Things You should Know Gravity Light Thermodynamics Atoms Particles.

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Presentation transcript:

Things You should Know Gravity Light Thermodynamics Atoms Particles

Gravity With Relativity Gravity is not action at a distance, but objects responding to the curvature of Space and Time in their immediate neighborhood Kepler’s Laws are valid for almost all gravitationally bound systems. The centre around which things orbit is the centre of mass of the system.

Rubber Sheet Gravity

Gravitational Light Bending

Space-time Diagram

World lines

Acceleration as Space time curve

Paths in Space-time

Orbits around Centre of Mass

Atoms Electrons orbit nucleus ( Protons and Neutrons) Held together by attraction of opposite electrical charge Possible energies described by spectrum Electrons can change energies by either absorbing or emitting light

Atomic Dimensions

States of an Atom

Atomic Energy Levels (Spectra)

Atomic Number and Isotopes

Isotopes

Light Wave-Particle Duality Frequency, Energy and Wavelength are all related Different types of light described by electromagnetic spectrum Stars have an absorption spectrum : Light from hot surface (continuous) Minus light absorbed by gas in atmospheres (the star’s and Earth’s)

Light as an Electro-Magnetic Wave

E&M Spectrum

Electromagnetic Spectrum

Atmospheric absorption

Inverse Square Law for light intensity

The Photo-electric effect

The Light Spectrum of an Atom

The Light Spectrum of a Celestial Object

The Spectrum of Mars

Kirchoff’s Laws

Shifting Spectral Lines

Broadening of Spectral Lines

Thermodynamics Heat is a form of energy manifested in random (thermal) motion of molecules Temperature determines the average heat energy per molecule Pressure is force per unit area which equals the average thermal energy per unit volume Density is the average number of molecules per unit volume Hot opaque objects emit light in a continuous spectrum called a Planck curve which depends only on temperature At low temperature matter clumps together, as you add heat it flies apart

Temperature Scales

Temperature as Molecule Energy

Ideal Gas Law

Blackbody Radiation – Planck Curves

Thermodynamic Behaviour of Matter

Phase Diagram for Water

Heat Transfer Conduction – Heat energy passed from molecule to molecule via contact (mostly in solids) Convection – Heated material rises, taking its heat with it (requires gravity and large temperature difference) Radiation – Heat transferred by emission and absorption of light

Conduction

Convect-1

Convect-2

Convect-3

Convection Thermal

Flotation

Particle Physics Four Forces (interactions): Gravity, Electromagnetism, Weak, Strong Gravity – Stars, Solar System, Galaxy, Universe E&M – Atoms, Molecules, Bricks Weak – can transform one type of fermion into another Strong – Protons, Neutrons, Nucleus Each force carried by a gauge boson, matter particles are called fermions (Quarks and Leptons) each fermion has rules for how it interacts with the Gauge Bosons

Particle Cookbook

The Four Interactions

Gauge Bosons

Properties of Gauge Bosons

Properties of the Interactions

Annihilation

Annihilation and Creation

Formation of Molecules

Fermions

Fermion Generations

Leptons

Quark Flavours

Hadrons – objects composed of Quarks

Binding of Nucleus

Quark Colours

Quark Confinement

Nucleons composed of Quarks

Schematic of the atom