An electron in a hydrogen atom is approximated by a one-dimensional infinite square well potential. The normalised wavefunction of an electron in a stationary state is defined as (x) = √ sin (27), where n is the principal quantum number and L is the width of the potential. The width of the potential is L = 1 x 10-10 m. (a) Explain the meaning of the term normalised wavefunction and why normalisation is important. (b) Use the wavefunction defined above with n = 2 to determine the probability that an electron in the first excited state will be found in the range between x = 0 and x = 1 × 10-¹¹ m. Use an appropriate trigonometric identity to simplify your calculation. (c) Use the time-independent Schrödinger Equation and the wavefunction defined above to find the energies of the first two stationary states. You may assume that the electron is trapped in a potential defined as V(x) = { 0 for 0≤x≤ L ∞ for elsewhere.
An electron in a hydrogen atom is approximated by a one-dimensional infinite square well potential. The normalised wavefunction of an electron in a stationary state is defined as (x) = √ sin (27), where n is the principal quantum number and L is the width of the potential. The width of the potential is L = 1 x 10-10 m. (a) Explain the meaning of the term normalised wavefunction and why normalisation is important. (b) Use the wavefunction defined above with n = 2 to determine the probability that an electron in the first excited state will be found in the range between x = 0 and x = 1 × 10-¹¹ m. Use an appropriate trigonometric identity to simplify your calculation. (c) Use the time-independent Schrödinger Equation and the wavefunction defined above to find the energies of the first two stationary states. You may assume that the electron is trapped in a potential defined as V(x) = { 0 for 0≤x≤ L ∞ for elsewhere.
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![An electron in a hydrogen atom is approximated by a one-dimensional infinite square well
potential. The normalised wavefunction of an electron in a stationary state is defined as
*(x) = √√ sin ("").
L
where n is the principal quantum number and L is the width of the potential. The width of
the potential is L = 1 x 10-¹0 m.
(a) Explain the meaning of the term normalised wavefunction and why normalisation is
important.
(b) Use the wavefunction defined above with n = 2 to determine the probability that
an electron in the first excited state will be found in the range between x = 0 and
x = 1 × 10-¹¹ m. Use an appropriate trigonometric identity to simplify your calculation.
(c) Use the time-independent Schrödinger Equation and the wavefunction defined above to
find the energies of the first two stationary states. You may assume that the electron is
trapped in a potential defined as
V(x) =
0 for 0≤x≤L
∞ for elsewhere.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fa94ef811-7aeb-45cc-a8c4-872250660697%2Ff8d599ad-abcd-468c-af23-7cb5fb58318e%2Ffgltkp8_processed.jpeg&w=3840&q=75)
Transcribed Image Text:An electron in a hydrogen atom is approximated by a one-dimensional infinite square well
potential. The normalised wavefunction of an electron in a stationary state is defined as
*(x) = √√ sin ("").
L
where n is the principal quantum number and L is the width of the potential. The width of
the potential is L = 1 x 10-¹0 m.
(a) Explain the meaning of the term normalised wavefunction and why normalisation is
important.
(b) Use the wavefunction defined above with n = 2 to determine the probability that
an electron in the first excited state will be found in the range between x = 0 and
x = 1 × 10-¹¹ m. Use an appropriate trigonometric identity to simplify your calculation.
(c) Use the time-independent Schrödinger Equation and the wavefunction defined above to
find the energies of the first two stationary states. You may assume that the electron is
trapped in a potential defined as
V(x) =
0 for 0≤x≤L
∞ for elsewhere.
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