atomic Flashcards

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1
Q

Bohr’s first pstulate

A

Electrons move in circular orbits about the nucleus under the influence of coulomb attraction, obeying classical mechanics –> exsistence of the nucleus

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2
Q

bohrs 2nd postulate

A

an electron can only move in an orbit for which its orbital angular momentum L is an intergral multiple of hbar (hbar=h/2pi)

L=nhbar n is a integer

–> introduces quantisation

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3
Q

bohrs third postulate

A

the electron is stable in its orbit: constant energyy E and does not radiate
–> removes problem of stability ( by stating that this law of classical mechanics does not apply)

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4
Q

bohrs fourth postulate

A

absoption and emission are possible through the movement of an electron between two stable orbits and a and b. Radiation frequency , v, of absoption/emission given by
v_ab = (Ea-Eb)/h

–>, basically einsteins postualte v=E/h

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5
Q

what did sommerfeld do

A

observed high resolution spectra lines and took inspiration from Bohr’s model to derive an extension on this model

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6
Q

what does the sommerfeld extension allow

A

elliptical orbits as well as circular orbits . All orbits have the same energy. This is keplers law of Ellipses. sommerfeld stated that it is also true for atoms

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7
Q

what does k do

A

distinguish between elliptical and circular orbits.

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8
Q

orbital angular momentum quantum numbers

A

l=0 s sharp
l=1 p principle
l=2 d diffuse
l=3 f fundamental

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9
Q

atoms in a uniform magnetic field

A

will experience Zeeman effect

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10
Q

atoms in a non-uniform magnetic field

A

will undergo displacement–> stern Gerlachh effect

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11
Q

the zeeman effect (what did he observe)

A

that when placed in a magnetic field, an atom’s emission spectrum contains lines that arre split into several components.

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12
Q

what is the zeeman effect

A

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

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13
Q

what did the stern-gerlach experiment show

A

it provided direct proof that the z component of the magnetic dipole moments of atoms is quantised. space qunatisation

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14
Q

what did the stern-gerlach experiment involve

A

the experiment involves directing a beam of silver atoms (produced by a hot oven) through a non-uniform magnetic field. the beam is collimated by an aperture before entering a magnet that produces a magnetic field that increasses in intensity in the z direction

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15
Q

what was the result of the stern gerlach experiment

A

he found that the beam is split into two components, one in the +z direction and the other in the -z direction

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16
Q

spin-orbit interaction

A

an internal magnetic field is associated with the electrons orbital angular momentum.

17
Q

spin orbit coupling

A

The electron is acted on by a strong internal magnetic field, the orientation of which is determined by L. This produces a torque on its spin magnetic dipole moment, the orientation of which is determined by S. This torque casuses L and S to couple together known as spin orbit coupling

18
Q

define total angular momentum J

A

J=L+S

19
Q

Pauli Exclusion Principle

A

A state specified by the quantum number n,l,m can be occupied by at most two electrons, one with spin up and the other with spin down.

20
Q

why do doublets occur

A

due to the smaller spliiting caused by the psin-orbit interaction . The 3p level is split into j =3/2 and j =1/2 states

21
Q

Normal zeeman effect

A

Occurs for atomic systems with zero total spin angular momentum

an applied magnetic field couples tothe total orbital angular momentum

the levels split by an amount determined by a constant and hte magnetic quantum number m

22
Q

Anomalous Zeeman effect

A

occurs for atomic systems that have atotal spin angular momentum

this caues a different splitting ratio in different levels leading to the observation of more that three components to a transition.

23
Q

Emission spectra

A

: An emission spectrum is composed of a series of discrete spectral lines.
Each line arises from a specific transition between two bound states as an excited
electron de-excites to a lower energy level resulting in the emission of a photon.

24
Q

absoption spectra

A

An absorption spectrum consists of a continuum with narrow dark lines
appearing at specific wavelengths. These absorption lines arise after a photon is
absorbed, exciting an electron from a lower energy level to a bound upper state

25
Q

production of optical spectra lines

A

Optical spectral lines occur when an outer (valence) electron makes a
transition between two bound states causing the emission of a photon.

26
Q

production of xray spectral lines

A

X-ray spectra correspond to states of inner or ‘core’ electrons which are bound in
filled shells

27
Q

Absorption

A

absorption of a photon takes the atom from a lower energy level E1 to a energetically higher energy level E2. A photon with Delta E= E2-E1=hv is removed from the radiation field

28
Q

spontaneous emission

A

An electron in a higher energy state, E2 dexcites to a lower energy state E1. spontaneously emitting a photon of specific energy E to the radiation field

29
Q

stimulated emission

A

emission of photon by atom under the influence of applied radiation field. Two photons result from interaction of a single incoming photon. The ‘new’ photon has the same phase and frequency and travels in the same direction as the incoming photon.

30
Q

what is an absoption edge in an xray spectroscopy

A

absorption edges are quantum at which the absorption coefficeient jumps to a higher energy value. These edges correspond to the series limits for the K, L , M …, series. The sub shells also appear as edges.