The Big Bang Theory

Slides:



Advertisements
Similar presentations
Objectives: 1. relate the cosmological principle to isotropy and homgeneity of the universe. 2. understand how Hubble’s law is used to map the universe,
Advertisements

Major Epochs in the Early Universe t3x10 5 years: Universe matter dominated Why? Let R be the scale length.
The Expanding Universe!
Dec 10, 2003Astronomy 100 Fall 2003 Honor credit– need to have those papers this week! THE FINAL IS DECEMBER 15 th : 7-10pm! Today is last lecture with.
A Scientific History of the Universe. How do we predict the conditions of the early universe? What are the different eras in the early universe? What.
Chapter 17 The Beginning of Time
Chapter 17: The Birth of the Universe
The Big Bang Necessary? –Expansion of the Universe –Origin of CMBR 400 photons/cc Black body temperature profile –Helium content Universal nucleosynthesis.
ORIGIN OF THE UNIVERSE P In the beginning, God created the heaven and the earth; and the earth was without form and void; and darkness was upon the face.
Cosmology The Origin and Future of the Universe Part 2 From the Big Bang to Today.
The Big Bang Or… The Standard Model. Precepts of the standard model The laws of Physics are the same throughout the Universe. The Universe is expanding.
La teoria del big bang y la formacion del Universo.
Big Bang …..was actually very small and quiet. Atoms are mostly empty space.
Astronomy 100 Tuesday, Thursday 2:30 - 3:45 pm Tom Burbine
© 2010 Pearson Education, Inc. Chapter 23 The Beginning of Time.
Chapter 29 Exploring the Early Universe. Guiding Questions 1.Has the universe always expanded as it does today? 2.What is antimatter? How can it be created,
Background radiation (light) from Big Bang (visible) freely streaming from universe since atoms formed at temperature ~ 3,000 K (cf. sun = 6000 K)
Introductory Video: The Big Bang Theory Objectives  Understand the Hubble classification scheme of galaxies and describe the structure of the Milky.
Evolution of the Universe (continued)
The Big Bang Or… The Standard Model. Precepts of the standard model The laws of Physics are the same throughout the Universe. The Universe is expanding.
The Big Bang. CMBR Discussion Why can’t the CMBR be from a population of unresolved stars at high redshift?
Planets & Life PHYS 214 Dr Rob Thacker Dept of Physics (308A) Please start all class related s with “214:”
Particle Physics at the Energy Frontier Tevatron → LHC & The Very Early Universe Tony LissAir Force Institute of TechnologyApril 10, 2008.
Theory on the Formation of the Universe
Hubble’s Law Our goals for learning What is Hubble’s Law?
Exploring the Early Universe Chapter Twenty-Nine.
The Big Bang!. “To make an apple pie from scratch, you must first invent the universe” Carl Sagan 1980.
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
© 2010 Pearson Education, Inc. Chapter 23 The Beginning of Time.
Today: “Nucleosynthesis… another phase change in early universe… and why is the Universe so Flat?” HW for next time: Onion, “the nucleus and forces of.
BIG BANG TIMELINE FILL IN YOUR MISSING DATA. THE BIG BANG 0 to seconds Temperature- theorized to be infinite Infinitely small, Infinitely Dense,
The Professional Development Service for Teachers is funded by the Department of Education and Skills under the National Development Plan PARTICLE Physics.
In the Beginning 1)The Early Universe 2)SETI December 2, 2002 Final Exam will be held in Ruby Diamond Auditorium NOTE THIS!!! not UPL Dec. 11, am-noon.
A singularity formed by a previous collapsed Universe? Multiple Universes? We just don’t know… YET What Caused It?
Big Bang A Trip to the Beginning of the Universe by Stefan Diehl.
THE BIG BANG Theory… How did the universe begin?.
Chapter 17 The Beginning of Time. Running the Expansion Backward Temperature of the Universe from the Big Bang to the present (10 10 years ~ 3 x
CO-The Big Bang Theory LO-Describe the events leading to the formation of the Universe. 1.
The Beginning of Time: Evidence for the Big Bang & the Theory of Inflation.
Goal: To understand the history of the universe especially the beginning Objectives: 1)To learn about the beginning of the Big bang! 2)To explore the Big.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
1 Cosmology HNRT 227 Chapter October 2015 Great Idea: The universe began billions of years ago in the big bang and it has been expanding ever since.
The Hot Big Bang Monday, November 17 Pick up corrected Problem Set 6 (average score = 84); Recitation 4:30 pm today, McPherson 4054.
The Big Bang. Big Bang Theory A well tested Scientific Theory Widely accepted by the Scientific Community It explains the development of the Universe.
The UniverseSection 3 Section 3: Origin of the Universe Preview Key Ideas Bellringer What Is the Universe? What Happened at the Beginning? Predicting the.
Universe Tenth Edition Chapter 26 Exploring the Early Universe Roger Freedman Robert Geller William Kaufmann III.
 Pinning down the date of creation with such precision is impressive, but we have gone much further. We have begun to piece together the whole history.
Discovering the Universe Eighth Edition Discovering the Universe Eighth Edition Neil F. Comins William J. Kaufmann III CHAPTER 18 Cosmology Cosmology.
Modern Theories of the Universe The final work EVA OPATŘILOVÁ 2015.
Lecture 24: The Epochs of the Universe Astronomy 1143 – Spring 2014.
Important Stuff (Section 3) The Final Exam is Monday, December 19, 1:30 pm – 3:30 pm The Final Exam room is Physics 150 Bring 2 pencils and a photo-id.
After the Big Bang. ENERGY & MASS The infant Universe was searingly HOT! It was full of energy of intense radiation. Albert Einstein’s equation E=mc2.
The Big Bang Theory.
The Standard Model of Particle Physics
Chapter 23 The Beginning of Time
Chapter 22: The Birth of the Universe
It is the study of MATTER and the changes it undergoes.
Astrophysics II: Cosmology
Alternative to Big Bang theory: Steady State Cosmology
Universe! Early Universe.
Big Bang: timeline.
The Big Bang Model The most widely accepted theory TODAY on the formation of the universe  …Subject to change!
The Beginning of Time (Birth Of The Universe)
Cosmology Chapter 15 Great Idea:
Early Universe.
Did someone monkey with the laws of nature ? Unit 1.1
The Big Bang Theory.
Frontiers of fundamental physics
Early Universe.
Origin of Universe - Big Bang
Presentation transcript:

The Big Bang Theory

The big bang theory describes the development of the universe from the time just after it came into existence up to today. It's one of several scientific models that attempts to explain why the universe is the way it is. It is the most widely accepted and popular theory to explain the origin of the universe. The Big Bang Theory

While many people believe that the Big Bang theory refers to an explosion, it actually refers to the expansion of the universe.

E = mc² Developed by Albert Einstein Defined mass as highly concentrated energy with c being the speed of light. With high enough concentrations of energy, that energy can form matter.

Uh oh…Antimatter! When matter and anitmatter come into contact, they annihilate each other. The existence of antimatter was first predicted by Paul Direc.

The Big Bang Timeline

Planck Epoch Time: 0 to seconds after the Big Bang. Temperature: Kelvin Size: about meters At this point in the Big Bang timeline, gravity separates from the other forces.

Grand Unification Epoch Time: to seconds after the Big Bang. Temperature: Kelvin Size: about meters Strong force separates from the weak force and electromagnetic force. (Gravity is the fourth fundamental force) Important: It was at this point that more matter was created than antimatter.

Electroweak Epoch Time: to seconds after the Big Bang. Temperature: Kelvin Size: about meters Huge expansion in the beginning of this epoch. Weak force separates from the electromagnetic force, establishing the 4 fundamental forces we have today: Gravity, Strong, Weak, Electromagnetic

Quark Epoch Time: to seconds after the Big Bang. Temperature: Kelvin Size: unknown Quarks combine to make protons.

Hadron Epoch Time: to 1 second after the Big Bang. (FINALLY, 1 SECOND!!) Temperature: Kelvin Size: unknown Existence of antimatter are cancelled out

Lepton Epoch Time: 1 second to 3 minutes after the Big Bang Temperature: 10 9 Kelvin Size: unknown Formation of hydrogen and helium starts to occur.

Epoch of Nucleosynthesis Time: 3 minutes to 300,000 years after Big Bang Temperature: 3000 Kelvin Size: unknown After 3 minutes, the universe consists of 75% hydrogen, 25% helium, and traces of lithium, boron, and beryllium. After 300,000 years, light in the form of radio and microwaves now exist.

Big Bang Visual You and your lab partner will be making a visual of the big bang and all the epochs. This visual can be a timeline, story, book, poster, advertisement, or whatever else you can think of but it must include: 1.Each Big Bang Epoch clearly labeled and the significant event that occurred in each 2.A picture to represent each Epoch 3.You must include times, sizes, or temps 4.Creativity!!! Each person/group will share their visual