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Calculate the lifetime (in seconds) for each of the four n = 2 states of hydrogen. Hint: You’ll need to evaluate matrix elements of the form <ψ100xψ200>,<ψ100yψ211>, and so on. Remember that role="math" localid="1658303993600" x=rsinθcosϕ,y=rsinθsinϕandz=rcosθ. Most of these integrals are zero, so inspect them closely before you start calculating. Answer: 1.60×10-9seconds for all except role="math" localid="1658304185040" ψ200, which is infinite.

Short Answer

Expert verified

The life time for each of the four n=2 states of hydrogen isτ=1A=1.60×10-9s

Step by step solution

01

Step 1: states of hydrogen

At standard conditions of hydrogen is a gas of diatomic molecules having the formula H2. It is colourless, tasteless, nontoxic, and highly combustible. Hydrogen is the most abundant chemical substance in the universe, constituting roughly 75% of all normal matter

02

Step 2: Calculating the life time for each of the four n=2 states of hydrogen

In Problem 9.1 we calculated the matrix elements of z; all of them are zero except 100z210=28352a.

As for x and y, we noted that

100>,200and210>areeven(inx,y),whereas21+1>is odd. So the only non-zero matrix elements are 100x21+1and100y21+1 Using the wave functions in Problem 9.1:

100x21+1=1πa3+18πa1ae-r/are-r/2asinθe+iϕrsinθcosϕr2sinθdrdθdϕ=+18πa40r4e-3r/2adr0πsin3θdθ02πcosϕ+isinϕcosϕdϕ=+18πa44!2a3543π=+2735a

100y21+1=+18πa44!2a354302πcosϕ+isinϕsinϕdϕ=+18πa44!2a3543+iπ=-i2735a100r200=0;100r21027235ak^;100r21+1=2735a+i^-ij^,and21+1>100>)

Meanwhile, ω=E2-E1ħ=1ħE14-E1=-3E14ħ so for the three l = 1 states:

A=-33E1326ħ3ea221531013πo˙0ħc3=-2938πE13e2a2o˙0ħ4c3=21038E1mc22ca=2103813.60.511×1063.00×1080.529×10-10m=6.27×108/s;τ=1A=1.60×10-9s

Thus life time for each of the four n=2 states of hydrogen is τ=1A=1.60×10-9s

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Most popular questions from this chapter

As a mechanism for downward transitions, spontaneous emission competes with thermally stimulated emission (stimulated emission for which blackbody radiation is the source). Show that at room temperature (T = 300 K) thermal stimulation dominates for frequencies well below 5×1012Hz , whereas spontaneous emission dominates for frequencies well above . Which mechanism dominates for visible light?

Suppose you don’t assume Haa=Hbb=0

(a) Find ca(t)and cb(t) in first-order perturbation theory, for the case

.show that , to first order in .

(b) There is a nicer way to handle this problem. Let

.

Show that

where

So the equations for are identical in structure to Equation 11.17 (with an extra

(c) Use the method in part (b) to obtain in first-order
perturbation theory, and compare your answer to (a). Comment on any discrepancies.

Calculate ca(t)andcb(t), to second order, for a time-independent perturbation in Problem 9.2. Compare your answer with the exact result.

You could derive the spontaneous emission rate (Equation 11.63) without the detour through Einstein’s A and B coefficients if you knew the ground state energy density of the electromagnetic field P0(ω)for then it would simply be a case of stimulated emission (Equation 11.54). To do this honestly would require quantum electrodynamics, but if you are prepared to believe that the ground state consists of one photon in each classical mode, then the derivation is very simple:

(a) Replace Equation 5.111by localid="1658381580036" N0=dkand deduce P0(ω) (Presumably this formula breaks down at high frequency, else the total "vacuum energy" would be infinite ... but that's a story for a different day.)

(b) Use your result, together with Equation 9.47, to obtain the spontaneous emission rate. Compare Equation 9.56.

Suppose you don’t assumeH'aa=H'aa=0

(a) Findca(t)andcb(t)in first-order perturbation theory, for the case

ce(0)=1,cb(0)=0.show that |ca(1)(t)|2+|cb(1)(t)|2=1, to first order inH^' .

(b) There is a nicer way to handle this problem. Let

daeih0tHaac(tc)dtc0ca,dbei20tHbbc(tc)dtc0cb.

Show that

role="math" localid="1658561855290" d-a=-iheiϕH'abe-iω0tdb;db-=-iheiϕH'bae-iω0tda

where

ϕ(t)1h0l[H'aa(t')-H'bb(t')]dt'.

So the equations fordaanddbare identical in structure to Equation 11.17 (with an extra role="math" localid="1658562498216" eiϕtackedontoH^')

ca-=-ihH'abe-iω0tcb,cb-=-ihH'baeiω0tca

(c) Use the method in part (b) to obtainrole="math" localid="1658562468835" ca(t)andcb(t)in first-order
perturbation theory, and compare your answer to (a). Comment on any discrepancies.

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