars and wormhole-like solutions
• Viable Singularity-Free f(R) Gravity Without a Cosmological Constant
• Traversable Wormhole Solutions in $f(R)$ Gravity Via Karmarkar Condition
• Wormhole solutions in $f(R,L_m)$ gravity
• Constraining values of bag constant for strange star candidates
• Investigation of Traversable Wormhole Solutions in Modified $f(R)$ Gravity with Scalar Potential
• Quasinormal Modes of Black holes in $f(Q)$ gravity
• Seeking exactly solvable models of traversable wormholes supported by phantom energy
• Existence of Wormhole Solutions in $f(Q,T)$ Gravity under Non-commutative Geometries
• Composite vacuum Brans-Dicke wormholes
• GUP Corrected Casimir Wormholes in $f(Q)$ Gravity
• Dark energy, wormholes, and the Big Rip
• Coincident f(Q) gravity: black holes, regular black holes and black bounces
• Density Dependence of Nucleon Bag Constant, Radius and Mass in an Effective Field Theory Model of QCD
• Coincident gauge for static spherical field configurations in symmetric teleparallel gravity
• Buchdahl quark stars within $f(Q)$ theory
• Evolving topologically deformed wormholes supported in the dark matter halo
• Static spherically symmetric wormholes with isotropic pressure
• Wormhole solutions in $f(Q,T)$ gravity with a radial dependent B parameter
• Geometrically deformed charged anisotropic models in $f(Q,T)$ gravity
• Modified Chaplygin Traversable Wormholes
• Study of charged gravastar model in $f(\mathcal{Q})$ gravity
• Wormhole on the Brane with Ordinary Matter: The Broader View
• Chiral symmetry and strangeness content in nuclear physics parametrized by a medium dependent bag constant
• A Comprehensive Study of Massive Compact Star Admitting Conformal Motion Under Bardeen Geometry
• Does violation of Cosmic No-hair Conjecture guarantee the existence of Wormhole?
• Validity of energy conditions of matter in traversable wormholes under the $f(Q)$ modified gravity theory

Cited by in corpus (2)

• Influence of GUP corrected Casimir energy on zero tidal force wormholes in modified teleparallel gravity with matter coupling
• Strange Quark Stars and Condensate Dark Stars in Bumblebee Gravity