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Integration in physics

N uclear Physics

Rutherford’s experiment

Rutherford found that the nucleus is tens of thousands of times smaller in radius than the atom itself;

Experiments show that we can model a nucleus as a sphere with a radius R that depends on the total number of nucleons (neutrons and protons) in the nucleus.

Size of the nucleus

  • The neutrons and protons are grouped together in the nucleus, which is at the center of the atom;

  • If the atom were the size of your classroom, the nucleus would be the size of a single grain of sand at the center of the room;

  • Most of an atom’s mass is concentrated in the nucleus.

  • The radius of most nuclei obeys the empirical equation , where =1.2 fm or 1.2 × 10-15 m

Isotops

  • Atoms of the same element that have the same number of protons (Z) but a different number of neutrons (N) or A are known as ISOTOPES.

  • These have similar chemical properties, because the number of protons in the nucleus equals the number of electrons in the shells.

The atomic mass

  • Because the atomic masses are so small, the (unified) atomic mass unit (u or amu) is used instead of the kg;

  • 1 u = 1.660538921(73) × 10-27 kg or 931.494 MeV/c2 is defined as 1/12 of the mass of one atom.

Particle Type

Mass [kg]

Mass [u]

Mass [MeV/c2]

Electron

9.109 × 10-31

0.000549

0.511

Neutron

1.675 × 10-27

1.008665

939.6

Proton

1.673 × 10-27

1.007277

938.3

Hydrogen

1.674 × 10-27

1.007825

938.9

Carbon-12

1.993 × 10-26

12.00000

11 177.9

The Strong Nuclear Force

  • It has been shown experimentally that a strong nuclear force acts on all nucleons and it is nearly independent of charge. Electrons do not “feel” this force;

  • Holds protons and neutrons together in a nucleus;

  • Mostly attractive, and it can exceed the Coulomb repulsive force;

  • Short-range force, as it acts over distances comparable to the nucleus size.

T he Strong Nuclear Force Range

Attractive in the range: 1 to 5 fm, but repulsive below ~1 fm (= 10-15 m)

Nuclear Stability

  • Light nuclei (Z < ~20) are most stable if they contain equal numbers of protons and neutrons (i.e. N = Z);

  • N > Z in heavy nuclei (Z > ~20);

  • As the number of protons increases the electrostatic repulsion among them increases, too, and so more neutrons are required to increase the attractive nuclear force among the nucleons;

  • Eventually the Coulomb repulsive force prevails and no stable nuclei exist for Z >83.

Radioactivity

1 Bq = 1 decay/s

1 Ci = 3.7 × 1010 Bq

The spontaneous disintegration of certain atomic nuclei accompanied by the emission of the three main types of radiation: alpha particles, beta particles or gamma rays

There are 3 (main or historical) types of nuclear radiation:

  1. alpha (α) decay ( both Z and A change):

  1. beta () decay ( , , Z changes, A stays the same):

  1. gamma (γ) decay (high-energy photon emission, A and Z do not change):

Other types of radiation

  1. Beta (-) decay

  1. Beta (+) decay

Note : the neutrino and its antiparticle have no charge or mass, but have spin and kinetic energy

The Math of Radioactivity

  • Radioactivity appears to be a random process;

  • The decay rate is proportional to the number of unstable nuclei in a sample:

Show that:

The decay constant 𝛌 ) is positive and indicates how fast the radioactive material decays.

- initial number of radioactive nuclei

The positive rate of decay is also called activity (measured in Bq or Ci):

with - initial activity.

Half-life of radioactive decay

The half-life, , of a radioactive substance is the time it takes for half of a given number of its nuclei to decay:

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