Atomic Physics Flashcards

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1
Q

what does spectroscopy involve

A

the measurement of the wavelength frequency and energy of EM radiation

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2
Q

deBroglie equation

A

P=hbar(K) =h/lambd=hv/c

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3
Q

Absorption

A

a photon takes the atom from E_1 to E_2. A photon with energy deltaE = E_2 - E_1 = hv is removed from the radiation field

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4
Q

spontaneous emission

A

AN electron in a higher energy state de-excites to a lower energy state spontaneouslt emitting a phtoton of a specific energy E_if (I= intial energy state, f= final energy state) to the radiation field

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5
Q

what type of gas involve emission

A

hot gas, due to the atoms needing to be in a excited state

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6
Q

Bohr first postulate

A

Electronsmove in circular orbits about the nucleus under the influence of coulomb attraction, obeying classical mechanics.

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7
Q

what did Bohr’s first postulate show

A

the existence of the nucleus

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8
Q

Bohr’s second postulate

A

An electron can only move in an orbit for which its orbital angular momentum L in an integral multiple of hbar L=n(hbar)

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9
Q

what did Bohr’s second postulate show

A

it introduced quantisation

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10
Q

Bohr’s third postulate

A

The electron is stable in its orbit: constant energy E and does not radiate

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11
Q

What does Bohr’s third postulate show

A

It removes problem of stability (by stating that this law of classical mechanics does not apply)

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12
Q

Bohr’s Fourth postulate

A

Absorption and emission are possible through the movement of an electron between two stale orbits, a and b. Radiation frequency v of absorption / emission goes by : V_ab = (E_a - E_b)/h

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13
Q

what did Bohr’s fourth postulate show

A

Basically Einstein’s postulate v=E/h

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14
Q

n-fold degenerate

A

when the total energy of the electron onl depends on n

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15
Q

What four things did schordinger’s theory reveal about the properties of the atom

A

Probability density functions
orbital angular momentum
electron spin
transition rate

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16
Q

what are degenerate eigenfunctions

A

eigenfunctions corresponding to the same eigenvalue are degenerate

17
Q

magnetic dipole in a non uniform field

A

a magnetic diploe in a non uniform field experiences a torque which will cause precession and a force which will cause displacement.

18
Q

what will atoms experience in a uniform magnetic field

A

Zeeman effect

19
Q

what will happen to atoms in a non-uniform field (what effect)

A

atoms undergo displacement due to the stern Gerlach effect

20
Q

what is the Zeeman effect

A

The Zeeman effect is the splitting of atomic energy levels and the associated spectral lines that result when the atoms are placed in a magnetic field.

21
Q

what did the stern Gerlach experiment show

A

The experiment showed, qualitatively,that the orientation of atoms in space is quantised.
space quantisation.

it showed that Schrödinger’s theory was not complete due to missing out electron spin.

22
Q

Define total angular Momentum J

A

J = L + S

where J = total angular momentum
S = torque due to spin
L = orientation

23
Q

Quantum defect

A

A quantum defect, δ(n,l)—a correction to the principle quantum number, n.

24
Q

anomalous Zeeman effect

A

The splitting of some spectral lines did not occur as expected in a magnetic field.

25
Q

normal zeeman effect

A

used to describe lines that split as expected. Ths splitting can be explained by the quantization of angular momentum.

26
Q

3 Things about Normal Zeeman effect

A
  • atomic systems with 0 total spin angular momentum
  • applied magnetic field couples to the total orbital angular momentum - the levels split by an amount determined by a constant and the magnetic quantum number m
27
Q

2 things about anomalous Zeeman effect

A
  • occurs for atomic systems that have total sin angular momentum.
  • This causes a different splitting ratio in different levels leading to the observation of more than three components to a transition