Wormholes supported by phantom-like modified Chaplygin gas
Mubasher Jamil, M. Umar Farooq, Muneer Ahmad Rashid

TL;DR
This paper explores the theoretical construction of wormholes supported by phantom energy modeled as modified Chaplygin gas, satisfying key physical conditions but requiring null energy condition violation.
Contribution
It presents new solutions for wormholes supported by phantom-like modified Chaplygin gas, satisfying flare-out and asymptotic flatness conditions.
Findings
Wormhole solutions satisfy flare-out and asymptotic flatness.
Null energy condition must be violated for wormhole stability.
Supports the feasibility of phantom energy in wormhole physics.
Abstract
We have examined the possible construction of a stationary, spherically symmetric and spatially inhomogeneous wormhole spacetime supported by the phantom energy. The later is supposed to be represented by the modified Chaplygin gas equation of state. The solutions so obtained satisfy the flare out and the asymptotic flatness conditions. It is also shown that the averaged null energy condition has to be violated for the existence of the wormhole.
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