NUCLEAR AND PARTICLE PHYSICS-5

Range-energy relationship for a-particle

Geiger Empirical relation R = aE3/2            E is in Mev,              R is in meter

    E = bR2/3                            a= 0.315 ´ 10-2,    b = 2.12 ´ 102

     The velocity vยตร–E       \v 3 ยต E 3/2      R = c v 3  where c has same value in all cases v 3 = 1.03 ´ 1027R

 Knowing R, one can calculate energy (E) or velocity (v) of a-particle emitted by the source. Geiger empirical relation is found to be applicable for a-particles having range 3 to 7 cms in air. R is found to be proportional to v3/2 for lower energies whereas for higher energies, it is proportional to v4 .

 

 Geiger-Nuttall law

Empirical relation between range R of a-particles and the decay constant l of the emitting nuclei known as Geiger-Nuttall law. Log l = A+B log R Where slope B is almost same but A has different values for different series





Theory of a-decay a-particle emission Potential energy of a nucleus and an a-particle as a function of their separation     U(r) = 2๐‘๐‘’2 /๐‘Ÿ

           For r = 3 ´ 10-12 cm, the potential energy is 9 Mev and increases to some maximum value for smaller values of r. This repulsive potential prevents a-particles from entering the nucleus and form a potential barrier. Close to the nucleus and inside, the coulomb potential must break down and be replaced by attractive potential.







The interaction between the nucleus and the a-particles in the region of uncertainty is represented by a constant attractive potential U0 exerted over a distance r0 called effective radius of the nucleus. To escape from the nucleus, the particle must have a kinetic energy at least as greater as the energy at the maximum of the potential energy curve. Similarly, the a- particle approaching nucleus from outside could penetrate only if it has enough energy to overcome the potential barrier.

The maximum value must be greater than 9 Mev since a-particles from Th C’ are scattered by uranium. Uranium nucleus emits a-particles with an energy of about 4 Mev. Classically it is difficult to understand the emission of a-particles from the nucleus.



ฮฒ particles and ฮฒ decay

                In ๐œท decay, a nucleus with (Z, A) emits a negatively charged electron and being transformed to Nucleus (Z+1, A). Fermi formulated the theory of ๐›ฝ decay using Pauli’s neutrino concept.

                                  n → p + ๐‘’ + ̅ฮฝe ;    ̅ฮฝe is anti-neutrino. The production of a positron emission (๐›ผ, ๐‘›) reaction has been demonstrated by Curie and Joliot.

 In ๐œท + decay, a proton bound in the nucleus converted to a bound neutron with the emission of positron and neutrino.

                p→ n + ๐‘’ + + ๐œ—๐‘’

      ๐›ฝ + decay:    AZX  AZ-1Y+ ๐›ฝ + + ๐œ—๐‘’

     ๐›ฝ decay: AZX  AZ+1Y+ ๐›ฝ + ̅ฮฝe

 Electron capture:  In the electron capture process, a Proton bound in the nucleus changes to a bound neutron by capturing one of the atomic electron (shortly from the K-shell) with an emission of a neutrino.

                p + e → n + ๐œ—๐‘’

            AZXN + e (๐›ฝ ) AZ-1YN+1 + ๐œ—๐‘’

K electrons are nearest to the nucleus and the probability of their being captured by Proton is large and hence the process is called K electron capture. The vacancy created by the K-shell is filled by the electrons from higher energy states i.e. L, M, N resulting in x-ray emission. The emitted electron in ๐›ฝ decay is not an orbital electron. The ๐›ฝ particle energy spectrum is a continuous spectrum extending from a minimum and attaining a maximum and then falls to zero at a certain energy called as endpoint energy.

 

 

 

 For beta emitters, the value of Emax varies from 0.25MeV to 2.15MeV.

   Pauli postulated a particle called antineutrino which is emitted in the electron emission process. It has (1) zero charges, (2) intrinsic spin -1/2, (3) zero rest mass.

In positron emission and electron capture, the particle emitted is neutrino which has (1) zero charges (2) intrinsic spin 1/2, and (3) zero rest mass.

Dirac's relativity theory shows that every particle with S = 1/2 spin has its antiparticle. The electron has its antiparticle positron, proton and anti-proton, neutron and antineutron.

     Neutrino ๐œ— has a spin ๐‘†๐œ— anti-parallel to its momentum ๐‘ƒ๐œ—.

Antineutrino ๐œ—̅  has a spin ๐‘†๐œ—̅ parallel to its momentum ๐‘ƒ๐œ—̅.

 Explanation: The continuous nature of the ๐›ฝ decay spectrum is unexpected because the beta transition connects two states of definite energy. Pauli proposed that in beta decay, ๐ธ๐›ฝ is the energy of the beta particle, ๐ธ0 is the end point energy, the energy associated with the neutrino is ๐ธ๐‘› = ๐ธ0 - ๐ธ๐›ฝ i.e. in each beta decay, the disintegration energy is shared in a continuous manner by ๐œ—, ๐›ฝ particle and the recoil nucleus.

 

 Based on Pauli's neutrino hypothesis, Fermi developed the theory for ๐›ฝ decay to obtain the continuous energy spectrum as well as decay constant for beta emission. Fermi postulated that the electron and antineutrino are created at the time of ๐›ฝ emission. The ๐›ฝ particle and neutrino belong to leptons. Leptons are defined by leptonic number 1 and for anti lepton it is –1.

 For nucleons (proton and neutron), l = 0

For electron and neutrino, l = 1

For positron and anti neutrino, l= -1

 ๐›ฝ decay:    n → p + ๐›ฝ + ๐œ—̅

                             l = 0    0   1    -1

๐›ฝ + decay:      p → n + ๐›ฝ + + ๐œ—

                  l = 0     0     -1      1

  EC process:

             p + ๐›ฝ → n + ๐œ—

          l = 0    1      0     1


 


 

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