Showing posts with label #19. Show all posts
Showing posts with label #19. Show all posts

Nuclear & Particle Physics - Alpha/Rutherford Scattering

When alpha particles are directed onto atoms in a thin metal foil, some make very close collisions with the nuclei of the atoms and are scattered at large angles. If an alpha particles with an initial kinetic energy of 5 MeV happens to be scattered through an angle of 180o, which of the following must have been its distance of the closest approach to the scattering nucleus? (Assume that the metal foil is made of silver, with Z = 50.)

A. 1.22 × 501/3 fm
B. 2.9 × 10−14 m
C. 1.0 × 10−12 m
D. 3.0 × 10−8 m
E. 1.7 × 10−7 m
(GR9677 #19)
Solution:

"When alpha particles are directed onto atoms in a thin metal foil, some make very close collisions with the nuclei of the atoms and are scattered at large angles."→ Rutherford Scattering: the discovery of nucleus.

Rutherford estimated the radius of a silver nucleus to be 2 × 10−14 m, by observing the angular dependence of alpha-particle scattering (source).

Answer: B


Calculation:

Conservation of Energy: U = T

= kqα q/ T
=  kqα qT

Given:
= 5 MeV = 5 × 10eV
Z= 50 → qZα50e
Zα = 2 → qα Zα2

= 1/4πɛ0 = 1/(4 × 3.14 × 8.85 × 10−12)  ≈ 1010  Nm2/C2

= (1010 Nm2/C2× 50e × 2e) / (× 10eV)
= 2 × 10Nm2/VC

With e = 1.60 × 10−19 C
1 Volt = 1 Nm/C

= 2 × 10× 1.60 × 1019 m ≈ 3 × 10−14 m


Classical Mechanics - Gravitation

Which of the following is most nearly the mass of the Earth? (The radius of the Earth is about 6.4 × 10m)

A. 6 × 1024 kg
B. 6 × 1027 kg
C. 6 × 1030 kg
D. 6 × 1033 kg
E. 6 × 1036 kg
(GR9277 #19)
Solution:

F =  mg = GMm/r2
Mgr2/G
M = 9.8 × (6.4 × 106)/ (6.67 × 10−11)
≈ 10 × 6 × 1012+11  
= 6 × 1024

Answer: A

Nuclear & Particle Physics - Hydrogen

The energy levels of the hydrogen atom are given in terms of the principal quantum number n and a positive constant A by the expression 

A. A(+ ½)
B. A(1 − n²)
C. A(¼ + 1/n)
D. An²
E. −A/n²
(GR8677 #19 )
Solution:

Energy level of hydrogen atom: En = −13.6/n² eV

Answer: E

Nuclear & Particle Physics - The Sun’s Energy

The primary source of the sun’s energy is a series of thermonuclear reactions in which the energy produces is c2 times the mass difference between

A. two hydrogen atoms and one helium atom
B. four hydrogen atoms and one helium atom
C. six hydrogen atoms and two helium atoms
D. three helium atoms and one carbon atom
E. two hydrogen atoms plus two helium atoms and one carbon atom
(GR0177 #19)
Solution:

In the Sun’s core, the protons of the hydrogen atoms (which largely make up the Sun) collide into each other and stick together or “fuse” to create helium nuclei.

4H → He + energy

It takes 4H nuclei to create a He nucleus due to the conservation of atomic mass.

Hydrogen atomic mass = 1 proton = 1.
Helium atomic mass = 2 protons + 2 neutrons = 4.

Answer: B