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Calculate the 鈥渟eries limit鈥 of the Lyman series of spectral lines. This is defined as the shortest wavelength possible of a photon emitted in a transition from a higher initial energy level to the ni=1 final level. (Note: In figure 7.5, the spectral lines of the series 鈥渃rowd together鈥 at the short-wavelength end of the series).

Short Answer

Expert verified

The shortest wavelength possible in the Lyman series is 91.2 nm.

Step by step solution

01

Identification of the shortest wavelength

Photon energy is the energy carried by a single photon. The amount of energy is directly proportional to the photon's electromagnetic frequency and thus, is inversely proportional to the wavelength.

The energy of the emitted photon is,

E=hc 鈥.. (1)

Where, h is Plank鈥檚 constant, c is the speed of light, and role="math" localid="1659178129240" is the wavelength of the photon.

The Planck鈥檚 constant, h=1240eVnm

From eq. (1) you get that energy is high if the wavelength is low.

Hence, shortest wavelength will be because of the highest energy possible in the Lyman series, i.e. n=n=1,

Where, n is the principal quantum number.

02

Calculation of shortest wavelength:

As you know that energy of a state is

En=-13.6eVn2(n=12,3,)

Where, n is the principal quantum number.

Hence, Energy corresponding to n=n=1will be given by,

E=E-E1=-13.6eV2+13.6eV12=0+13.6eV1

E=1.36eV 鈥.. (2)

Now, substitute 1240eVnmfor localid="1659179281565" hand E=1.36eVfor E into equation (1).

1.36eV=1240eVnm=91.2nm

Hence, required shortest wavelength of the Lyman series is 91.2 nm.

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Most popular questions from this chapter

Classically, an orbiting charged particle radiates electromagnetic energy, and for an electron in atomic dimensions, it would lead to collapse in considerably less than the wink of an eye.

(a) By equating the centripetal and Coulomb forces, show that for a classical charge -e of mass m held in a circular orbit by its attraction to a fixed charge +e, the following relationship holds

=er-3/240m.

(b) Electromagnetism tells us that a charge whose acceleration is a radiates power P=e2a2/60c3. Show that this can also be expressed in terms of the orbit radius as P=e696203m2c3r4. Then calculate the energy lost per orbit in terms of r by multiplying the power by the period T=2/and using the formula from part (a) to eliminate .

(c) In such a classical orbit, the total mechanical energy is half the potential energy, or Eorbit=-e280r. Calculate the change in energy per change in r : dEorbit/dr. From this and the energy lost per obit from part (b), determine the change in per orbit and evaluate it for a typical orbit radius of 10-10m. Would the electron's radius change much in a single orbit?

(d) Argue that dividing dEorbit/dr by P and multiplying by dr gives the time required to change r by dr . Then, sum these times for all radii from rinitial to a final radius of 0. Evaluate your result for rinitial=10-10m. (One limitation of this estimate is that the electron would eventually be moving relativistically).

Question: Consider a cubic 3D infinite well of side length of L. There are 15 identical particles of mass m in the well, but for whatever reason, no more than two particles can have the same wave function. (a) What is the lowest possible total energy? (b) In this minimum total energy state, at what point(s) would the highest energy particle most likely be found? (Knowing no more than its energy, the highest energy particle might be in any of multiple wave functions open to it and with equal probability.)

For the more circular orbits, =n-1and

P(r)r2ne-2r/na0

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b) Show that the expectation value of the radius is given by

r=n(n+12)a0

and the uncertainty by

r=na0n2+14

c) What happens to the ratior/rin the limit of large n? Is this large-n limit what would be expected classically?

To conserve momentum, an atom emitting a photon must recoil, meaning that not all of the energy made available in the downward jump goes to the photon. (a) Find a hydrogen atom's recoil energy when it emits a photon in a n = 2 to n = 1 transition. (Note: The calculation is easiest to carry out if it is assumed that the photon carries essentially all the transition energy, which thus determines its momentum. The result justifies the assumption.) (b) What fraction of the transition energy is the recoil energy?

Knowing precisely all components of a nonzero Lwould violate the uncertainty principle, but knowingthat Lis precisely zerodoes not. Why not?

(Hint:For l=0 states, the momentum vector p is radial.)

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