4 - radius of nucleus & mass spectrometer

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  • 8/12/2019 4 - Radius of Nucleus & Mass Spectrometer

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    Nuclear Physics

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    Recap

    The famous Geiger-Marsden Alpha scattering

    experiment (under Rutherfords guidance)

    In 1909, Geiger and Marsden were

    studying how alpha particles are scattered

    by a thin gold foil.

    Alpha

    source

    Thin gold foil

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    Geiger-Marsden

    As expected, most alpha particles were

    detected at very small scattering angles

    Alpha particles

    Thin gold foil Small-angle

    scattering

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    Geiger-Marsden

    To their great surprise, they found that

    some alpha particles (1 in 20 000) had

    very large scattering angles

    Alpha particles

    Thin gold foil Small-angle

    scattering

    Large-angle

    scattering

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    Explaining Geiger and Marsdens results

    The results suggested that the positive (repulsive) charge must beconcentrated at the centre of the atom. Most alpha particles do not pass

    close to this so pass undisturbed, only alpha particles passing very close to

    this small nucleus get repelled backwards (the nucleus must also be very

    massive for this to happen).

    Remember on this scale, if the

    nucleus is 2 cm wide, the atom

    would be 200 m wide!

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    Rutherford did the calculations!

    Rutherford calculated theoretically the

    number of alpha particles that should be

    scattered at different angles (using

    Coulombs law). He found agreement withthe experimental results if he assumed the

    atomic nucleus was confined to a diameter

    of about 10-15metres.

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    Closest approach (new)

    Using the idea of energy conservation, Rutherford found

    it is possible to calculate the closest an alpha particle

    can get to the nucleus during a head-on collision.

    Alpha particle

    nucleus

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    Closest approach

    Initially, the alpha particle has kinetic

    energy = mu2

    K.E. = mu2

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    Closest approach

    At the point of closest approach, the

    particle reaches a distance rfrom the

    nucleus and comes momentarily to rest.

    r

    K.E. = 0

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    Closest approach

    All the initial kinetic energyhas been

    transformedto electrical potential energy.

    K.E. = 0

    r

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    Closest approach

    Using the formula for electrical potential energywhich is derived from Coulombs law

    Kinetic energy lost = Electrical potential

    mu2= 1 q1q2

    4o r

    K.E. = 0

    r

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    Closest approach

    Rearranging we get;

    r = 1 q1q2

    4o mu2

    In this case k is the Coulomb constant

    K.E. = 0

    r

    umkr qq

    2

    21

    21

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    Closest approach

    For an alpha particle, m = 6.7 x 10-27kg, q1= 2 x (1.6 x

    10-19C) and u is around 2 x 107m.s-1. If the foil is made

    of gold, q2is 79 x (1.6 x 10-19C).

    r = 1 q1q2

    4o mu2

    r = 1 x (2 x 1.6 x 10-19C) x (79 x 1.6 x 10-19C)

    4x 8.85 x 10-12Fm-1 x 6.7 x 10-27kg x (2 x 107m.s-1)2

    r = 2.7 x 10-14m

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    Rutherfords findings From the equation Rutherford found that the alpha particles

    approached nuclei to within 3.2 x 10-14 m when the foil was made of

    gold. Hence the radius of the gold nucleus must be less than this

    value.

    For silver atoms the closest distance of approach was found to be

    2 x 10-14 m.

    From these results, Rutherford concluded that the positive charge is

    concentrated in a small sphere, that he called the nucleus. Whose

    radii is no greater than about 10-14 m.

    A new length was suggested for these small values called the

    femtometer (fm) where 1 fm 10

    -15

    m. Since the time of Rutherfords scattering experiments, a multitude of

    other experiments have shown that most nuclei are roughly

    spherical and have an average radius given by;

    A is the mass number and r0is a constant

    equal to 1.2 x 10-15 m.

    31

    0Arr

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    Video

    Closest approach, and mass spectrometer

    http://www.youtube.com/watch?v=PiTtRaqqJAshttp://www.youtube.com/watch?v=PiTtRaqqJAs
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    The mass spectrometer

    A VERY useful machine for measuring the

    masses of atoms (ions) and their relative

    abundances.

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    The Mass Spectrometer

    ions

    produced

    velocity selector

    ionsaccelerated

    Region of

    magnetic field

    detector

    ion beam

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    The Mass Spectrometer

    Electrons are produced at a

    hot cathode and accelerated

    by an electric field. Collisionwith gas particles produces

    ions.

    Substance to be tested

    is turned into a gas byheating.

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    The Mass Spectrometer

    Ions acclerated by

    an electric fieldNarrow slit through

    which ions pass

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    The Mass Spectrometer

    Velocity selector In many experiments involving the motion of charged particles it is

    important to have particles moving with the same velocity. This is

    achieved by using a combination of an electric field and a magnetic

    field, as shown below. The orientation is known as crossed fields.

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    Mass Spec.Velocity selector

    A uniform electric field vertically downward is provided by a pair ofcharged parallel plates, while a uniform magnetic field is applied

    perpendicular to the page. For q positive, the magnetic force qvB is

    upward and the electric force qE is downward.

    If the fields are chosen such that the magnetic force balances the

    electric force, the particle moves in a straight horizontal line throughthe region of the fields.

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    Mass Spec.Velocity selector

    If we adjust the size of the two fields so that qvB = qE, we get

    Only those particles having this speed pass undeflected through the

    perpendicular electric and magnetic fields. The magnetic force

    acting on particles with speeds greater than this is stronger than the

    electric force, and these particles are deflected upward. Thosehaving speeds less than this are deflected downward.

    B

    Ev

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    The Mass Spectrometer

    Ions enter the velocity selectorwhich

    contains an electric field (down the

    page) and magnetic field (into the

    page) at right anglesto each other.

    By choosing a suitable value for the

    magnetic field the ions continue in a

    straight line. i.e. The force produced

    by the electric filed (qE) is equal to

    the force produced by the magnetic

    field (Bqv). qE = Bqv

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    The Mass Spectrometer

    qE = Bqv

    orv = E/B

    This means that only ions with a

    specific velocity pass through this

    region. (Hence velocity selector)

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    The Mass Spectrometer

    The selected ions all with the

    same velocity (but different

    masses of course) enter the

    second region of magnetic

    field (also into the page). They

    are deflected in a circular

    path.

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    The Mass Spectrometer

    Heavier ions continue forward

    and hit the sides, as do ions

    that are too light. Only ions of

    one particluar mass reach thedetector.

    The radius of the circle is

    given by R = mv/qB so the

    mass can be calculated from

    m = RqB/v

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    The Mass Spectrometer

    The magnetic field can be varied

    so that ions of different mass can

    be detected (higher B would

    mean that ions of larger mass

    could be directed at the detector).

    In an experiment B is gradually

    varied from low to high so that all

    ions pass through and their

    relative abundance measured.

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    The Mass Spectrometer

    The detector can measure the

    numbers of ions detected,hence giving an idea of

    relative abundance of different

    ions.

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    The Mass Spectrometer

    The mass spectrometer is

    particulary useful foridentifying isotopesof the

    same element.

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    Nuclear energy levels

    We have seen previously that electrons exist inspecific energy levels around the atom.

    There is evidence that energy levels existinside the nucleus too.

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    Nuclear energy levels

    When a nucleus decays by

    emitting an alpha particle or

    a gamma ray, the particles

    or photons emitted are onlyat specific energies (there is

    not a complete range of

    energies emitted, only

    certain specific levels).

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    Nuclear energy levels

    An alpha particle or photon thus has an

    energy equal to the difference between

    energy levels of the nucleus.

    energy

    levels in235U

    (MeV)

    51.57

    0.051

    0.013

    0.000

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    Nuclear energy levels

    In the alpha decay of 239Pu to 235U, the plutonium

    nucleus with an energy of 51.57 MeV can decay into

    Uranium at 3 different energy levels.

    energy

    levels in235U

    (MeV)

    51.57

    0.051

    0.013

    0.000

    Plutonium-239

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    Nuclear energy levels

    If the 239Pu (51.57 MeV) decays to the ground stateof235U (0 MeV), an alpha particle of energy 51.57 MeV is

    emitted.

    energy

    levels in235U

    (MeV)

    51.57

    0.051

    0.013

    0.000

    Plutonium-239

    Alpha emission (51.57

    MeV)

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    Nuclear energy levels

    If the 239Pu (51.57 MeV) decays to the 2nd excited state

    of 235U (0.051 MeV), an alpha particle of energy 51.57-

    0.051 = 51.52 MeV is emitted. The uranium nucleus is

    now in an excited state so can decay further by gamma

    emission to the ground state.energy

    levels in235U

    (MeV)

    51.57

    0.051

    0.013

    0.000

    Plutonium-239

    Alpha emission

    (51.52 MeV)

    Gamma

    emission (0.051

    MeV)

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    Nuclear energy levels

    In fact the nucleus could decay first to the 0.013 level,

    and then the ground state, thus emitting two gamma

    photons.

    energy

    levels in235U

    (MeV)

    51.57

    0.051

    0.013

    0.000

    Plutonium-239

    Alpha emission

    (51.52 MeV)

    Gammaemission (0.038

    MeV)

    Gamma

    emission

    (0.013MeV)

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    Nuclear energy levels

    Notice that the energy of the emitted alpha

    particles can only have certain discrete

    values and that the gamma rays are

    observed with a discrete spectra.

    Remember gamma rays are part of the

    EMS.

    This is evidence that the nucleus like theatom is a quantum system and so has

    discrete energy levels.

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    Radioactive decay

    Beta () and positron decay (+)

    decay

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    Radioactive decay

    In beta decay, a neutron in the nucleus

    decays into a proton, an electron and an

    antineutrino.

    n p + e + ve1

    0

    1

    1

    0

    -1

    0

    0

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    Radioactive decay

    In positron decay, a proton in the nucleus

    decays into a neutron, a positron (the

    antiparticle of the electron) and a neutrino.

    p n + e + ve

    http://www.youtube.com/watch?v=lAAmAbJvvJg

    1

    1

    1

    0

    0

    +1

    0

    0

    http://www.youtube.com/watch?v=lAAmAbJvvJghttp://www.youtube.com/watch?v=lAAmAbJvvJg
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    The antineutrino

    The antineutrinoin beta decaywas not

    detected until 1953, although its presence

    had been predicted theoretically.

    n p + e + ve1

    0

    1

    1

    0

    -1

    0

    0

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    The antineutrino

    The mass of the neutron is bigger than

    that of the proton and electron together.

    n p + e + ve

    1.008665u(1.007276 + 0.0005486)u = 0.00084u

    1

    0

    1

    1

    0

    -1

    0

    0

    1.008665 u 1.007276 u 0.0005486 u

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    The antineutrino

    This corresponds (using E = mc2) to an

    energy of 0.783 MeV.

    n p + e + ve1

    0

    1

    1

    0

    -1

    0

    0

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    The antineutrino

    This extra energy should show up as kinetic energy ofthe products (proton and electron). Since the electronshould carry most of the kinetic energy away, so weshould observe electrons with an energy of about 0.783

    MeV.

    n p + e + ve

    In fact we observe electrons with a rangeof energiesfrom zero up to 0.783 MeV.

    1

    01

    1

    0

    -1

    0

    0

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    The antineutrino

    Where is the missing energy? In 1933 Wolfgang Pauli and

    Enrico Fermi hypothesized the existence of a third very light

    particle produced during the decay. Enrico Fermi coined the

    term neutrino for the little neutral one

    n p + e + ve1

    0

    1

    1

    0

    -1

    0

    0

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    Radioactive decay

    The rate of decay (number of nuclei that will

    decay per second) is proportional to the

    number of undecayed nuclei

    dN = -N

    dt

    = decay constant = the likelihood that an

    individual particle will decay in a second

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    The radioactive decay law

    If the number of nuclei present in a sample at t =

    0 is N0, the number Nstill present at time tlater

    is given by

    N = Noe-t

    where is the decay constant (the probabilitythat a nucleus will decay in unit time)

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    Half-life

    After one half-life, the number of original

    nuclei present is equal to N0/2. Putting this

    into the radioactive decay law;

    N0/2 = N0e(-t)where tis the half-life

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    Activity

    A =N = N = Noe-t

    t

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    Measuring half-life

    For short half-lives, the half life can usually

    be measured directly.

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    Measuring half-life

    For longer half lifes, values of activitycan

    be measured and the decay law can be

    used to calculate and thus t.

    Measure the activity A and chemicallyfindthe number of atoms of the isotope.

    UseA = N and then t= ln2