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The Atom and the Elements



Atoms are made up of:

  • nucleons \to protons (charge +e\bcth{+e}, mass 1u\approx1u)
\to neutrons (no charge, mass 1u\approx1u)

  • electrons (charge e\bcth{-e}, tiny mass)

where ee is the elementary charge:
 e=1.602×1019 C \boxed{ \ e=1.602\times10^{-19} \ C \ }


and uu is the atomic mass unit, defined to be one-twelfth of the mass of a Carbon atom:

 1 u=1.66×1027 kg \boxed{\ 1\ u=1.66\times10^{-27} \ kg \ }



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Atomic number: the number of protons in the nucleus, ZZ

Mass number: the number of protons and neutrons in the nucleus, AA


The chemical element XX is written as:
 ZAX \boxed{ \ _Z ^A X \ }


Isotopes are element varieties with the same number of protons, but different number of neutrons.

Example: hydrogen with its isotopes protium (1 proton), deuterium (1 proton and 1 neutron), tritium (1 proton and 2 neutrons)







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Nuclear Forces and Binding Energy

Protons are positively charged. But in the nucleus, they are forced to be close together. Like charges repel. So why does the nucleus stay together?

The strong nuclear force is responsible for holding the nucleus together! This force is much stronger than the repulsion between protons.


The binding energy is the energy needed to break a nucleus into its constituent protons and neutrons. It is also the energy that is released when protons and neutrons come together and form the nucleus.

The binding energy is given by the mass defect Δm\bcf {\Delta m}, which is the difference between the mass of the separated nucleons and the mass of the whole nucleus.


Wize Concept
  • The mass defect is always positive: a system of separated nucleons always has a greater mass than a system of bound nucleons.
  • When a nucleus forms, the mass defect is transformed into binding energy.
  • When a nucleus breaks apart, binding energy is transformed into mass.



Einstein's equation tells us how mass and energy can be converted into each other:
 E=Δmc2 \boxed{ \ E=\Delta mc^2 \ }
  • EE is energy (here, the binding energy)
  • Δm\Delta m is mass (here, the mass defect)
  • cc is the speed of light, 3×108 m/s3\times10^{8} \ m/s




When dealing with the energies of small particles, a more convenient unit for energy is the electron-volt (eVeV), which is the energy gained by an electron traveling through a potential difference of one volt:

 1 eV=1.602×1019J \boxed{\ 1\ eV=1.602\times10^{-19}J\ }

Fusion and Fission Reactors

This discovery leads to the application of both fusion and fission reactors. There are both energies released when atoms are combined together (lighter elements creating heavier elements) and when they are separated (heavier elements turning into lighter elements)
  • Nuclear Reactors use the energy created from these to heat up water which then turns into steam and the steam turns turbines thus producing energy!

Practice: Binding Energy per Nucleon


Find the binding energy per nucleon for 24He_2^4He and for  612C_{\ 6}^{12}C. Which nucleus is more stable?

mass of the proton: 1.0078 u1.0078 \ u
mass of the neutron: 1.00867 u1.00867 \ u
mass of the helium atom: 4.0026 u4.0026 \ u
mass of the carbon atom: 12.0107 u12.0107 \ u
(1 amu = 1.66x10-27kg)