How to arrive at Bessel function solution to 1D polynomial potential

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To derive the Bessel function solution for the 1D polynomial potential described by the differential equation u'' + c x^n u = 0, a change of variables is necessary. By substituting x^(n/2) = t, the equation can be transformed into a standard Bessel differential form. This involves expressing the original function u in terms of u(t) and adjusting the derivatives accordingly. The resulting solution can be expressed in terms of Bessel functions, specifically J_{\pm m}(\eta), where m is defined as 1/(n + 2) and η is the integral of k(x). Understanding these transformations is crucial for applying the Bohr-Sommerfeld quantization condition effectively.
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My quantum text, leading up to the connection formulas for WKB and the Bohr-Sommerfeld quantization condition states that for

\begin{align}u'' + c x^n u = 0 \end{align}

one finds that one solution is

\begin{align}u &= A \sqrt{\eta k} J_{\pm m}(\eta) \\ m &= \frac{1}{{n + 2}} \\ k^2 &= c x^n \\ \eta &= \int_0^x dx' k(x')\end{align}

I'd like to know how this was arrived at. Could somebody outline what set of change of variables would one make to put the differential equation above into the standard Bessel differential form?
 
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Try first a change of variables xn/2 = t. Compute the ODE in terms of u(t) then.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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