## 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:** 37 times

Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary.
In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution.
Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.

**Add your own feedback and questions here:**

*You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.*

*
*