The Hydrogen Atom: Photon Energy of n=4 to n=3 Transition

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SUMMARY

The energy of the photon emitted during the transition of a hydrogen atom from the n=4 to n=3 energy state is calculated using the Rydberg formula. The formula is E = -Rhc(1/n1^2 - 1/n2^2), where R is the Rydberg constant (1.097x10^-2 nm^-1), h is Planck's constant (6.626x10^-34 J*s), and c is the speed of light (2.998x10^8 m/s). Substituting n1=4 and n2=3 yields an energy of 2.178x10^-18 J, corresponding to a wavelength of approximately 911.7 nm, which is in the infrared region of the electromagnetic spectrum.

PREREQUISITES
  • Understanding of the Rydberg formula for hydrogen transitions
  • Knowledge of Planck's constant and its application in quantum mechanics
  • Familiarity with the concept of energy levels in hydrogen atoms
  • Basic understanding of the electromagnetic spectrum
NEXT STEPS
  • Study the derivation and applications of the Rydberg formula
  • Explore the significance of Planck's constant in quantum physics
  • Learn about energy level transitions in other elements beyond hydrogen
  • Investigate the properties of infrared radiation and its applications
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Students of physics, educators teaching quantum mechanics, and researchers focusing on atomic transitions and spectroscopy will benefit from this discussion.

UrbanXrisis
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What is the energy of the photon when the Hydrogen aton transitions from the n=4 to n=3 energy state?
 
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UrbanXrisis said:
What is the energy of the photon when the Hydrogen aton transitions from the n=4 to n=3 energy state?

It has E = E4 - E3 because energy is conserved.

Use the Bohr energy level equation to find the indiviual level values
 


The energy of a photon emitted during the transition of a hydrogen atom from the n=4 to n=3 energy state can be calculated using the Rydberg formula:

E = -Rhc(1/n1^2 - 1/n2^2)

Where E is the energy of the photon, R is the Rydberg constant (1.097x10^-2 nm^-1), h is Planck's constant (6.626x10^-34 J*s), and c is the speed of light (2.998x10^8 m/s).

Plugging in the values for n1=4 and n2=3, we get:

E = -((1.097x10^-2 nm^-1)(6.626x10^-34 J*s)(2.998x10^8 m/s))(1/4^2 - 1/3^2)

= -2.178x10^-18 J

Therefore, the energy of the photon emitted during the n=4 to n=3 transition is 2.178x10^-18 J. This corresponds to a wavelength of approximately 911.7 nm, which falls within the infrared region of the electromagnetic spectrum.
 

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