L5 - rate eqns Flashcards

1
Q

whata approx when soft collisions dominate

A

adiabatic or wuasi static approx

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2
Q

For large beta what happenes

A

Any oscillations of the atomic probabilitya re well damped

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3
Q

population rate eqns

A

drho11/dt and same for 22

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4
Q

R12 meaning

A

R12 = R21
avsorption and stimulated emission rate

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5
Q

info on R12 params and shape

A

Lorentzian profile proportinal to |E0|^2 so proportioanl to I of light
If Detuning less the R21 More

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6
Q

R12 definition

A

Sigma Phi
Sigma depend on v ( freq of incident excitation light)

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7
Q

Sigma

A

Absorption cross section
Sig dep on detuning

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8
Q

Phi

A

Photon flux
Associatied with the light field E0
units: Photons per (area time)
Proportional to light intensity (I is macroscopic measuremnet)

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9
Q

Energy of a photon

A

E = h v(n)

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10
Q

Density of atoms in a state

A

N1 = N rho11
N2 = N rho22
these are the density of atoms ina given level

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11
Q

Gamma meaning

A

Inelastic collision energy transition probability

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12
Q

Compare inelastic collisions vs spontatnoues emission

A

Gamma_12, Gamma_21 &laquo_space;A21
inelatic have little influence comapred to spont emission
so N1 + N2 = NT tends to remain constnat

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13
Q

Steady state we cna assume

A

Constant photon flux Phi

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14
Q

N2 population
case: NO flux

A

Phi = 0
N2 = N2(0) exp(-A21 t)
All atoms end up in GS
spont emission dominates ( inelastic collision Gamma not really large enough)
No stimulated processes (due to sigma Phi) i.e. R12,R21

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15
Q

N2 population:
Case: Low flux
Weak excitiation

A

R21 = sigma Phi != 0 but R21 &laquo_space;A21
So more e- lost from N2 due to spont emission than is brought up by the stimulated absorption

if N2(0) then
N2(t) = constant [1 - exp(-A21t)]
same decaying exp reaches max 1 (t = 0)= > N2 = 0 initially
when t large exp -> and N2 is at a max => SATURATION

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16
Q

N2 population:
Case: Low flux behavrious in graph

A

Initally asymptotic approach (concave down)

17
Q

N2 population:
Case: High flux
Strong excitiation

A

R21 = sigma Phi&raquo_space;A21
stimulated rate&raquo_space; spont emission rate
N2 (t) -> N/2 —– SATURATION

18
Q

Why high flux not good enough

A

N - > N/2 saturation
Require population inversion for gain not population equalisation

19
Q

N2 population:
Case: High flux - Power broadening
Strong excitiation

A

Assume statead state and exp factor&raquo_space;1
N2(t=infty)/N = lorentzian profile
profile widens with larger X ( larger E0)

So N2(infty)/N becomes broader and taller as E0 flux increases