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Introduction to Atomic and Quantum Physics - Sommerfeld Theory

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Page 1: Introduction to Atomic and Quantum Physics - Sommerfeld Theory

Lectures:

Chapter 1

Chapter 2

Chapter 3

Chapter 4

Chapter 5

Chapter 6

Chapter 7

Chapter 8

Chapter 9

Chapter 10

Chapter 11

Chapter 12

V. Theory of Sommerfeld

V.1. RULES quantization WILSON - Sommerfeld

Wilson quantization rules - Sommerfeld relate to any physical quantity, which is a periodic function of time(when describing a system functions are functions that the system is periodycznymi kwantowalny).

where & tau - period

p q - momentum corresponding to the generalized coordinate q

n q - the number of quantum

Example: The point of mass m moving in a circular orbit.

(R, & phi) q 1 = r, q 2 = & phi

r = const & phi = & omega t

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(V.1.1)

Page 2: Introduction to Atomic and Quantum Physics - Sommerfeld Theory

Since L = P, then:, Namely:

Dependence (V.1.4) compatible (identical) to the second postulate of Bohr . It is the mathematicalsolution.

If (V.1.1) is applied to an oscillating particle of mass m, we can find the total energy:

Equation (V.1.5) is consistent with the fourth postulate of Bohr .

Sommerfeld generalized Bohr model and showed that the electron in the orbit can move the elliptical orbit (thewheel is a special case), the number of orbits depends on n is exactly equal to it. n - we'll call the main quantum number.

V.2. The fine structure of the hydrogen spectrum.

All spectral lines ranging from n = 2 are split - it's fine structure. subtle structure is explained on the basis of relativistic account.

(V.1.2)

(V.1.3)

(V.1.4)

(V.1.5)

Page 3: Introduction to Atomic and Quantum Physics - Sommerfeld Theory

12/9/12 Introduction to atomic and quantum physics - Sommerfeld Theory

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Rys.V.1. The fine structure of the hydrogen atom spectrum.

Sommerfeld was able to calculate the parameters of the orbits and their energies.

, N & phi = 1, 2, 3, ...

, N r = 0, 1, 2, ...

Equations (V.2.3), (V.2.3b), (V.2.3c) - define the orbit at which the electron moves.

- The main quantum number

- Azimuthal quantum number

- Define the shape of the orbit

V.3. EXAMPLES OF ORBIT Sommerfeld.

Rys.V.2. Examples Sommerfeld orbits.

In terms of energy all the orbits for the n are the same as the energy does not depend on n & phi - orbital

degeneracy. degeneration was abolished after the introduction of relativistic account.

(V.2.1)

(V.2.2)

(V.2.3)

(V.2.3b)

(V.2.3c)

Page 4: Introduction to Atomic and Quantum Physics - Sommerfeld Theory

12/9/12 Introduction to atomic and quantum physics - Sommerfeld Theory

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Energy - is characteristic of the orbit

Z (V.3.2) that explains the structure and spectral lines subtle effect After taking into

account the relativistic energy is given by:

where: E NR - part nonrelativistic (V.2.3c)

E R - Amendment relativistic

Amendment describes the shift of energy levels - the appearance of fine structure.

and - the fine structure constant, the characteristic size of the formulas of quantum physics There are many interpretations of the constant a, one of which is:

v 1 is the electron velocity on the first orbit

As a result, the existence of the fine structure appear more levels and creates a more complicated spectrum.

(V.3.1)

(V.3.2)

(V.3.3)

(V.3.4)

(V.3.5)

Page 5: Introduction to Atomic and Quantum Physics - Sommerfeld Theory

Rys.V.3. Allowed transitions are indicated by green arrows, red means go prohibited.

The fact that transitions are allowed and which are not, says the selection rule:

(V.3.6)