A Finding a suitable form factor for a given set of conditions

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I want to plot Hawking temperature as a function of z(inverse of horizon radius), which requires making use of a form factor A(z). I want to make an ansatz for form factor such that I get the desired plots.
This is basically a physics problem but I will try my best to highlight the mathematics behind it.
Suppose I have two functions:

$$T(z,B)=\frac{\text{z}^3 e^{-3 A(\text{z})-B^2 \text{z}^2}}{4 \pi \int_0^{\text{z}} \xi ^3 e^{-3 A(\xi )-B^2 \xi ^2} \, d\xi },$$
$$\phi(z,B)=\int_0^z \sqrt{-\frac{2 \left(3 x A''(x)-3 x A'(x)^2+6 A'(x)+2 B^4 x^3+2 B^2 x\right)}{x}} \, dx$$ where z \in \mathbb{R^+} and B \in [0,1]

and I want to find a function A(z), which is known as the form factor in literature, such that the plot of the function T(z,B) v/s z has one local minimum along with the condition that T(z,B)\rightarrow\infty when z\rightarrow0, also \phi(z) is real-valued. When I take the ansatz A(z)=-a z^2, I am able to satisfy the above condition for B\in[0,0.6] and get plots like:
now.jpg


Now for a different model, I need to use such an ansatz for A(z) such that I may be able to satisfy the real valued-ness of \phi(z) and get a local minimum as well as a maximum for the plot of T(z,B) v/s z with the condition that T(z,B)\rightarrow\infty when z\rightarrow0 and T(z,B)\rightarrow0 when z\rightarrow\infty to get plots like these:
wanted.jpg


If possible I want to keep B\in[0,1]. The constant a has to be used in the form factor somehow, whose value is 0.15. The form factor can also be written in terms of A(z,B). Is there a way to use Mathematical analysis to come up with such a form factor? Any help in this regard would be truly beneficial!
 
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The way you formulated the problem better fits to a mathematical subforum.
 
Jacobson’s work (1995) [1] demonstrated that Einstein’s equations can be derived from thermodynamic principles, suggesting gravity might emerge from the thermodynamic behavior of spacetime, tied to the entropy of horizons. Other researchers, such as Bekenstein [2] and Verlinde [3], have explored similar ideas, linking gravity to entropy and holographic principles. I’m interested in discussing how these thermodynamic approaches might apply to quantum gravity, particularly at the Planck...

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