Week 2 - Structure of the Atom Flashcards

1
Q

The Atom

A
  • Everything is made of atoms

Contains
o Nucleus
 Protons (+ charge)
 Neutrons (no charge)

o Electrons orbiting the nucleus (Bohr model of atom)
 -ve charge
 1/1840 mass of a proton (neutron)

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2
Q

Ernest Rutherford

A

Shot alpha particles at gold foil
o Discovered some passed through, while some scattered back at very sharp angles
o Therefore, hypothesising that there was something large within the atom (nucleus)

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3
Q

Ernest Rutherford: Model Problems

A
  • Explained some observations
  • Orbiting charged particles on a circular trajectory should radiate electromagnetic energy (lose energy)
    o Should therefore, spiral towards the nucleus
    o However, this is not what was observed
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4
Q

Neils Bohr

A
  • Uses basic concepts of the Rutherford model

- Postulated new rules for orbiting electrons

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5
Q

Neils Bohr Model of the Atom

A
  • Electrons orbit the nucleus at a fixed radii (i.e. in defined shells)
  • Electrons do not radiate energy but their energy is fused and determined by shell number (and charge in nucleus)
  • Electrons can make transitions from one level to another
    o And emit or absorb the energy difference
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6
Q

Uniqueness of Atomic Elements

A
  • Each atomic element has a unique number of protons, neutrons and electrons
  • Unique set of electron orbital radii and energies
  • Electron making transition between energy levels will emit or absorb electromagnetic radiation with a unique wavelength and energy
  • Atomic signature
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7
Q

Characterising Atoms

A

Atomic Number
- Number of protons in the nucleus

Mass Number
- Total number of protons and neutrons in the nucleus

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8
Q

Isotopes

A

o Same number of protons

o Different number of neutrons

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9
Q

Electrons

A
  • In a neutral atom the number of electron equals the number of protons
  • Atomic number = proton + electron
  • Electrons exist in discrete orbitals or shells and energy levels
  • As atomic number increases (number of electrons increase)
  • Inner electron shells fill first
  • Each shell can hold a maximum number of electrons
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10
Q

Electron Shells

A

K Shell has the greatest energy

Closest to +ve nucleus

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11
Q

Electron Transitions

A

If an electron is forcibly removed from an inner shell
o Electron from outer shell will make the transition to inner shell

o Electromagnetic wave is them emitted
 Visible light
 Ultraviolet
 X-rays

o Wavelength of EM wave depends on difference between energy levels

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12
Q

Electron Binding Energy: Definition

A
  • Amount of energy required to completely remove the electron from the atom
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13
Q

Electron Binding Energy

A
  • After removal of electron –> atom becomes ionised (+ve charge)
  • The process of removing an electron is called ionisation
    o Electron must be bound to the atom initially
    o Must be free from the atom after the process
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14
Q

Transition of Electron to Another Shell

A
  • Excitation
  • Fluorescence
    o If energy is not high enough to cause ionisation, electron just changes levels
    o Emission is determined by energy levels
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15
Q

What Determines Electron Binding Energy?

A
  • The number of protons in the nucleus
    o e.g., more protons = more +ve charge (electrons will be more tightly bound)
  • The proximity of an electron to the nucleus (the orbit or shell it sits in)
  • An electron in a particular shell in a particular atom will always have the same binding energy
  • Binding energy of electron depends on the atomic number and shell
    o Tungsten (atomic number = 74)
     K-Shell binding energy is always 69.5 keV
     L-Shell binding energy is always 10.2 keV
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16
Q

Atomic Balance and Creation of Ions

A
  • Atoms can lose electrons
    o Becomes +ve charged (cation)
  • Atom can gain electrons
    o Becomes -ve charged (anion)
  • Atoms are generally neutrally balanced
    o Protons = Electrons
17
Q

Isotopes

A
  • Nuclei which contain the same number of protons but different number of neutrons are known as isotopes
18
Q

Electrostatic Repulsive Force

A
  • Protons repel each other –> electrostatic repulsion due to magnetic field
19
Q

Strong Nucleus Force

A
  • Gravitational force between nucleon masses is too weak to overcome the electrostatic repulsive force
  • Attractive force between nucleons (proton-proton, neutron-neutron, neutron-proton)
  • Has a very short range (10^-15) (100 times larger than electrostatic repulsive force)
  • At longer distance – insignificant
  • Effectively only acts between neighbouring nucleons
  • Allows nuclei to be stable
20
Q

Stable-Unstable Nuclei

A
  • Strong force is able to balance out the repulsive force
  • As number of protons increase –> more neutrons are required to counterbalance the repulsive force between protons (maintain stability)
  • Balancing of repulsive and attractive forces is no longer possible by adding more neutrons
    o Limited Range of Strong Force (10^-15m)
21
Q

Bismuth

A
  • For Z > 83 a nucleus is unstable
  • Nuclei spontaneously break apart or rearrange their internal structure
    o Known as Radioactivity