01-Atomic n Nuclear Structure

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    Atoms Ordinary matter is composed of atoms. An atom

    consists of a tiny nucleus made up of protons and

    neutrons, on the order of 20,000 times smaller than the

    size of the atom. The outer part of the atom consists of

    a number of electrons equal to the number of protons,

    making the normal atom electrically neutral.

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    Evolution of Theory for Matter

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    Democritus

    400 B.C.

    Aristotle350 B.C.

    JohnDalton1808

    J.J.Thomson

    1897

    HantaroNagaoka

    1904

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    Models of Atom

    Thomsons plum pudding model

    Rutherfords model - the first

    planetary model

    Bohrs model

    Paulis exclusion principle (1925)

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    Rutherford Scattering

    The Rutherford Atomic Model - 1911

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    Distance Of Closest Approach

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    Rutherfords ingredients:

    Newtonian Mechanics (F = ma)

    Coulomb Interaction=> Distance of closest approach

    Coulomb repulsion between the a -particle (2+) and the Au nucleus (79+)

    Let initial KE of a= PE at closest approach distance r.

    KE (a) = 6 MeV

    Therefore, r = 3.8x10-14 m = 38 fm = 38 fermi

    r

    qq

    r

    qq

    F

    21

    0

    2

    21

    0

    4

    1PE

    ;4

    1

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    Distance of closest approach

    The faster an alpha particle is travelling, i.e. the more energy it has,

    the closer it can get to the nucleus before being repelled away.

    For any given initial energy, we can calculate how close the alpha

    particle can get to the nucleus.

    We call this the distance of closest approach.7

    PE

    r

    a

    Stops here

    Distance of closest

    approach

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    Failures of Classical Atomic Model Unstable model, since an accelerated charge radiates i.e. will emit

    light and therefore lose E

    classical mechanics did not work for the planetary model - it

    violated classical laws of electromagnetism

    considerable problems with atomic spectra

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    Bohr Model 1913 A countable number of stationary

    states exist. (electrons in aselection of allowed orbit radii)

    EM radiation emitted when

    electron jumps/transitions between

    states

    Classical rules apply to stationary

    states, but not during transitions

    between states. Angular momentum occurs in

    integer multiples of h/2.

    i.e. mvr = nhence quantized.10

    n=1

    n=2

    n=3

    2 1h E E

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    Quantized Energy States

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    Hydrogen spectral series:

    Patterns in the Spectra

    10 10 0 10 00 10 000

    (IR),8,7,61

    5

    11Pfund

    (IR),7,6,51

    4

    11Brackett

    (IR),6,5,41311Paschen

    (UV),4,3,21

    1

    11Lyman

    nm01097.0

    light)(visible,5,4,31

    2

    11Balmer

    22

    22

    22

    22

    1

    22

    n

    n

    R

    nn

    R

    nn

    R

    nn

    R

    R

    n

    n

    R

    n

    n

    n

    n

    n

    12

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    Energy Transfer Mechanisms

    Excitation of the Atom

    When a sufficient amount of energy is transferred to the atom,causing an electron to jump from the lower to higher energylevels, the atom is said to be excited.

    Ionization of the Atom

    When a sufficient amount of energy is transferred to the atom,causing an electron to be removed from the electric field of thenucleus, the is said to be ionized, and the negative electron

    together with the remaining positively charged atom, is calledthe ion pair.

    Excitation and ionization are the main mechanisms

    through which energy is transferred from radiation to

    matter

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    Problem with Bohrs model and classical

    mechanics

    Could only predict correctly the energy levels of H.

    The dual behavior of light (particle and wave) could

    not be explained by classical mechanics

    The approach of Bohr of mixing classical mechanicwith quantizing certain variables was suddenly

    heavily used

    other accurate predictions were made with newsemi-classical or relativistic models

    Prelude to Quantum Mechanics 14

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    Pauli principle: No two electrons in an atom

    can be in the same state Quantization came naturally out of quantum mechanics

    Four quantum numbers fully described the electron energylevels

    Principal quantum number : n

    Describes the orbital shells

    n=1, 2 and 3 for K, L and M shells respectively

    Corresponds to Bohrs angular momentum quantization

    Azimuthal quantum number: l

    Explains fine structure in spectrum (elliptic orbit)

    l = 0, 1, 2, , n

    Magnetic quantum number: m

    Explains splitting of spectral lines in magnetic field - Zeeman Effect

    m = [-l, l]

    Intrinsic spin (angular momentum) of electron: s s = [-1/2, ]

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    Neutron Chadwiick-1932.

    The mystery particle (Y) has ~ proton mass but no chargeThe Neutron

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    Nuclear Terminology Atomic number (Z) is the number of protons in the nucleus of an atom, and

    also the number of electrons in a neutral atom

    Nucleon: proton (Z) or neutron (N)

    Nuclide: nucleus uniquely specified by the values of N & Z

    Mass number (A) is the total number of nucleons in a nucleus (A=Z+N)

    Isotopes: nuclides with the same protons (Z) e.g. 235U and 238U

    Isotones: nuclides with the same neutrons (N) e.g. 2H (d) and 3He Isobars: nuclides with the same A

    Atomic mass unit (u): one-twelfth of the mass of a neutral atom of 12C (six

    protons, six neutrons, and six electrons). 1 u = 1.66 x 1027 kg = 931.5 MeV/c2

    Atomic mass is the mass of a neutral atom and includes the masses of

    protons, neutrons, and electrons as well as all the binding energy.

    Nuclear mass is the mass of the nucleus and includes the masses of the

    protons and neutrons as well as the nuclear binding energy, but does not

    include the mass of the atomic electrons or electronic binding energy.

    Radioisotopes: members of a family of unstable nuclides with a common

    value of Z

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    Nuclear Notation atomic mass = A

    atomic number = Z = number of protons (+) = number of

    electrons ()

    AZ = number of neutrons (no charge) = N

    e.g.238

    U.A = 238 and U has Z = 92 protons. Therefore, 146 neutrons.

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    Nuclear Units

    SI units are fine for macroscopic objects like footballs but arevery inconvenient for nuclei and particles therefore nuclear unitsare used as:

    Energy: 1 eV = energy gained by electron in beingaccelerated by 1V.

    Mass: MeV/c2

    (or GeV/c2

    )1 MeV/c2= 1.78X10-30kg. 1 GeV/c2= 1.78X10-27kg.Or use Atomic Mass Unit defined by mass of 12C= 12 u

    Momentum: MeV/c (or GeV/c)1 eV/c = e/c kg m s-1

    Cross sections:1 barn =10-28 m2

    Length: fermi (fm)

    1 fm = 10-15m. 19

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    Nuclear Units

    Nuclear energies are very high compared to atomic processes,and need larger units

    Nuclear sizes are quite small and need smaller units

    Nuclear masses are measured in terms of atomic mass units

    (amu, u) with the carbon-12 nucleus defined as having a massof exactly 12 amu. It is also common practice to quote the restmass energy E = mc2as if it were the mass. The conversion toamu is: 20

    1amu = 1.6605 x 10-27kg = 931.5 MeV/c2

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    Constituents of Atoms

    The electrons, protons and neutrons which make up an atomhave definite charges and masses.

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    Constituents of Atoms

    While the charges and masses are precisely known, the sizing isnot. Our best information about the proton and neutron indicatesthat they are constituent particles. However we can attribute tothem a radius of about

    1.2 x 10-15

    meters = 1.2 fm

    The electron is a fundamental particle which is apparently notmade out of any constituent particles.

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    THE END