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The Universe
(Observed and non-Observed constituents)
By
Halo Anwar
22 Feb 2017
Overview
• Structure of Universe
• Models explaining Universe
• Observed Universe
-Observational Overview
-Solar System
-Laws of Physics
• Non-Observed Universe
(Dark matter and Dark Energy)
Dark Energy
73%
Dark Matter
23%
“Normal Matter”
4%
Structure of Universe
Models explaining Universe
• Brahmanda (Cosmic Egg) Universe (15th -13th century B.C)
Indian
• Anaxagorian Universe (5th century B.C) Greek
• Atomic Universe – Democritus (5th century B.C) Greek
• Aristotelian Universe (4th century B.C) Greek
• Heliocentric Universe-Aristarchus (3rd century B.C) Greek
• Ptolemaic Universe(Geocentric) (2nd century A.D) Greek -
Egypt
• Abrahamic Universe-Christians, Muslims and Jewsh
6th – 11th Century A.D
• The Copernican (Heliocentric) Model – 1543 Polish
• Static (or Newtonian) Universe – 1687
• Einsteinian Universe – 1915
• Big Bang Model - Georges Lemaître 1927
• Oscillating Universe – 1930
• Steady State Universe - Fred Hoyle 1949
• Inflationary (or Inflating) Universe - Alan Guth 1980
• Multiverse -Andre Linde 1983
Ptolemaic Universe(Geocentric)
The Copernican Model
Big Bang Model
Oscillating Universe
Observed Universe ( 3000 MPc=9× 1025 𝑚)
(Observational Overview)
1. Visible Parts
• Stars; Nuclear fusion is source of star light
• Galaxies; ours is Milky way ( ̴1011
stars),
• Local group; small groups of galaxies, nearest galaxy from us
is Large Magellanic Cloud (LMC) 50 kpc away.
• Clusters of galaxies; superclusters and voids: larger groups of
galaxies on a scale 100 MPc
• Large-scale smoothness; above 100 MPc scale universe looks
smooth
2. Non-Visible parts
• Microwaves: the most important waveband for cosmology,
(1965 CMBR support for Big Bang accidental discovery)
• Radio waves: for high resolution maps of distant galaxies
• Infra red: spotting young galaxies,
• X-rays: clusters of galaxies;
3. Particles in the Universe
• Baryons: particles made up of three quarks except electron
• Mesons: quark and anti-quark, pion (𝜋)
• Photons: can interact with the baryons and electrons
• Neutrinos: extremely weakly interacting particles, radioactive
decay.
Solar System
Solar System
• Origin and evolution : (Condensation theory)
• Sun: Most of Solar mass (𝑀⨀ = 1.989 × 1030
𝑘𝑔)
• Planets:
-Terrestrial planets: (Mercury, Venus, Earth, Mars)
-Jovian Planets: (Jupiter, Saturn, Uranus, Nepton,
Pluto)
• Moons: Earth(1), Jupiter(67) biggest 4-Galileo
moons 1610, Mars(2), Saturn (62), Uranus (27),
Neptune (14), Pluto(5).
• Meteoroids (meteorite): bodies between planets
• Comets
• Dust and Gases
Laws of Physics
• Kepler’s Laws of Planetary Motion
• Hubble’s Law: v=hd
• Stellar Parallax: d=1/parallax angle
• Redshift:
𝑧 =
∆𝜆
𝜆
=
1+ 𝑣
𝑐
1− 𝑣
𝑐
− 1
Defines whether the galaxies moving toward or
away from us
z=0 fixed
Z=+ redshift (away)
z=- blueshift (toward)
Friedman Equations
• Density evolution equation (fluid equation)
𝜌 + 3
𝑎
𝑎
𝜌 +
𝑝
𝑐2
= 0
• Standard Friedman equation
𝑎 /𝑎 2
=
8𝜋𝐺
3
𝜌 −
𝑘𝑐2
𝑎2
• Acceleration equation
𝑎
𝑎
= −
4𝜋𝐺
3
𝜌 +
3𝑝
𝑐2
Einstein Field Equations:
• is Einstein tensor which describes the
geometry of spacetime, G is Newtonian constant.
• is stress-energy tensor which describes the
properties of matter.
• It is easy to notice that this equation is linking
geometry to matter as Einstein himself claims.
G
T
 RgRG
2
1

Non-Observed Universe
• 96% of Universe is unknown
1. Dark Energy 73%: responsible of accelerating
the expansion of the universe.
2. Dark Matter 23%: not interacting with
electromagnetics spectrum and with ordinary
matter, invisible, its existence inferred by its
effect such as gravitational lensing.
Thank you

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The universe

  • 1. The Universe (Observed and non-Observed constituents) By Halo Anwar 22 Feb 2017
  • 2. Overview • Structure of Universe • Models explaining Universe • Observed Universe -Observational Overview -Solar System -Laws of Physics • Non-Observed Universe (Dark matter and Dark Energy)
  • 3. Dark Energy 73% Dark Matter 23% “Normal Matter” 4% Structure of Universe
  • 4. Models explaining Universe • Brahmanda (Cosmic Egg) Universe (15th -13th century B.C) Indian • Anaxagorian Universe (5th century B.C) Greek • Atomic Universe – Democritus (5th century B.C) Greek • Aristotelian Universe (4th century B.C) Greek • Heliocentric Universe-Aristarchus (3rd century B.C) Greek • Ptolemaic Universe(Geocentric) (2nd century A.D) Greek - Egypt • Abrahamic Universe-Christians, Muslims and Jewsh 6th – 11th Century A.D • The Copernican (Heliocentric) Model – 1543 Polish
  • 5. • Static (or Newtonian) Universe – 1687 • Einsteinian Universe – 1915 • Big Bang Model - Georges Lemaître 1927 • Oscillating Universe – 1930 • Steady State Universe - Fred Hoyle 1949 • Inflationary (or Inflating) Universe - Alan Guth 1980 • Multiverse -Andre Linde 1983
  • 10. Observed Universe ( 3000 MPc=9× 1025 𝑚) (Observational Overview) 1. Visible Parts • Stars; Nuclear fusion is source of star light • Galaxies; ours is Milky way ( ̴1011 stars), • Local group; small groups of galaxies, nearest galaxy from us is Large Magellanic Cloud (LMC) 50 kpc away. • Clusters of galaxies; superclusters and voids: larger groups of galaxies on a scale 100 MPc • Large-scale smoothness; above 100 MPc scale universe looks smooth 2. Non-Visible parts • Microwaves: the most important waveband for cosmology, (1965 CMBR support for Big Bang accidental discovery)
  • 11. • Radio waves: for high resolution maps of distant galaxies • Infra red: spotting young galaxies, • X-rays: clusters of galaxies; 3. Particles in the Universe • Baryons: particles made up of three quarks except electron • Mesons: quark and anti-quark, pion (𝜋) • Photons: can interact with the baryons and electrons • Neutrinos: extremely weakly interacting particles, radioactive decay.
  • 13. Solar System • Origin and evolution : (Condensation theory) • Sun: Most of Solar mass (𝑀⨀ = 1.989 × 1030 𝑘𝑔) • Planets: -Terrestrial planets: (Mercury, Venus, Earth, Mars) -Jovian Planets: (Jupiter, Saturn, Uranus, Nepton, Pluto) • Moons: Earth(1), Jupiter(67) biggest 4-Galileo moons 1610, Mars(2), Saturn (62), Uranus (27), Neptune (14), Pluto(5). • Meteoroids (meteorite): bodies between planets • Comets • Dust and Gases
  • 14. Laws of Physics • Kepler’s Laws of Planetary Motion • Hubble’s Law: v=hd • Stellar Parallax: d=1/parallax angle
  • 15. • Redshift: 𝑧 = ∆𝜆 𝜆 = 1+ 𝑣 𝑐 1− 𝑣 𝑐 − 1 Defines whether the galaxies moving toward or away from us z=0 fixed Z=+ redshift (away) z=- blueshift (toward)
  • 16. Friedman Equations • Density evolution equation (fluid equation) 𝜌 + 3 𝑎 𝑎 𝜌 + 𝑝 𝑐2 = 0 • Standard Friedman equation 𝑎 /𝑎 2 = 8𝜋𝐺 3 𝜌 − 𝑘𝑐2 𝑎2 • Acceleration equation 𝑎 𝑎 = − 4𝜋𝐺 3 𝜌 + 3𝑝 𝑐2
  • 17. Einstein Field Equations: • is Einstein tensor which describes the geometry of spacetime, G is Newtonian constant. • is stress-energy tensor which describes the properties of matter. • It is easy to notice that this equation is linking geometry to matter as Einstein himself claims. G T  RgRG 2 1 
  • 18. Non-Observed Universe • 96% of Universe is unknown 1. Dark Energy 73%: responsible of accelerating the expansion of the universe. 2. Dark Matter 23%: not interacting with electromagnetics spectrum and with ordinary matter, invisible, its existence inferred by its effect such as gravitational lensing.