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In this paper, we discuss the thermodynamic properties of the evolving Lorentzian wormhole.
- For the shape function $b(r) = r_{0}^2/r$, it is shown that the wormhole spacetime admits two apparent horizons, the inner and the outer one.
- The inner horizon expands while the outer contracts with the passage of time.
- Corresponding to these horizons, we have three types of wormholes, regular, extreme and the naked wormholes.
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