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Ch 41: Quantum Mechanics II: Atomic Structure
Young & Freedman Calc - University Physics 15th Edition
Young & Freedman Calc15th EditionUniversity PhysicsISBN: 9780135159552당신이 사용하는 게 아니라요?교과서 변경
40장, 문제 27

Calculate the energy difference between the ms=12m_{s}=\(\frac\)12 ('spin up') and ms=12m_{s}=-\(\frac\)12 ('spin down') levels of a hydrogen atom in the 1s1s state when it is placed in a 1.451.45 T magnetic field in the negative zz-direction. Which level, ms=12m_{s}=\(\frac\)12 or ms=12m_{s}=-\(\frac\)12, has the lower energy?

검증된 단계별 안내
1
Understand the problem: The energy difference between the spin-up (ms = +1/2) and spin-down (ms = -1/2) states of an electron in a magnetic field is due to the Zeeman effect. The energy of each state is given by the formula E = -μz * B, where μz is the z-component of the magnetic moment and B is the magnetic field strength.
Recall the relationship between the magnetic moment and the spin quantum number: The magnetic moment μz is related to the spin quantum number ms by the formula μz = -g * μB * ms, where g is the g-factor (approximately 2 for an electron), μB is the Bohr magneton (9.274 × 10^-24 J/T), and ms is the spin quantum number (+1/2 or -1/2).
Substitute the expression for μz into the energy formula: The energy of a state becomes E = g * μB * ms * B. For ms = +1/2 (spin-up) and ms = -1/2 (spin-down), calculate the energy for each state using this formula.
Determine the energy difference: The energy difference ΔE between the two states is given by ΔE = E(ms = +1/2) - E(ms = -1/2). Substitute the values of ms and simplify the expression to find ΔE = g * μB * B.
Identify the lower energy state: Since the energy is proportional to ms, the ms = -1/2 (spin-down) state will have a lower energy in a magnetic field pointing in the negative z-direction. This is because the magnetic moment aligns with the field direction, minimizing the energy.

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주요 개념

질문에 올바르게 답하기 위해 반드시 이해해야 하는 핵심 개념들은 다음과 같습니다.

Zeeman Effect

The Zeeman Effect describes the splitting of spectral lines in the presence of a magnetic field. In the context of atomic physics, it explains how the energy levels of electrons in an atom, such as hydrogen, are affected by an external magnetic field, leading to different energy states for different spin orientations.
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가이드 코스
07:40
The Doppler Effect

Magnetic Moment

The magnetic moment is a vector quantity that represents the magnetic strength and orientation of a magnetic source. For electrons, it is related to their spin and orbital motion, and it determines how the electron's energy levels shift in a magnetic field, with different orientations experiencing different energy levels.
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가이드 코스
03:08
Intro To Dipole Moment

Energy Level Calculation

The energy difference between the spin states in a magnetic field can be calculated using the formula ΔE = gμB B, where g is the Landé g-factor, μB is the Bohr magneton, and B is the magnetic field strength. This calculation allows us to determine which spin state has lower energy based on the orientation of the magnetic moment in the applied field.
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가이드 코스
05:01
Calculating Max Height with Energy Conservation
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교과서 질문

The hyperfine interaction in a hydrogen atom between the magnetic dipole moment of the proton and the spin magnetic dipole moment of the electron splits the ground level into two levels separated by 5.9×1065.9\(\times\)10^{-6} eV. Calculate the wavelength and frequency of the photon emitted when the atom makes a transition between these states, and compare your answer to the value given at the end of Section 41.541.5. In what part of the electromagnetic spectrum does this lie? Such photons are emitted by cold hydrogen clouds in interstellar space; by detecting these photons, astronomers can learn about the number and density of such clouds.

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(b) Use v=rωv=r\(\omega\) and the result of part (a) to calculate the speed vv of a point at the electron's equator. What does your result suggest about the validity of this model?

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A hydrogen atom undergoes a transition from a 2p2p state to the 1s1s ground state. In the absence of a magnetic field, the energy of the photon emitted is 122122 nm. The atom is then placed in a strong magnetic field in the zz-direction. Ignore spin effects; consider only the interaction of the magnetic field with the atom's orbital magnetic moment. How many different photon wavelengths are observed for the 2p1s2p\(\rightarrow\)1s transition? What are the mlm_l values for the initial and final states for the transition that leads to each photon wavelength?

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The doubly charged ion N2+ is formed by removing two electrons from a nitrogen atom. What is the ground-state electron configuration for the N2+ ion?

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