問題一覧
1
B. The state of a quantum system is represented by a wavefunction, which contains all possible measurements of the system.
2
A. W must be an eigenfunction of A with a corresponding eigenvalue
3
A. The wavefunction collapses into a single eigenfunction corresponding to one of the eigenvalues.
4
C. The uncertainty principle applies, meaning that measuring one observable precisely increases uncertainty in the other.
5
A. a
6
C. h/2
7
B. [x^p^x]=ih
8
A. The wavefunction collapses into the eigenfunction on corresponding to an.
9
A. The same eigenvalue a n with probability 1.
10
A. It determines the shape of the orbital.
11
A. Hermitian operators guarantee that eigenvalues correspond to real physically measurable quantities.
12
C. Any function of a Hermitian operator is alto Hermitian.
13
D. The Hamiltonian operator always commutes with the momentum operator in all systems.
14
C. A must be a Hermitian operator.
15
C. The expectation value of an operator is given by (A)»Ψ-AWdx, even if W is not normalized.
16
A. A particle's position and momentum cannot be measured simultaneously with arbitrary precision because measurement disturbs the system.
17
Α. Δρ >_h/2L
18
B. The square of the expansion coefficient (cn) in the eigenfunction expansion of W.
19
B. It behaves as a free-particle motion.
20
A. Energy levels depend only on n, and states with different I values but the samen are degenerate.
21
B. The hydrogen atom problem.
22
C. It decays exponentially.
23
B.r=a0
24
A. The wavefunction collapses into an eigenstate of Å associated with the measured eigenvalue.
25
B. A spherical surface where the probability density is zero.
26
A. Separation into center-of-mass and relative motion coordinates.
27
C. The electrons independently follow a 1s-orbital distribution similar to hydrogen
28
C. Parahelium has electrons in a singlet spin state, while orthohelium has electrons in a triplet spin state
29
C. n-1-1
30
A. A simple hydrogenic wavefunction for each electron, neglecting electron- electron interactions
31
B)-Z/n^2 RH
32
A) Principal quantum number (n)
33
C) The total wavefunction must be antisymmetric under the exchange of two electrons
34
B) Exchange energy results from the antisymmetry of the total wavefunction and is a purely quantum mechanical effect
35
C) A hydrogen-like Coulomb potential due to the nucleus
36
C) It assumes electrons do not interact with each other
37
A) One electron remains in the 1s orbital while the second electron is excited to a higher orbital
38
B)-3.25RH
39
C) It splits degenerate states into different energy levels
40
C) 1s2s→ 1s2
41
C) It ignores electron-electron repulsion
42
B) It decreases the effective nuclear charge felt by the electrons
43
C) Because electrons are fermions and obey the Pauli Exclusion Principle
44
A) The spatial wavefunction must be symmetric
45
B) To satisfy the Pauli Exclusion Principle
46
C) E=-8RH
47
C) The principal (n), azimuthal (1), magnetic (ml), and spin (ms) quantum numbers
48
B) Orbital angular momentum quantum number I
49
B) Electron-electron interactions and screening effects
50
A) L = 0
51
A) s = 0 for singlet states and s = 1 for triplet states
52
A) deta L = 0 , +- (but not L = 0 -> L = 0 )
53
C) 3d
54
A) It assumes that each electron moves in an average field created by all other electrons.
55
D) L = 1,2
56
D) J = 2, 3, 4
57
B) Electron-electron repulsions significantly modify energy levels.
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1
B. The state of a quantum system is represented by a wavefunction, which contains all possible measurements of the system.
2
A. W must be an eigenfunction of A with a corresponding eigenvalue
3
A. The wavefunction collapses into a single eigenfunction corresponding to one of the eigenvalues.
4
C. The uncertainty principle applies, meaning that measuring one observable precisely increases uncertainty in the other.
5
A. a
6
C. h/2
7
B. [x^p^x]=ih
8
A. The wavefunction collapses into the eigenfunction on corresponding to an.
9
A. The same eigenvalue a n with probability 1.
10
A. It determines the shape of the orbital.
11
A. Hermitian operators guarantee that eigenvalues correspond to real physically measurable quantities.
12
C. Any function of a Hermitian operator is alto Hermitian.
13
D. The Hamiltonian operator always commutes with the momentum operator in all systems.
14
C. A must be a Hermitian operator.
15
C. The expectation value of an operator is given by (A)»Ψ-AWdx, even if W is not normalized.
16
A. A particle's position and momentum cannot be measured simultaneously with arbitrary precision because measurement disturbs the system.
17
Α. Δρ >_h/2L
18
B. The square of the expansion coefficient (cn) in the eigenfunction expansion of W.
19
B. It behaves as a free-particle motion.
20
A. Energy levels depend only on n, and states with different I values but the samen are degenerate.
21
B. The hydrogen atom problem.
22
C. It decays exponentially.
23
B.r=a0
24
A. The wavefunction collapses into an eigenstate of Å associated with the measured eigenvalue.
25
B. A spherical surface where the probability density is zero.
26
A. Separation into center-of-mass and relative motion coordinates.
27
C. The electrons independently follow a 1s-orbital distribution similar to hydrogen
28
C. Parahelium has electrons in a singlet spin state, while orthohelium has electrons in a triplet spin state
29
C. n-1-1
30
A. A simple hydrogenic wavefunction for each electron, neglecting electron- electron interactions
31
B)-Z/n^2 RH
32
A) Principal quantum number (n)
33
C) The total wavefunction must be antisymmetric under the exchange of two electrons
34
B) Exchange energy results from the antisymmetry of the total wavefunction and is a purely quantum mechanical effect
35
C) A hydrogen-like Coulomb potential due to the nucleus
36
C) It assumes electrons do not interact with each other
37
A) One electron remains in the 1s orbital while the second electron is excited to a higher orbital
38
B)-3.25RH
39
C) It splits degenerate states into different energy levels
40
C) 1s2s→ 1s2
41
C) It ignores electron-electron repulsion
42
B) It decreases the effective nuclear charge felt by the electrons
43
C) Because electrons are fermions and obey the Pauli Exclusion Principle
44
A) The spatial wavefunction must be symmetric
45
B) To satisfy the Pauli Exclusion Principle
46
C) E=-8RH
47
C) The principal (n), azimuthal (1), magnetic (ml), and spin (ms) quantum numbers
48
B) Orbital angular momentum quantum number I
49
B) Electron-electron interactions and screening effects
50
A) L = 0
51
A) s = 0 for singlet states and s = 1 for triplet states
52
A) deta L = 0 , +- (but not L = 0 -> L = 0 )
53
C) 3d
54
A) It assumes that each electron moves in an average field created by all other electrons.
55
D) L = 1,2
56
D) J = 2, 3, 4
57
B) Electron-electron repulsions significantly modify energy levels.