COSMOLOGICAL PRINCIPLE
|
|
- Oliver Griffin
- 5 years ago
- Views:
Transcription
1 THE BIG BANG
2 COSMOLOGICAL PRINCIPLE According to cosmological principle, the universe is homogeneous and isotropic (Looks same in all directions) When you look up at night, your line of sight must eventually encounter a star. Olbers s Paradox If homogeneous and isotropic entire night sky should be as bright as the sun.
3 COSMOLOGICAL PRINCIPLE Then, if not, which it is homogeneous and isotropic (the light hasn t got here, yet), or it is not homogeneous and isotropic, you must assume that one or both of the following statements is wrong or false. The universe is infinite in extent, because the light hasn t gotten here yet or It is unchanging in time.
4 COSMOLOGICAL PRINCIPLE So, because the sky is still dark at night or the night sky is still black, then: The universe must be either finite, or Evolves over time, or both.
5 FUZZY OBJECTS In the mid 1750 s, a Frenchman named Charles Messier started observing fuzzy patches in the night sky that he thought where comets. They where not. They turned out to be what he called nebula. A nebula is a general term used for any fuzzy patch on the sky, either light or dark. He named them M 1, M 2, M 54, M 105, ect. Edmund Hubble started looking at these nebula and saw galaxies.
6 AN OBSERVED REDSHIFT There was already observational evidence in support of an expanding universe. In 1912, American astronomer Vesto Slipher observed a spiral galaxy (considered a "spiral nebula" at the time, since astronomers didn't yet know that there were galaxies beyond the Milky Way) and recorded its redshift. He observed that all such nebula were traveling away from the Earth. The problem was that these results were quite controversial at the time and the full implications of them were not considered.
7 EARLY EXPANDING UNIVERSE FINDINGS In 1922, Russian cosmologist & mathematician Alexander Friedman found that solutions to Einstein's general relativity field equations resulted in an expanding universe. As a believer in a static, eternal universe, Einstein added a cosmological constant to his equations, "correcting" for this "error" and thus eliminating the expansion. He would later call this the biggest blunder of his life".
8 GALAXIES In 1924, astronomer Edwin Hubble was able to measure the distance to these "nebula" and discovered that they were so far away that they were not actually part of the Milky Way... He had discovered that the Milky Way was only one of many galaxies, and that these "nebulae" were actually galaxies in their own right.
9 GEORGES LEMAITRE In 1927, Roman Catholic priest and physicist Georges Lemaitre independently calculated the Friedman solution and again suggested that the universe must be expanding. This theory was supported by Hubble when, in 1929, he found that there was a correlation between the distance of the galaxies and the amount of redshift in that galaxy's light. The distant galaxies were moving away faster, which was exactly what was predicted by Lemaitre's solutions.
10 GALAXIES PICTURES In 1929, Edmund Hubble developed Hubble s Law and took pictures of galaxies, measuring the speeds of each. Knowing speed, in the equation of speed, speed = distance/time, and solving for time, so, time = distance/speed, you can bring all galaxies back to a single point.
11 GEORGES LEMAITRE In 1931, Lemaitre went further with his predictions, extrapolating backwards in time, he finds that the matter of the universe would reach an infinite density and temperature at a finite time in the past. This means the universe must have begun in an incredibly small, dense point of matter - a "primeval atom."
12 PHILOSOPHICAL SIDE NOTE The fact that Lemaitre was a Roman Catholic priest concerned some, as he was putting forth a theory which presented a definite moment of "creation" to the universe. In the 20's & 30's, most physicists - like Einstein - were inclined to believe that the universe had indeed always existed. That it was steady. In essence, the Big Bang theory was seen as "too religious" by many people.
13 AGE OF THE UNIVERSE Since Hubble s constant is not precise the best guess is the universe is between 10 and 20 billion years old. Most astronomers predict between 10 and 14 billion years. Most Astronomers believe the universe came from a gigantic explosion of pure energy.
14 AGE OF THE UNIVERSE The big bang represented the beginning of the entire universe mass, energy, space, and time came into being at that instant. Theorists estimate the known Physics of today is adequate to describe the universe since 1 X seconds after the Big Bang. Close enough to the original time, until the summer of 2012.
15 SIR FRED HOYLE The term, the Big Bang, was coined by the English astrophysicist Fred Hoyle in Hoyle, who championed a rival cosmological theory, despite popularising the theory by giving it a name, challenged the belief that the cosmos was caused by a huge explosion 12,000 million years ago. He advocated the "steady state" theory - that the cosmos had no beginning but new galaxies were formed as others moved apart. Hoyle meant the "Big Bang" to be a term of derision, but the name was so catchy that it stuck.
16 CONCERNS REMAINED One of these was the problem of homogeneity. Why does the universe look identical, in terms of energy, regardless of which direction one looks? The Big Bang theory does not give the early universe time to reach thermal equilibrium, so there should be differences in energy throughout the universe.
17 COSMIC MICROWAVE BACKGROUND RADIATION The accidental discovery of cosmic microwave background radiation is a major development in modern physical cosmology. Although predicted by earlier theories, it was first found accidentally by Arno Penzias and Robert Woodrow Wilson as they experimented with the Holmdel Horn Antenna.
18 COSMIC MICROWAVE BACKGROUND RADIATION After thoroughly checking their equipment, removing some pigeons nesting in the antenna and cleaning out the accumulated droppings, the noise remained. Both concluded that this noise was coming from outside our own galaxy although they were not aware of any radio source that would account for it.
19 COSMIC MICROWAVE BACKGROUND RADIATION At that same time, Robert H. Dicke, Jim Peebles, and David Wilkinson, astrophysicists at Princeton University just 37 miles away, were preparing to search for microwave radiation in this region of the spectrum. Dicke and his colleagues reasoned that the Big Bang must have scattered not only the matter that condensed into galaxies but also must have released a tremendous blast of radiation. With the proper instrumentation, this radiation should be detectable.
20 COSMIC MICROWAVE BACKGROUND RADIATION When a friend told Penzias about a preprint paper he had seen by Jim Peebles on the possibility of finding radiation left over from an explosion that filled the universe at the beginning of its existence, Penzias and Wilson began to realize the significance of their discovery. The characteristics of the radiation detected by Penzias and Wilson fit exactly the radiation predicted by Robert H. Dicke and his colleagues at Princeton University.
21 COSMIC MICROWAVE BACKGROUND RADIATION The discovery was evidence for an expanding universe, (Big Bang Theory) and was evidence against the steady state model. In 1978, Penzias and Wilson were awarded the Nobel Prize for Physics for their joint discovery.
22 STEPHEN HAWKING SINGULARITY THEORY The work of Stephen Hawking proposed that the universe acted like an exploding star, a supernova. A singularity in solutions of the Einstein field equations is one of two things: a. a situation where matter is forced to be compressed to a point (a space-like singularity) b. a situation where certain light rays come from a region with infinite curvature (time-like singularity)
23 STEPHEN HAWKING SINGULARITY THEORY Hawking and his Cambridge friend and colleague, Roger Penrose, showed in 1970 that if the universe obeys general relativity and fits any of the Friedmann models, then it must have begun as a singularity. Remember, Friedmann was the Russian scientisits who used Einstein s equations to predict an explanding universe.
24 HEAT SIGNATURE Evidence collected by the COBE satellite between 1990 to 1992, showed that the universe was not an even temperature, but has hot spots that eventually became the galaxies. The cosmic microwave background radiation is a remnant of the Big Bang and the fluctuations are the imprint of density contrast in the early universe.
25 EXISTING CONTROVERSIES While the Big Bang theory is accepted by the vast majority of physicists, there are still some minor questions concerning it. Most importantly, however, are the questions which the theory cannot even attempt to answer.
26 EXISTING CONTROVERSIES What existed before the Big Bang? What caused the Big Bang? Is our universe the only one? The answers to these questions may well exist in String Theory...\..\..\..\Videos\Michio Kaku Explains String Theory_(360p).avi
27 THE GOD PARTICLE The Higgs boson, Higgs particle, or the God particle, is a proposed elementary particle in the Standard Model of particle physics. The Higgs boson's existence would have profound importance in particle physics because it would prove the existence of the hypothetical Higgs field and the means by which elementary particles acquire mass...\..\..\..\videos\angels and Demons - The God Particle_(360p).avi
28 THE GOD PARTICLE The Higgs boson is named for Peter Higgs who, along with two other teams, proposed the mechanism that suggested such a particle in On 4 July 2012, the CMS and the ATLAS experimental teams at the Large Hadron Collider independently announced that they each confirmed the formal discovery of a previously unknown boson of mass between GeV/c 2.
29 THE GOD PARTICLE The particle s behavior so far has been "consistent with" a Higgs boson. Proof of the Higgs field (by observing the associated particle), and evidence of its properties, is likely to greatly affect human understanding of the universe.
30 THE GOD PARTICLE This announcement means that observations show the newly discovered boson could be a Higgs boson, and it is widely believed by scientists to be very likely a Higgs boson, but further study of this particle, now that its existence is proven, will still be required to place beyond doubt the question whether the particle is in fact confirmed as a Higgs boson...\..\..\..\videos\scientists confirm 'God Particle' exists_(360p).avi
31 BIG BANG THEORY - WHAT ABOUT GOD? Any discussion of the Big Bang theory would be incomplete without asking the question, what about God? This is because cosmogony (the study of the origin of the universe) is an area where science and theology meet. Creation was a supernatural event. That is, it took place outside of the natural realm.
32 BIG BANG THEORY - WHAT ABOUT GOD? This fact begs the question: is there anything else which exists outside of the natural realm? Specifically, is there a master Architect out there? We know that this universe had a beginning. Was God the "First Cause"?
33 MARK TWAIN There is something fascinating about science. One gets such a wholesale return of conjecture out of such a trifling investment of fact.
The expansion of the Universe, and the big bang
The expansion of the Universe, and the big bang Q: What is Hubble s law? A. The larger the galaxy, the faster it is moving way from us. B. The farther away the galaxy, the faster it is moving away from
More informationPHY1033C/HIS3931/IDH 3931 : Discovering Physics: The Universe and Humanity s Place in It Fall 2016
PHY1033C/HIS3931/IDH 3931 : Discovering Physics: The Universe and Humanity s Place in It Fall 2016 Online evaluations open Announcements Final Exam Thursday, 15 December, 10am - 12, noon In-class NPB 1002
More informationChapter 26: Cosmology
Chapter 26: Cosmology Cosmology means the study of the structure and evolution of the entire universe as a whole. First of all, we need to know whether the universe has changed with time, or if it has
More informationLecture Outlines. Chapter 26. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 26 Astronomy Today 8th Edition Chaisson/McMillan Chapter 26 Cosmology Units of Chapter 26 26.1 The Universe on the Largest Scales 26.2 The Expanding Universe 26.3 The Fate of the
More informationAstronomy 1 Winter Lecture 24; March
Astronomy 1 Winter 2011 Lecture 24; March 7 2011 Previously on Astro-1 Introduction to special relativity Introduction to general relativity Introduction to black holes, stellar and supermassive Today..
More informationBig Bang Theory PowerPoint
Big Bang Theory PowerPoint Name: # Period: 1 2 3 4 5 6 Recombination Photon Epoch Big Bang Nucleosynthesis Hadron Epoch Hadron Epoch Quark Epoch The Primordial Era Electroweak Epoch Inflationary Epoch
More informationAbstracts of Powerpoint Talks - newmanlib.ibri.org - The Cosmos. Robert C. Newman
The Cosmos Robert C. Newman The Cosmos Carl Sagan said: "The cosmos is all that is, or ever was, or ever will be." If Christianity is true, Sagan is mistaken. But we can perhaps define the cosmos as "All
More informationThe Dawn of Time - II. A Cosmos is Born
The Dawn of Time - II. A Cosmos is Born Learning Objectives! Why does Olbers paradox show the Universe began?! How does Hubble s Law tell us the age of the Universe? If Hubble s Constant is large, is the
More informationAstronomy 162, Week 10 Cosmology Patrick S. Osmer Spring, 2006
Astronomy 162, Week 10 Cosmology Patrick S. Osmer Spring, 2006 Information Makeup quiz Wednesday, May 31, 5-6PM, Planetarium Review Session, Monday, June 5 6PM, Planetarium Cosmology Study of the universe
More informationThe Big Bang Theory was first proposed in the late 1920 s. This singularity was incredibly dense and hot.
The Big Bang Theory was first proposed in the late 1920 s. It states that there was an infinitely small, infinitely dense point that contained everything that is the universe. This singularity was incredibly
More informationCosmology: The History of the Universe
Cosmology: The History of the Universe The Universe originated in an explosion called the Big Bang. Everything started out 13.7 billion years ago with zero size and infinite temperature. Since then, it
More informationFigure 19.19: HST photo called Hubble Deep Field.
19.3 Galaxies and the Universe Early civilizations thought that Earth was the center of the universe. In the sixteenth century, we became aware that Earth is a small planet orbiting a medium-sized star.
More informationThe Big Bang. Mr. Mike Partridge Earth & Space Science J.H. Reagan High School, Houston, TX
The Big Bang Mr. Mike Partridge Earth & Space Science J.H. Reagan High School, Houston, TX Notes Outlines Theories of the Universe Static Universe What is the Big Bang Theory What is the evidence supporting
More informationAstronomy 210 Final. Astronomy: The Big Picture. Outline
Astronomy 210 Final This Class (Lecture 40): The Big Bang Next Class: The end HW #11 Due next Weds. Final is May 10 th. Review session: May 6 th or May 9 th? Designed to be 2 hours long 1 st half is just
More informationUNIT 3 The Study of the. Universe. Chapter 7: The Night Sky. Chapter 8: Exploring Our Stellar Neighbourhood. Chapter 9:The Mysterious.
UNIT 3 The Study of the Universe Chapter 7: The Night Sky Chapter 8: Exploring Our Stellar Neighbourhood Chapter 9:The Mysterious Universe CHAPTER 9 The Mysterious Universe In this chapter, you will: identify
More informationCosmology. Thornton and Rex, Ch. 16
Cosmology Thornton and Rex, Ch. 16 Expansion of the Universe 1923 - Edwin Hubble resolved Andromeda Nebula into separate stars. 1929 - Hubble compared radial velocity versus distance for 18 nearest galaxies.
More informationAccording to the currents models of stellar life cycle, our sun will eventually become a. Chapter 34: Cosmology. Cosmology: How the Universe Works
Chapter 34: Cosmology According to the currents models of stellar life cycle, our sun will eventually become a a) Cloud of hydrogen gas b) Protostar c) Neutron star d) Black hole e) White dwarf id you
More informationCosmology. Stellar Parallax seen. The modern view of the universe
Cosmology The modern view of the universe SC/NATS 1730, XXVIIICosmology 1 Stellar Parallax Copernicus said stellar parallax couldn t be seen because the stars were so far away. A strictly ad hoc explanation
More informationThe Expanding Universe
Cosmology Expanding Universe History of the Universe Cosmic Background Radiation The Cosmological Principle Cosmology and General Relativity Dark Matter and Dark Energy Primitive Cosmology If the universe
More informationOlbers Paradox. Why is the sky dark? Possible answers:
Olbers Paradox Why is the sky dark? If the universe were infinitely big and infinitely old, there should be no dark patches in the sky (Heinrich Wilhelm Olbers (1757-- 1840) ) Possible answers: Dust? No,
More informationChapter 17 Cosmology
Chapter 17 Cosmology Over one thousand galaxies visible The Universe on the Largest Scales No evidence of structure on a scale larger than 200 Mpc On very large scales, the universe appears to be: Homogenous
More informationIsland Universes. Up to 1920 s, many thought that Milky Way encompassed entire universe.
Island Universes Up to 1920 s, many thought that Milky Way encompassed entire universe. Observed three types of nebulas (clouds): - diffuse, spiral, elliptical - many were faint, indistinct - originally
More information26. Cosmology. Significance of a dark night sky. The Universe Is Expanding
26. Cosmology Significance of a dark night sky The Universe is expanding The Big Bang initiated the expanding Universe Microwave radiation evidence of the Big Bang The Universe was initially hot & opaque
More informationCosmology. An Analogy 11/28/2010. Cosmology Study of the origin, evolution and future of the Universe
Cosmology Cosmology Study of the origin, evolution and future of the Universe Obler s Paradox If the Universe is infinite why is the sky dark at night? Newtonian Universe The Universe is infinite and unchanging
More informationCOSMOLOGY The Universe what is its age and origin?
COSMOLOGY The Universe what is its age and origin? REVIEW (SUMMARY) Oppenheimer Volkhoff limit: upper limit to mass of neutron star remnant more than 1.4 M à neutron degeneracy Supernova à extremely dense
More informationThe Big Bang Theory. Rachel Fludd and Matthijs Hoekstra
The Big Bang Theory Rachel Fludd and Matthijs Hoekstra Theories from Before the Big Bang came from a black hole from another universe? our universe is part of a multiverse? just random particles? The Big
More informationAstronomy 122 Outline
Astronomy 122 Outline This Class (Lecture 26): The Primeval Fireball Next Class: Dark Matter & Dark Energy ICES Form!!! HW10 due Friday Hubble s Law implications An expanding Universe! Run in movie in
More informationCH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence
CH 14 MODERN COSMOLOGY The Study of Nature, origin and evolution of the universe Does the Universe have a center and an edge? What is the evidence that the Universe began with a Big Bang? How has the Universe
More informationThe Big Bang. Olber s Paradox. Hubble s Law. Why is the night sky dark? The Universe is expanding and We cannot see an infinite Universe
The Big Bang Olber s Paradox Why is the night sky dark? The Universe is expanding and We cannot see an infinite Universe Hubble s Law v = H0 d v = recession velocity in km/sec d = distance in Mpc H 0 =
More informationAstronomy 150: Killer Skies Lecture 35, April 23
Assignments: ICES available online Astronomy 150: Killer Skies Lecture 35, April 23 HW11 due next Friday: last homework! note: lowest HW score dropped but: HW11 material will be on Exam 3, so be sure to
More informationDoppler Effect. Sound moving TOWARDS. Sound moving AWAY 9/22/2017. Occurs when the source of sound waves moves towards or away
Burkey- ESS QUIZ Thursday At the instant of the Big Bang, all the matter, energy, time, & space in the Universe was condensed into a single, tiny point. We call this Singularity. Doppler Effect Occurs
More informationImplications of the Hubble Law: - it is not static, unchanging - Universe had a beginning!! - could not have been expanding forever HUBBLE LAW:
Cosmology and the Evolution of the Universe Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -greater distance greater redshift Implications of the Hubble Law: - Universe is
More informationCosmology and the Evolution of the Universe. Implications of the Hubble Law: - Universe is changing (getting bigger!) - it is not static, unchanging
Cosmology and the Evolution of the Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -exceptions in Local Group -with distance measurements - found a relationship greater distance
More informationAn expanding cosmos The most important discovery in astronomy?
+ Portrait of Edwin Hubble, undated Credit: Perlmutter et al.,1998, Astrophysical Journal, vol. 516 An expanding cosmos The most important discovery in astronomy? Szydagis 03.28.2018 Mythbusters is owned
More informationAstro-2: History of the Universe
Astro-2: History of the Universe Lecture 7; May 2 2013 Previously on astro-2 A scientific theory is a logically self-consistent model or framework for describing the behavior of a related set of natural
More informationCosmology. What is Cosmology?
Cosmology What is Cosmology? The study of the structure and evolution of the entire universe The idea is to form picture of the entire Universe: origin, size, and future We will make assumptions that what
More information! Expansion of the Universe! Difference between expansion and explosion
This Class (Lecture 32): The Big Bang! Expansion of the Universe! Difference between expansion and explosion HW 11 due on Dec 5 th Music: The Universe Song Animaniacs! In a homogenous Universe, what does
More informationAstronomy 113. Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter. Olber s Paradox. Cosmology. Olber s Paradox. Assumptions 4/20/18
Astronomy 113 Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter Cosmology ³The study of the origins, structure, and evolution of the universe ³Key moments: ²Einstein General Theory of Relativity ²Hubble
More informationAstronomy 113. Dr. Joseph E. Pesce, Ph.D Joseph E. Pesce, Ph.D.
Astronomy 113 Dr. Joseph E. Pesce, Ph.D. The Big Bang & Matter 17-2 Cosmology ³ The study of the origins, structure, and evolution of the universe ³ Key moments: ² Einstein General Theory of Relativity
More informationLecture 22: The expanding Universe. Astronomy 111 Wednesday November 15, 2017
Lecture 22: The expanding Universe Astronomy 111 Wednesday November 15, 2017 Reminders Online homework #10 due Monday at 3pm Then one week off from homeworks Homework #11 is the last one The nature of
More informationo Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe
Standard 1: Students will understand the scientific evidence that supports theories that explain how the universe and the solar system developed. They will compare Earth to other objects in the solar system.
More informationAstronomy: The Big Picture. Outline. What does Hubble s Law mean?
Last Homework is due Friday 11:50 am Honor credit need to have those papers this week! Estimated grades are posted. Does not include HW 8 or Extra Credit THE FINAL IS DECEMBER 15 th : 7-10pm! Astronomy:
More informationFormation of the Universe. What evidence supports current scientific theory?
Formation of the Universe What evidence supports current scientific theory? Cosmology Cosmology is the study of the Nature, Structure, Origin, And fate of the universe. How did it all begin? Astronomers
More information9.2 The Universe. p. 368
9.2 The Universe p. 368 Cosmology the study of the universe, including its origin, how it is changing, and its future. The Hubble Space Telescope (HST) The American astronomer Edwin Hubble (1889-1953)
More informationLecture 37 Cosmology [not on exam] January 16b, 2014
1 Lecture 37 Cosmology [not on exam] January 16b, 2014 2 Structure of the Universe Does clustering of galaxies go on forever? Looked at very narrow regions of space to far distances. On large scales the
More informationA theory is An explanation that fits the facts.
A theory is An explanation that fits the facts. Needs to explain, or at least be consistent with all the characteristics and facts observed. Needs to also be consistent with what we know about the rest
More informationi>clicker Quiz #14 Which of the following statements is TRUE?
i>clicker Quiz #14 Which of the following statements is TRUE? A. Hubble s discovery that most distant galaxies are receding from us tells us that we are at the center of the Universe B. The Universe started
More informationASTR 200 : Lecture 27. Expansion and large scale structure
ASTR 200 : Lecture 27 Expansion and large scale structure 1 A preference for recession In 1912, american astronomer Vesto Slipher began painstakingly acquiring spectra of `spiral nebulae' and was the first
More informationwhat scientist believe happened to form the universe, and it is called the Big Bang Theory.
Schjelderup 1 Ari Schjelderup David Schaffer PHYS-1040-009 10/30/11 The Big Bang Theory When I was a little girl I asked my mom how long god had been around. She told me he had been around forever. When
More informationv = H o d Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d):
Hubble s Law: Distant galaxies move away fastest Velocity (v) is proportional to Distance (d): v = H o d The Hubble Constant was measured after decades of observation: H 0 = 70 km/s/mpc Velocity (km/s)
More informationVU lecture Introduction to Particle Physics. Thomas Gajdosik, FI & VU. Big Bang (model)
Big Bang (model) What can be seen / measured? basically only light _ (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)
More informationIntroduction to Cosmology (in 5 lectures) Licia Verde
Introduction to Cosmology (in 5 lectures) Licia Verde http://icc.ub.edu/~liciaverde Program: Cosmology Introduction, Hubble law, Freedman- Robertson Walker metric Dark matter and large-scale cosmological
More informationOlbers Paradox. Lecture 14: Cosmology. Resolutions of Olbers paradox. Cosmic redshift
Lecture 14: Cosmology Olbers paradox Redshift and the expansion of the Universe The Cosmological Principle Ω and the curvature of space The Big Bang model Primordial nucleosynthesis The Cosmic Microwave
More informationCosmology. Chapter 18. Cosmology. Observations of the Universe. Observations of the Universe. Motion of Galaxies. Cosmology
Cosmology Chapter 18 Cosmology Cosmology is the study of the structure and evolution of the Universe as a whole How big is the Universe? What shape is it? How old is it? How did it form? What will happen
More informationAstronomy 114. Lecture35:TheBigBang. Martin D. Weinberg. UMass/Astronomy Department
Astronomy 114 Lecture35:TheBigBang Martin D. Weinberg weinberg@astro.umass.edu UMass/Astronomy Department A114: Lecture 35 09 May 2005 Read: Ch. 28,29 Astronomy 114 1/18 Announcements PS#8 due Monday!
More informationA brief history of cosmological ideas
A brief history of cosmological ideas Cosmology: Science concerned with the origin and evolution of the universe, using the laws of physics. Cosmological principle: Our place in the universe is not special
More informationthe evidence that the size of the observable Universe is changing;
Q1. Describe, in as much detail as you can: the evidence that the size of the observable Universe is changing; the evidence that, billions of years ago, all the matter in the Universe was tightly packed
More informationParadigm Shifts in Cosmology
FEATURE Principal Investigator Naoshi Sugiyama Research Area Astrophysics Paradigm Shifts in Cosmology The paradigm shift as put forward by Thomas Kuhn means revolutionary changes in the normative concepts
More informationAri Schjelderup David Schaffer PHYS /30/11 The Big Bang Theory
Schjelderup 1 Ari Schjelderup David Schaffer PHYS-1040-009 10/30/11 The Big Bang Theory When I was a little girl I asked my mom how long God had been around. She told me he had been around forever. When
More informationModule 3: Astronomy The Universe Topic 1 Content: Cosmology Presentation Notes
Pretend that you have been given the opportunity to travel through time to explore cosmology. Cosmology is the study of how the universe formed and what will happen to it. Watch through your viewport as
More informationThe Universe. Unit 3 covers the following framework standards: ES 8 and 12. Content was adapted the following:
Unit 3 The Universe Chapter 4 ~ The Formation of the Universe o Section 1 ~ The Scale of the Universe o Section 2 ~ The Formation of the Universe o Section 3 ~ The Future of the Universe Chapter 5 ~ Galaxies
More informationChapter 25: Beyond our Solar System The Universe pp
Chapter 25: Beyond our Solar System 25.3 The Universe pp 715-721 The Milky Way Galaxy On a clear and moonless night, away from city lights, you might see a a band of light in the sky. This band is The
More informationCosmology. Big Bang and Inflation
Cosmology Big Bang and Inflation What is the Universe? Everything we can know about is part of the universe. Everything we do know about is part of the universe. Everything! The Universe is expanding If
More information11/18/2008. General Theory of Relativity (1915) Cosmologists had decided that the universe was eternal (rather than created) Problem:
Cosmologists had decided that the universe was eternal (rather than created) General Theory of Relativity (1915) Problem: Gravitational attraction would cause the universe to collapse. 1 Solution: Addition
More informationTaking the Measure of the Universe. Gary Hinshaw University of British Columbia TRIUMF Saturday Series 24 November 2012
Taking the Measure of the Universe Gary Hinshaw University of British Columbia TRIUMF Saturday Series 24 November 2012 The Big Bang Theory What is wrong with this picture? The Big Bang Theory The Big bang
More informationTesting the Big Bang Idea
Reading: Chapter 29, Section 29.2-29.6 Third Exam: Tuesday, May 1 12:00-2:00 COURSE EVALUATIONS - please complete these online (recitation and lecture) Last time: Cosmology I - The Age of the & the Big
More informationBig Bang Theory How the Universe was Formed
Big Bang Theory How the Universe was Formed Objectives Explain the Big Bang Theory. Give evidence to support the Big Bang Theory. Dispel misconceptions about the Big Bang Theory. Explain problems with
More informationHow Did the Universe Begin?
How Did the Universe Begin? As we will discuss in this lecture, it looks like the Universe started about 14 billion years ago and has been expanding (space stretching) ever since. The model of what happened
More informationThe Big Bang: Fact or Fiction?
A new perspective on Einstein s universe The Big Bang: Fact or Fiction? Cormac O Raifeartaigh and Brendan Mcann (WIT) Werner Nahm (DIAS) and Simon Mitton (Univ. of Cambridge) Cosmology: the study of the
More informationCosmology II. Shape and Geometry of the Universe. Physics 113 Goderya. Back to our 2- dimensional analogy:
Cosmology II Physics 113 Goderya Chapter(s): 18 Learning Outcomes: The Cosmological Principle Considering the largest scales in the universe, we make the following fundamental assumptions: 1) Homogeneity:
More informationPhysics Nobel Prize 2006
Physics Nobel Prize 2006 Ghanashyam Date The Institute of Mathematical Sciences, Chennai http://www.imsc.res.in shyam@imsc.res.in Nov 4, 2006. Organization of the Talk Organization of the Talk Nobel Laureates
More informationIntroduction and Fundamental Observations
Notes for Cosmology course, fall 2005 Introduction and Fundamental Observations Prelude Cosmology is the study of the universe taken as a whole ruthless simplification necessary (e.g. homogeneity)! Cosmology
More informationBig Bang Theory. How did this theory develop, and what is the evidence for it?
Big Bang Theory Big Bang Theory Big bang theory suggests that the universe began from a single point about 13.82 billion years ago. What existed before this event is completely unknown to science, but
More informationAstronomy Hour Exam 2 March 10, 2011 QUESTION 1: The half-life of Ra 226 (radium) is 1600 years. If you started with a sample of 100 Ra 226
Astronomy 101.003 Hour Exam 2 March 10, 2011 QUESTION 1: The half-life of Ra 226 (radium) is 1600 years. If you started with a sample of 100 Ra 226 atoms, approximately how many Ra 226 atoms would be left
More informationCosmology: The Origin and Evolution of the Universe Chapter Twenty-Eight. Guiding Questions
Cosmology: The Origin and Evolution of the Universe Chapter Twenty-Eight Guiding Questions 1. What does the darkness of the night sky tell us about the nature of the universe? 2. As the universe expands,
More informationHow do we measure properties of a star? Today. Some Clicker Questions - #1. Some Clicker Questions - #1
Today Announcements: HW#8 due Friday 4/9 at 8:00 am. The size of the Universe (It s expanding!) The Big Bang Video on the Big Bang NOTE: I will take several questions on exam 3 and the final from the videos
More informationThe Formation of the Solar System
Earth and the Solar System The Formation of the Solar System Write a number beside each picture to rank each from the oldest (1) to the youngest (4). The universe includes everything that exists: all matter,
More informationModeling the Universe A Summary
Modeling the Universe A Summary Questions to Consider 1. What does the darkness of the night sky tell us about the nature of the universe? 2. As the universe expands, what, if anything, is it expanding
More informationStudying the universe
Studying the universe What is astronomy? A branch of science that deals with study of stars, planets, the universe as a whole The idea is that we live in a clockwork universe and is governed by laws that
More informationComplete Cosmos Chapter 24: Big Bang, Big Crunch Outline Sub-chapters
Complete Cosmos Chapter 24: Big Bang, Big Crunch Theory of the Big Bang. From that cataclysmic explosion, the Universe continues to expand. But will it stop and reverse? Outline How did the Universe begin?
More informationB. The blue images are a single BACKGROUND galaxy being lensed by the foreground cluster (yellow galaxies)
ASTR 1040 Accel Astro: Stars & Galaxies Today s s `Cosmological Events Look at models for our universe,, and what prompted ideas about big-bang bang beginnings Cosmic Microwave Background Simulation: Large-scale
More informationClass 5 Cosmology Large-Scale Structure of the Universe What do we see? Big Bang Cosmology What model explains what we see?
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System
More informationHubble's Law. H o = 71 km/s / Mpc. The further a galaxy is away, the faster it s moving away from us. V = H 0 D. Modern Data.
Cosmology Cosmology is the study of the origin and evolution of the Universe, addressing the grandest issues: How "big" is the Universe? Does it have an "edge"? What is its large-scale structure? How did
More informationAstronomy Introductory Online Activity Origins: Back to the Beginning
Astronomy Introductory Online Activity Origins: Back to the Beginning Astronomers point to an initial explosion called the Big Bang as the beginnings of our Universe. The PBS Television program Origins:
More informationIntroduction. How did the universe evolve to what it is today?
Cosmology 8 1 Introduction 8 2 Cosmology: science of the universe as a whole How did the universe evolve to what it is today? Based on four basic facts: The universe expands, is isotropic, and is homogeneous.
More informationMaking a Big Bang: Understanding the Observable Universe. Shane L. Larson Department of Physics Utah State University
Making a Big Bang: Understanding the Observable Universe Shane L. Larson Department of Physics Utah State University s.larson@usu.edu RMSGC Workshop USU Uintah Basin 24 June 2010 1 Storyline Time for some
More informationOverview DARK MATTER & DARK ENERGY. Dark Matter and Dark Energy I. Definition Current Understanding Detection Methods Cosmological Impact
DARK MATTER & DARK ENERGY Source: Max Ehrhardt Modiefied for Astronomy 101 Dark Matter and Dark Energy I Physics 113 Goderya Chapter(s): 18 Learning Outcomes: Overview Definition Current Understanding
More informationSpace and Time are the modes by which we think, not the conditions in which we live Albert Einstein
1 The dark Universe Andrew Taylor Space and Time are the modes by which we think, not the conditions in which we live Albert Einstein The only reason for time is so that everything doesn t happen at once
More informationThe first 400,000 years
The first 400,000 years All about the Big Bang Temperature Chronology of the Big Bang The Cosmic Microwave Background (CMB) The VERY early universe Our Evolving Universe 1 Temperature and the Big Bang
More informationthe evidence that the size of the observable Universe is changing;
Q. Describe, in as much detail as you can: the evidence that the size of the observable Universe is changing; the evidence that, billions of years ago, all the matter in the Universe was tightly packed
More informationHomework 6 Name: Due Date: June 9, 2008
Homework 6 Name: Due Date: June 9, 2008 1. Where in the universe does the general expansion occur? A) everywhere in the universe, including our local space upon Earth, the solar system, our galaxy and
More informationToday. Course Evaluations Open. Modern Cosmology. The Hot Big Bang. Age & Fate. Density and Geometry. Microwave Background
Today Modern Cosmology The Hot Big Bang Age & Fate Density and Geometry Microwave Background Course Evaluations Open Cosmology The study of the universe as a physical system Historically, people have always
More informationCosmology. Jörn Wilms Department of Physics University of Warwick.
Cosmology Jörn Wilms Department of Physics University of Warwick http://astro.uni-tuebingen.de/~wilms/teach/cosmo Contents 2 Old Cosmology Space and Time Friedmann Equations World Models Modern Cosmology
More informationPHYSICS FOR THE IB DIPLOMA CAMBRIDGE UNIVERSITY PRESS
Learning objectives Understand Hubble s law. Understand the scale factor and red-shift. Understand the cosmic microwave background radiation. Understand the accelerating universe and red-shift. D3 Cosmology
More informationHe doesn t really know what this indicates, just that it is a characteristic of most nebular which are really galaxies (He doesn t know that yet, not
1 His theory of general relativity says that when you measure length, time and mass, where you are matters. Your motion and thus these measurements are relative to other things. Everything is in motion,
More informationUnity in the Whole Structure
Cosmology II Unity in the Whole Structure How is it possible by any methods of observation yet known to the astronomer to learn anything about the universe as a whole? It is possible only because the universe,
More information13/01/2017. the. Big Bang. Friedmann, Lemaitre. Cosmic Expansion History
13/01/2017 the Big Bang Friedmann, Lemaitre & Cosmic Expansion History 1 Alexander Friedmann (1888 1925) George Lemaitre (1894 1966) They discovered (independently) theoretically the expansion of the Universe
More informationRocky Kolb Fermilab & University of Chicago. July 27, 2001 LP01 Rome
Rocky Kolb Fermilab & University of Chicago July 27, 2001 LP01 Rome A view of the universe, circa 1901 A.D. Kapteyn Universe 1) Composition: Starz in the hood 2) Arrangement: 6,500 light years Solar system
More informationCosmic Background, Euler s E Natural Logarithm and the Substratum
Cosmic Background, Euler s E Natural Logarithm and the Substratum By John Frederick Sweeney Abstract The Cosmic Microwave Background (CMB), rated at 2.7 degrees Kelvin, is nothing more than the activity
More informationEinstein s steady-state theory. The Big Bang: Fact or Fiction?
Einstein s steady-state theory An abandoned model of the universe The Big Bang: Fact or Fiction? Cormac O Raifeartaigh, Brendan Mcann (WIT) Werner Nahm (DIAS) and Simon Mitton (Univ. of Cambridge) Cosmology
More information