EBK PHYSICAL CHEMISTRY
EBK PHYSICAL CHEMISTRY
2nd Edition
ISBN: 8220100477560
Author: Ball
Publisher: Cengage Learning US
Question
Book Icon
Chapter 16, Problem 16.8E
Interpretation Introduction

(a)

Interpretation:

The values of ΔE in the transition energies for each individual transition for the 1S1P transition when a sample is exposed to a magnetic field of 2.35 T are to be calculated.

Concept introduction:

The phenomenon of splitting of a spectral line when a magnetic field is applied to it is known as Zeeman Effect. Magnetic field strength can be measured by using the Zeeman Effect. Applications of Zeeman Effect include NMR spectroscopy, MRI and electron spin resonance spectroscopy.

During an electronic transition, an electron from ground state moves straight to the excited state keeping the internuclear distance constant.

The change in the energy of the state, ΔE is calculated by the formula shown below.

ΔE=μBMLB

Expert Solution
Check Mark

Answer to Problem 16.8E

The values of ΔE in the transition energies for 1P in the 1S1P transition are 2.18×1023 J, 0 J and +2.18×1023 J.

Explanation of Solution

In case of 1S1P transition, the splitting of 1S state does not take place because for this state, the value of L=0 and so ML=0. Therefore, splitting of only 1P state occurs due to the presence of degenerate ML=10 and +1 states. The value of ΔE is calculated by the formula shown below.

ΔE=μBMLB…(1)

Where,

μB is the Bohr magneton (9.274×1024J/T).

ML is the magnetic quantum number.

B is the magnetic field.

The value of magnetic field is 2.35 T.

For, ML=1.

Substitute the values of μB, B and ML=1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×1×2.35 T=2.179×1023 J2.18×1023 J

For, ML=0

Substitute the values of μB, B and ML=0 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×0×2.35 T=0 J

For, ML=+1.

Substitute the values of μB, B and ML=+1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×+1×2.35 T=+2.179×1023 J+2.18×1023 J

Therefore, the values of ΔE in the transition energies for 1P in the 1S1P transition are 2.18×1023 J, 0 J and +2.18×1023 J.

Conclusion

The values of ΔE in the transition energies for 1P in the 1S1P transition are 2.18×1023 J, 0 J and +2.18×1023 J.

Interpretation Introduction

(b)

Interpretation:

The values of ΔE in the transition energies for each individual transition for the 1P1D transition when a sample is exposed to a magnetic field of 2.35 T are to be calculated.

Concept introduction:

The phenomenon of splitting of a spectral line when a magnetic field is applied to it is known as Zeeman Effect. Magnetic field strength can be measured by using the Zeeman Effect. Applications of Zeeman Effect include NMR spectroscopy, MRI and electron spin resonance spectroscopy.

During an electronic transition, an electron from ground state moves straight to the excited state keeping the internuclear distance constant.

The change in the energy of the state, ΔE is calculated by the formula shown below.

ΔE=μBMLB

Expert Solution
Check Mark

Answer to Problem 16.8E

The values of ΔE in the transition energies for 1P in 1P1D transition are 2.18×1023 J, 0 J and +2.18×1023 J.

The values of ΔE in the transition energies for 1D in 1P1D transition are 4.358×1023 J, 2.18×1023 J, 0 J, +2.18×1023 J and +4.35×1023 J.

Explanation of Solution

In case of 1P1D transition, the splitting of 1P state occurs due to the presence of degenerate ML=10 and +1 states. The value of ΔE is calculated by the formula shown below.

ΔE=μBMLB…(1)

Where,

μB is the Bohr magneton (9.274×1024J/T).

ML is the magnetic quantum number.

B is the magnetic field.

The value of magnetic field is 2.35 T.

For, ML=1.

Substitute the values of μB, B and ML=1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×1×2.35 T=2.179×1023 J2.18×1023 J

For, ML=0

Substitute the values of μB, B and ML=0 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×0×2.35 T=0 J

For, ML=+1.

Substitute the values of μB, B and ML=+1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×+1×2.35 T=+2.179×1023 J+2.18×1023 J

Therefore, the values of ΔE in the transition energies for 1P are 2.18×1023 J, 0 J and +2.18×1023 J.

In case of 1P1D transition, the splitting of 1D state occurs due to the presence of degenerate ML=210+1 and +2 states. The value of ΔE is calculated by the formula shown below.

ΔE=μBMLB…(1)

Where,

μB is the Bohr magneton (9.274×1024J/T).

ML is the magnetic quantum number.

B is the magnetic field.

The value of magnetic field is 2.35 T.

For, ML=2.

Substitute the values of μB, B and ML=2 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×2×2.35 T=4.358×1023 J

For, ML=1.

Substitute the values of μB, B and ML=1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×1×2.35 T=2.179×1023 J2.18×1023 J

For, ML=0

Substitute the values of μB, B and ML=0 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×0×2.35 T=0 J

For, ML=+1.

Substitute the values of μB, B and ML=+1 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×+1×2.35 T=+2.179×1023 J+2.18×1023 J

For, ML=+2.

Substitute the values of μB, B and ML=+2 in equation (1) to calculate the change in energy.

ΔE=9.274×1024J/T×+2×2.35 T=+4.35×1023 J

Therefore, the values of ΔE in the transition energies for 1D are 4.358×1023 J, 2.18×1023 J, 0 J, +2.18×1023 J and +4.35×1023 J.

Conclusion

The values of ΔE in the transition energies for 1P in 1P1D transition are 2.18×1023 J, 0 J and +2.18×1023 J.

The values of ΔE in the transition energies for 1D in 1P1D transition are 4.358×1023 J, 2.18×1023 J, 0 J, +2.18×1023 J and +4.35×1023 J.

Want to see more full solutions like this?

Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!
Students have asked these similar questions
The spin quantum number of a nitrogen-14 nucleus isI= 1. What would be the nuclear magnetic resonance spectrum for a proton resonance line that was split by interactionwith (a) two. (b) three equivalent nitrogen-14 nuclei?
(b) Calculate the half width in nanometers for Doppler broadening of the 4s S 4p transition for atomic nickel at 361.939 nm (3619.39 Å) at a temperature of 20,000 K in both wavelength and frequency units. (c) Estimate the natural line width for the transition in (b) assuming that the lifetime of the excited state is 5*10^(-8) s.
Singly-ionized carbon atoms are accelerated through 1050 V and passed into a mass spectrometer to determine the isotopes present. The magnetic field strength in the spectrometer is 0.180 T. (a) Determine the orbital radii for the 12C and 13C isotopes as they pass through the field. cm (12C) cm (13C) (b) Show that the ratio of the radii may be written in the form m1 = V by verifying that your radii in part (a) satisfy this formula. m1 m-
Knowledge Booster
Background pattern image
Similar questions
Recommended textbooks for you
  • Text book image
    Physical Chemistry
    Chemistry
    ISBN:9781133958437
    Author:Ball, David W. (david Warren), BAER, Tomas
    Publisher:Wadsworth Cengage Learning,
Text book image
Physical Chemistry
Chemistry
ISBN:9781133958437
Author:Ball, David W. (david Warren), BAER, Tomas
Publisher:Wadsworth Cengage Learning,