Ideas of Modern Physics - PowerPoint PPT Presentation

1 / 27
About This Presentation
Title:

Ideas of Modern Physics

Description:

Alpha particles are less penetrating still and positively charged. ... Alphas are He nuclei ... Since an alpha particle weighs 8000 times the electron mass, the ... – PowerPoint PPT presentation

Number of Views:39
Avg rating:3.0/5.0
Slides: 28
Provided by: duncanlc
Category:
Tags: alphas | ideas | modern | physics

less

Transcript and Presenter's Notes

Title: Ideas of Modern Physics


1
Ideas of Modern Physics
  • And when Water and Oil of Vitriol poured
    successively into the same Vessel grow very hot
    in the mixing, does not this heat argue a great
    Motion in the Parts of the Liquors? And does not
    this Motion argue, that the Parts of the two
    Liquors in mixing coalesce with Violence, and by
    consequence rush towards one another with an
    accelerated Motion?
  • -Isaac Newton

2
Premonitions
  • Newton could not help being impressed with his
    own mechanics and theory of gravitation.
  • He was also aware of how little he knew about
    matter and about light.
  • The intuitive description of chemical reactions
    in his own mechanical terms perhaps contained a
    germ of atomic theory.
  • Only many increasingly incisive experiments and
    theories concerning diverse physical phenomena
    would lead to conclusive answers.

3
Review
  • Einsteins analysis of Brownian motion determined
    the mass of the hydrogen atom m_H(gm)1/N_A where
    Avogadros number is 6.02e23
  • Through electrolysis, Faraday related hydrogen
    mass to charge 8600 CN_A e determining e
  • Millikans oil drop experiment measured e 1.602
    e-19 C directly.
  • Thomson measured the ratio e/m_e for cathode ray
    electrons and given e found m_e was tiny compared
    to m_H.
  • Discovery of nuclear radioactivity would provide
    probes of atomic structure.

4
Radiation
  • Unstable atoms spontaneously emit radiation of
    various kinds, both electrically neutral and
    electrically charged.

5
Exponential decay law
  • Decay processes are uncontrolled but follow a
    simple statistical law.
  • The probability an unstable nucleus has decayed
    after time t is Pexp-t/tau where tau is the
    lifetime.
  • Given N objects, the average change dN in a small
    time interval dt is the rate of decay dN/dt
    -N(t)/tau

6
Kinds of rays
  • Alpha particles are less penetrating still and
    positively charged. They turn out to be He
    nuclei.
  • Beta rays are less penetrating negatively charged
    particles. They turn out to be energetic
    electrons.
  • X, gamma rays are penetrating and electrically
    neutral. They turn out to be quanta of
    electromagnetic radiation. X-rays may be radiated
    by electrons. More energetic gamma rays are
    radiated by energetic protons in a nucleus.

7
Alpha particle emission
  • Some radioactive nuclei spontaneously fission
    (fall apart) into smaller nuclei releasing
    neutrons and fragments like (pnpn), a He-4
    nucleus.

Sg-263(106p,157n)gtRf-259(104p,155n)He-4(2p,2n)
8
Alphas are He nuclei
  • In 1909, Rutherford established that so called
    alpha-particles are in fact He-4 nuclei by
    collecting He gas created by neutralized alphas.

http//webserver.lemoyne.edu/faculty/giunta/EA/ROY
DSann.HTML
9
Beta particle creation
  • A free neutron weighs a bit more than a proton
    and decays to a proton plus an electron plus a
    (neutral neutrino)- ngtp,e,nu - in about 13
    minutes.
  • Within a nucleus, this process is suppressed
    because the neutron is tightly bound and
    conversion to a proton requires more energy than
    is available.

10
Radioactive beta decay
  • An excess neutron in a nucleus close to the edge
    of stability can decay. The rate is suppressed
    and may require millions or billions of years but
    in a gram containing N_A1e24 nucleons be
    observable.
  • A neutron is transformed into a proton and the
    electron and neutrino fly out - the elemental
    nucleus is transmuted.

C14 (6p,8n)gt N14(7p,7n) e nu
11
Subnuclear beta decay
  • A proton differs from a neutron by the flavor of
    on quark puud, nudd.
  • Neutron results from the weak interaction of
    quarks in which a down quark radiates a W boson
    which decays to electron and neutrino dgtu W-,
    W- gt e- nu
  • The neutrino was not observed directly until the
    1950s when nuclear reactors were available which
    produced vast numbers of unstable nuclei and
    neutrinos.

12
Example
  • Lead Pb has Z82 and stable isotopes with A 206
    (26),207(21),208(52)
  • The isotope with A210 is unstable.
  • Pb-210 gt Bi-(210) e- nu, tau 20 years.

13
Gamma and X-rays
  • Like atoms, nuclei have excited internal states
    and strong or weak decay may result in an excited
    nucleus which then decays emitting
    electromagnetic radiation
  • Example. In beta decay, the proton may recoil
    against the e and nu so is rattling around inside
    the nucleusCo-60 gt Ni-60 e nu, Ni60gt
    Ni-60 photon with E(photon) 1.2 MeV (gamma
    energy)

14
Geiger counter
  • A tube of gas with a charged axial wire.
  • Electrons are liberated in the gas and ions
    created by collisions of fast charged particles
    with neutral atoms of by absorption of x-rays
  • Electrons drift towards the wire and the ions to
    the wall constituting a small current pulse.

15
Energy in beta decay
  • M_n939.56 MeV/c2
  • M_p 938.27 MeV/c2 M_n1.29 MeV/c2
  • M_e 0.51 MeV/c2 is created
  • M_nu0 (at least lt 1 eV/c2!)
  • About 0.5 MeV is released as kinetic energy
    shared between the e and nu which are
    relativistic and the proton.

16
Energy in alpha decay
  • The binding energy per nucleon is 1 MeV
  • The energy release in alpha emission fission is a
    few MeV.
  • M_alpha 2M_p2M_n4000 MeV
  • The alpha is not relativistic yet carries energy
    equivalent to acceleration through a million volt
    electrostatic potential difference.

17
Rutherfords discovery
  • In 1906, Rutherford measured the charge to mass
    ratio of alpha particles detecting them with
    photographic emulsion. When mica was in the path
    he found the image blurred. Since an alpha
    particle weighs 8000 times the electron mass, the
    deflections could not be ascribed to scattering
    from electrons.
  • In 1909, he suggested Hans Geiger get his
    undergraduate Earnest Marsden to see if an alpha
    could be scattered at a large angle.

18
Scattering apparatus
  • R radon alpha source
  • F target metal foil
  • S zinc sulphide screen scintillates when struck
    by an alpha
  • M microscope

19
Marsden observed large angles
  • Rutherford wrote
  • Then I remember two or three days later Geiger
    coming to me in great excitement and saying "We
    have been able to get some of the alpha-particles
    coming backward " It was quite the most
    incredible event that ever happened to me in my
    life. It was almost as incredible as if you fired
    a 15-inch shell at a piece of tissue paper and it
    came back and hit you.

20
Angular distribution
  • Rutherford supposed the mass and positive charge
    was compressed into a volume much smaller than
    the atom and calculated the probability of
    scattering through an angle theta.
  • The formula fit the data!

21
Splitting the atom
  • The fun was just beginning!
  • In 1919, Rutherford established that an alpha
    impinging on a nitrogen nucleus can cause a
    hydrogen atom to appear! Newspaper headlines
    blared that Rutherford had "split the atom".
  • This was the beginning of nuclear physics when
    yet the real quantum structure of the atom had
    not been established.

22
The structure of the nucleus
  • The mass numbers A are not equal to the atomic
    charge numbers Z. Why?
  • Perhaps for example the alpha particle, the He
    nucleus, with A4 and Z2, was 4 protons and two
    electrons?
  • Rutherford suggested perhaps a proton and an
    electron could form not just a hydrogen atom but
    a tightly bound neutral state - a neutron.

23
Discovery of the neutron
  • A neutron is electrically neutral so does not
    respond to electric or magnetic fields nor
    produce ionization directly.
  • Rutherfords student James Chadwick searched for
    and discovered the neutron in 1932 and received
    the Nobel prize in 1935.

24
Processes behind discovery
  • Hit a nucleus (Be-9) with an alpha particle
    emitted in the decay of Po. It is absorbed to
    form an unstable isotope which releases an excess
    neutron of high energy (6 MeV).
  • A neutron encountering hydrogen will eject
    protons which create detectable ionization.

25
Measuring recoil proton energies
  • Protons knock electrons from atoms thereby losing
    energy and eventually stop.
  • The amount of material required to stop them
    determines their energy.

http//dbhs.wvusd.k12.ca.us/Chem-History/Chadwick-
1932/Chadwick-neutron.html
26
The size of the nucleus
  • The protons and neutrons in a nucleus turn out to
    be close packed into a sphere. The electric field
    is not infinite but in fact goes to zero at the
    center. In scattering electrons from nuclei,
    those which penetrate the nucleus deviate from
    Rutherfords scattering model so are sensitive to
    the nuclear radius.
  • Cross check Neutrons interact only via short
    range (contact) nuclear forces so the probability
    of interaction in a sample is proportional to the
    number of nuclei and the cross sectional area of
    a nucleus.

27
Summary
  • The early part of the 20th century was a tumult
    of new discoveries relating to atomic matter.
  • The basic structure of the atom was established
    but much remained to be understood.
Write a Comment
User Comments (0)
About PowerShow.com