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Stimulated Emission of Radiation<br />

- stimulated emission is referring to the emission of radiation (a photon) from one quantum<br />

system at its transition frequency induced by the presence of other photons at that frequency<br />

- introduced by Einstein in 1917 to derive Planck's blackbody radiation law<br />

- is the basis for the operation of a LASER (Light Amplification by Stimulated Emission of<br />

Radiation)<br />

Consider an assembly of N atoms with energy levels E i and E j in<br />

thermal equilibrium with a thermal radiation field with energy<br />

density u(ν) at temperature T<br />

- the transition frequency ν ij in the individual atom is<br />

- the probability of an atom in state i to absorb a photon is<br />

proportional to u(ν ij ) (related to the number of photons at that<br />

frequency) and to the probability B ij (Einstein B coefficient) of<br />

the atom to absorb a photon at that frequency<br />

<strong>phys4.15</strong> <strong>Page</strong> 1<br />

- thus, the total number of atoms per second that absorb a photon is<br />

where N i is the number of atoms in state i<br />

- an atom in state j has a probability A ji (Einstein A coefficient) to<br />

spontaneously decay into state i by emitting a photon at frequency ν in a<br />

process called spontaneous emission<br />

- also, an atom in state j has a probability B ji to decay into state i by<br />

emitting a photon at frequency ν ij stimulated by the presence of other<br />

photons at that frequency the number of which is proportional to u(ν ij )<br />

- this process is called stimulated emission<br />

- thus the total number N ji of atoms per second that make a transition into<br />

the lower state is given by<br />

- in thermal equilibrium the number of atoms that make a transition to lower energy<br />

must be identical to the number of atoms making a transition to higher energy<br />

<strong>phys4.15</strong> <strong>Page</strong> 2


Transitions in a collection of atoms<br />

interacting with a radiation field<br />

- in thermal equilibrium<br />

- solve for the energy density of the radiation field u(ν)<br />

- with the number of atoms in the ground N i or excited state N j is given by classical M.-B.<br />

statistics<br />

- thus<br />

<strong>phys4.15</strong> <strong>Page</strong> 3<br />

- hence the energy density of a radiation field in thermal equilibrium is given by<br />

- this is Planck's formula for blackbody radiation for<br />

- for identical upwards and downwards transition rates<br />

- and with the ratio of spontaneous emission to<br />

induced emission rate given by<br />

note:<br />

- stimulated emission does occur and is consistent with the form of the<br />

blackbody spectrum<br />

- the probability for stimulated absorption is equal to the probability<br />

stimulated emission<br />

- the likelihood of spontaneous emission relative to stimulated emission<br />

increases rapidly with frequency<br />

- knowing one of the parameters A ji , B ji , B ij we can determine the other<br />

ones<br />

- spontaneous emission is 'stimulated' by vacuum fluctuations (QED)<br />

<strong>phys4.15</strong> <strong>Page</strong> 4


Light Amplification by Stimulated Emission of Radiation (LASER)<br />

LASER<br />

Light Amplification by Stimulated Emission of Radiation<br />

properties:<br />

• monochromatic<br />

• coherent<br />

• directed<br />

• bright<br />

<strong>phys4.15</strong> <strong>Page</strong> 5<br />

Properties of LASER light<br />

monochromatic<br />

- relative line width<br />

coherence<br />

- temporal coherence<br />

- spatial coherence limited only by optics<br />

brightness<br />

- intensities<br />

- large photon flux<br />

in pulsed operation<br />

- short pulses<br />

<strong>phys4.15</strong> <strong>Page</strong> 6


The LASER<br />

1. active LASER medium (gas, dye, solid)<br />

2. pumping (light, electrical energy)<br />

3. 100% reflecting mirror<br />

4. coupling mirror (< 1% transmission)<br />

5. LASER beam<br />

<strong>phys4.15</strong> <strong>Page</strong> 7<br />

The LASER Principle<br />

- generation of a large number of excitations in a medium<br />

by (stimulated) absorption<br />

- a long lived metastable state to achieve population inversion<br />

- stimulated emission of radiation<br />

- storage of radiation field in a resonant cavity with<br />

partially transmitting mirror<br />

<strong>phys4.15</strong> <strong>Page</strong> 8


Generation of Population Inversion<br />

- excitation by optical pumping in a three level system<br />

- transition (possibly non-radiative) to a metastable state<br />

- stimulated emission<br />

- at least a three level system is required to achieve<br />

population inversion as the symmetry between the<br />

probability for absorption (B ij ) and emission (B ji ) results<br />

at best in equal population of the two states such that<br />

emission cannot be the dominant process (i.e. there would<br />

be no amplification in number of photons)<br />

<strong>phys4.15</strong> <strong>Page</strong> 9<br />

Examples of Lasers<br />

Ruby Laser: Cr + ions in Al 2 O 3 crystal (sapphire)<br />

- optical pumping using flash light<br />

- Helium-Neon Laser: gas mixture (90 % He, 10 % Ne) where He is excited electrically in gas<br />

discharge and energy is transferred in collision to Ne<br />

<strong>phys4.15</strong> <strong>Page</strong> 10


Nobel Prize in Physics 1964<br />

for fundamental work in the field of quantum electronics,<br />

which has led to the construction of oscillators and<br />

amplifiers based on the maser-laser principle<br />

Charles H. Townes Nicolay G. Basov Aleksandr M. Prokhorov<br />

<strong>phys4.15</strong> <strong>Page</strong> 11<br />

Laser-Pointer<br />

• housing<br />

• electronics<br />

• LASER<br />

and optics<br />

<strong>phys4.15</strong> <strong>Page</strong> 12


CD Player<br />

• compact disc<br />

• the mechanism<br />

• portable CD player<br />

(older modell)<br />

<strong>phys4.15</strong> <strong>Page</strong> 13<br />

Laser-Printer<br />

• resolution up to 20 µm or 50 points per mm (= 1270 dpi)<br />

• colors with multiple stages<br />

<strong>phys4.15</strong> <strong>Page</strong> 14


Material Processing<br />

• CO 2 gas LASER<br />

• up to 20 kW power<br />

www.trumpf.com<br />

<strong>phys4.15</strong> <strong>Page</strong> 15<br />

Lasers in Medicine<br />

• eye surgery<br />

• dermatology etc.<br />

<strong>phys4.15</strong> <strong>Page</strong> 16


Specific Heat of Solids<br />

- dependence of thermal energy stored in a solid on temperature<br />

- molar specific heat at constant volume c V : energy that needs to be added to 1 mol of a solid<br />

to increase its temperature by 1 Kelvin<br />

- thermal energy is stored in solids in the vibrations of its constituents (atoms, ions or<br />

molecules)<br />

- in a simple model the atoms can vibrate along 3 independent (x, y, z) directions that each<br />

can be considered as an independent harmonic oscillator<br />

- the equipartition theorem tells us the average energy stored in each degree of freedom, thus<br />

the total energy of a solid containing 1 mol = N 0 = 6.022 10 23 of atoms is given by<br />

- R = 8.31 J/mol is the ideal gas constant (pV = nRT)<br />

- specific heat (Dulong Petit law)<br />

<strong>phys4.15</strong> <strong>Page</strong> 17<br />

Dulong petit law fails for light elements (e.g.<br />

carbon) and at low temperatures, see plot<br />

- problem can be solved using the Bose-Einstein<br />

distribution function for the probability of an<br />

harmonic oscillator to have energy hν<br />

- average energy for a harmonic oscillator of frequency ν<br />

- total energy per mol<br />

- thus Einstein's specific heat formula is<br />

<strong>phys4.15</strong> <strong>Page</strong> 18


- the high temperature limit of Einstein's formula<br />

- therefore<br />

- at high temperatures the thermal energy is much larger than the typical level separation of<br />

the harmonic oscillators in the solid and the specific heat is close to the classical prediction<br />

- at low temperatures the thermal energy is comparable to the level separation and quantum<br />

statistics start to play a role<br />

- for lighter elements with smaller masses the oscillator frequencies are higher and thus<br />

quantum effects are more important even at higher temperatures<br />

- the zero point motion does not play a role for the specific heat as it is only a constant offset<br />

in energy<br />

<strong>phys4.15</strong> <strong>Page</strong> 19<br />

Debeye theory<br />

- Debeye regarded a solid as a continuous elastic medium with elastic standing waves<br />

instead of considering the atoms as individual oscillators the way Einstein did<br />

- these standing waves can have frequencies ν up to a maximum value ν max<br />

- they are like transverse and longitudinal elastic waves that propagate at the speed of<br />

sound in the solid<br />

- their energies are quantized as in a harmonic oscillator<br />

- each quantum of the elastic wave is called a phonon<br />

- Debeye assumed that 3N different modes exist per mol in a solid<br />

- the resulting formula describes the specific heat of the solid better than Einstein's<br />

formula<br />

- to be discussed in detail in solid state physiscs<br />

<strong>phys4.15</strong> <strong>Page</strong> 20

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