## Sunqm-3: Solving Schrodinger Equation for Solar Quantum Mechanics {N,n} Structure

**Authors:** Yi Cao

In this paper, Schrodinger equation is established for the non-spin Solar QM {N,n} structure model. Solving the Schrodinger equation gives the orbit energy En = -3.81E+11 *(m / n^2), where m is the orbital moving object's mass (in kg), and n is the total n of the orbit using Sun core {0,1} as r1. Combining r^2*|R(nl)|^2 to the deduced Sun's interior mass density formula D = 1.26E+23 / r^2.33, a plot of {N,n} QM calculated (that is close to the true) mass density vs. r (within Sun ball {0,2}) has been made.

**Comments:** 14 Pages.

**Download:** **PDF**

### Submission history

[v1] 2018-05-06 12:43:33

**Unique-IP document downloads:** 54 times

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