Thin accretion disks around multi-polytropic wormhole

Thin accretion disks around multi-polytropic wormhole

Blog Article

In this paper, we study the physical properties of thin accretion disks in static and spherically symmetric multi-polytropic wormhole space-time.Using the Novikov-Thorne model, the electromagnetic flux, temperature distribution, innermost stable circular orbits and radiative efficiency of thin mpu63zm/a disks are obtained.Comparing the results with traversable weboost splitter wormholes obtained by Morris and Thorne (TWH) and the Schwarzschild solution, we show that thin accretion disks around multi-polytropic wormhole geometry are more luminous and more efficient than the TWH and Schwarzschild black hole.