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On the Thermodynamical Black Hole Stability in the Space Time of a Global Monopole in f(R) Gravity

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Academic year: 2020

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Figure

Figure 1. Graphs for B(r, n) in function of position for each n-orders going from 1 to 4, where GM =  and 1κη2=0.3 10×−5
Figure 2. Graph for S r()H for n going from 2 to 4 and Schwarzschild black hole with global monopole, κη2=0.3 10×−5where in left panel ψ0.4 102nn=×− and in the right panel ψ0.4 102nn= −×−
Figure 4. Graph for the Hawkings temperature, T in function of the horizn radio rH , with κη2=0.3 10×−5 and n going from 2 to 4, with Schwarzschild black hole with global monopole ψ0.4 102nn= −×−
Figure 5. Graph for heat capacity, C, with κη2=0.3 10×−5 with ψ0.4 102nn= −×− and panel right
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