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AQA PHYS Paper 1
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Particle groups
Hadrons
Leptons
Leptons
Fundamental particles including
electron
, muon (heavy electron), and
neutrino
Lepton number
Leptons have a
lepton number
of 1, their antiparticles have a
lepton number
of -1
Types of neutrinos
Electron
neutrinos
Muon
neutrinos
Quark flavours
Up
Down
Strange
Strangeness
Strange quarks have strangeness
-1
, antistrange quarks have strangeness
+1
Baryon number
Baryons have a baryon number of
+1
or -1 if they contain
antiquarks
Neutrons
are up-down-down,
protons
are up-up-down
Electromagnetic force
Affects any
charged
particle, exchange particle is the
photon
Weak force
Affects any
particle
, exchange particles are W+, W-,
Z0 bosons
Strong force
Affects only hadrons, exchange particle is the
gluon
Electrostatic repulsion
and
strong force balance
to stabilise nuclei
Strong force range
4
fm, switches from attractive to repulsive at
0.5
fm
In any interaction,
charge
, baryon number and lepton number must be
conserved
Feynman diagrams
Represent weak interactions involving
W+/W-
bosons
In
beta minus decay
, a down quark in the
neutron
decays to an up quark, turning the neutron into a proton
Strangeness rules
Interactions involving
leptons
must be
weak
Interactions involving only
hadrons
and
conserving strangeness
must be strong
Interactions not
conserving strangeness
must be
weak
Charge to mass ratio
Charge in
coulombs
divided by mass in
kilograms
Types of radiation
Electromagnetic
(emitted by electrons)
Gamma
(emitted by nucleus)
Alpha
(emitted in radioactive decay)
Beta
(emitted in radioactive decay)
Heavier
nuclei are generally more unstable and likely to
decay
Alpha decay
1.
Nucleus
emits a
helium
nucleus (2 protons, 2 neutrons)
2
.
Daughter
nucleus has 2 fewer protons
Beta decay
1.
Neutron
in nucleus turns into
proton
, electron and antineutrino are emitted
2.
Daughter
nucleus has 1 more
proton
Electron-positron annihilation produces
2 photons
to
conserve momentum
Rest energy/mass energy
Energy =
mc^2
, can be converted to
photon
energy hf
Pair production
High energy photon
converts into
electron-positron
pair
Atomic energy levels
Electrons
orbit
nucleus
at discrete energy levels, can be excited to higher levels
Electron
de-excitation
Electron falls back to
lower
energy level, emitting
photon
Ionization
Electron can be excited to ionization level, leaving atom as
free
electron
Energy level units
Can be expressed in
joules
or
electron volts
(1 eV = 1.6x10^-19 J)
Emission spectrum
Shows
wavelengths
of photons emitted by an object, can identify its
composition
Absorption spectrum
Shows
wavelengths
absorbed by a gas or plasma, also identifies
composition
Fluorescent
tube
Electrons accelerated through
mercury
gas, emit
UV
which excites phosphor coating, emitting visible light
Wave-particle duality
Photons exhibit both wave and particle
properties
Photoelectric effect
Light shone on metal ejects electrons,
kinetic
energy depends on
frequency
not intensity
Work function
Minimum energy required to liberate an
electron
from a
metal
surface
Electron diffraction
Electrons exhibit
wave-like diffraction patterns
when fired at a target
de Broglie wavelength
Wavelength
of a particle = h/p, where h is Planck's constant and p is
momentum
Electricity
Flow of electric charge,
transfers
energy from source to
components
Lambda
Wavelength
of a particle
Faster speed
of a particle
Smaller
wavelength
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