Theory of relativity: Special Relativity and General Relativity

Slides:



Advertisements
Similar presentations
Newton’s Law of Universal Gravitation
Advertisements

Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
The Crisis of Classical Physics
Galileo simply described this as the fact that an observer in motion sees things differently from a stationary observer We use this as a part of our everyday.
Black Holes Dennis O’Malley. How is a Black Hole Created? A giant star (more than 25x the size of the sun) runs out of fuel –The outward pressure of the.
LIGO-G W Science: How the “facts” change Fred Raab LIGO Hanford Observatory.
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
GRAVITY.
Friday, October 24 Next planetarium show: Thurs, Nov. 6
Albert Einstein's Theory of General Relativity By: Ethan Brzana, David Gomez, and Thi Hong Dang Trinh.
Julia Sickels - jns5224 Sam Fisher - sef5176 Alyssa Hawras - aoh5295.
Review for Exam 3.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Day 4.  Discussion on Yesterday’s Probes  Work on Today’s Probes.
Objectives Solve orbital motion problems. Relate weightlessness to objects in free fall. Describe gravitational fields. Compare views on gravitation.
Physical Science Gravity. Objectives Explain that gravitational force becomes stronger as the masses increase and rapidly become weaker as the distance.
Universal Gravitation. ISAAC NEWTON (1642 – 1727) The rate of acceleration due to gravity at the Earth’s surface was proportional to the Earth’s gravitational.
Newtonian Gravitation and Orbits
Newton’s Law of Universal Gravitation
General Relativity For a general audience. Precession of Mercury Mercury’s entire orbit undergoes precession at a known rate. Most of it can be explained.
Chapter 26.2: Observing the Solar System
Origin of Modern Astronomy
UNIT NINE: Matter and Motion in the Universe  Chapter 26 The Solar System  Chapter 27 Stars  Chapter 28 Exploring the Universe.
The Theory of Relativity. What is it? Why do we need it? In science, when a good theory becomes inadequate to describe certain situations, it is replaced.
Gravitation In galaxy M31, one very similar to our own, there is almost certainly a super massive black hole at the center. This very massive object supplies.
Universal Gravitation Chapter 8. Isaac Newton and Gravity Newton realized an apple falls because of force Moon follows circular path, force needed Newton.
 Galileo was the first who recognize the fact that all bodies, irrespective of their masses, fall towards the earth with a constant acceleration.  The.
GRAVITY AND MOTION. WHAT IS GRAVITY?? Gravity- the force that pulls objects towards one another This causes all objects in the universe with a mass to.
General Relativity & Black Holes Jenn Felder and Nikki Linn Physics 220.
Relativity ds 2 = ( 1 - ) dt 2 – (1 + ) dr 2 – r 2 d  2 – r 2 sin 2  d 2 “ 2GM R R Twinkle, twinkle little star How I wonder where you are “1.75 seconds.
Chapter 13 Black Holes. What do you think? Are black holes just holes in space? What is at the surface of a black hole? What power or force enables black.
Relativity Momentum, mass, Energy, and Gravity
NS 1300 Dr. Hoge.  Can we slow light down?  Can we make things invisible?  Is it possible to travel faster than the speed of light?  Is faster than.
Gravity, Energy, and Light Einstein and Newton 1.
Student groups will create a research presentation which answers specific questions about “History of Classical Gravitational Theory” and “General Relativity.
Universal Gravitation Physics Mr. Padilla. Falling Apple hits Newton on the head. According to the law of inertia, it would not fall unless acted upon.
Gravitation Chapter 7, section 3. Geocentric Models Aristotle (384 – 322 BC) taught that the earth was surrounded by crystalline spheres on which the.
General Relativity and the Expanding Universe Allan Johnston 4/4/06.
Fundamental Principles of General Relativity  general principle: laws of physics must be the same for all observers (accelerated or not)  general covariance:
Extragalactic Astronomy & Cosmology Lecture GR Jane Turner Joint Center for Astrophysics UMBC & NASA/GSFC 2003 Spring [4246] Physics 316.
Early Astronomy Chapter 22, Section 1.
Principle of Equivalence: Einstein 1907 Box stationary in gravity field Box falling freely Box accelerates in empty space Box moves through space at constant.
Gravity and Motion. Gravity is what gives the universe its _________ A universal force that acts on _________ the objects in the universe Every particle.
Astronomy 1143 – Spring 2014 Lecture 18: Special Relativity.
Developing the Science of Astronomy (Chapter 4). Student Learning Objectives Compare ancient and modern theories of the solar system Apply Kepler’s Laws.
How We Know Where They’re Going.  Geocentric Model  Earth is the center of the universe  Philosophy at the time leads to the idea of perfection and.
Gravity – A Familiar Force. Gravitational Force Gravitational force – an attractive force that every object in the universe exerts on every other object.
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Gravity, Energy, and Light Einstein and Newton 1.
The Expanding Universe
Special Relativity Physics 12 Adv. Einstein’s Postulates  In 1905, while working as a patent clerk in Switzerland, Einstein published his paper on.
General Relativity and Grade-9 Astronomy. 0) Gravity causes time to slow down. Everyday Einstein: The GPS and Relativity OAPT Conference May 12 – 14 McMaster.
Life on Earth Without the Theories of Relativity How would our lives be different on Earth if we did not have any knowledge of the theory of relativity?
Universal Gravitation Brought to you by: Ashley, Chelsey, and Jordan.
PHYSICS. Albert Einstein Albert Einstein lived from he was. jewish. He is famous for E=mc squared (energy equals mass ×by the speed of light.
Conceptual Physics 11th Edition
Einstein’s postulates
Universal Gravitation
Lecture 10 Gravitational force (chap 7, 9.6)
Newton’s Law of Universal Gravitation
Newton’s Law of Universal Gravitation
Newton’s Law of Universal Gravitation
A New Vision of the Cosmos
Dark Matter Background Possible causes Dark Matter Candidates
Gravity and Motion.
Universal Gravitation
General Relativity: Part II
UNIT NINE: Matter and Motion in the Universe
Gravity Week of October 22nd.
Universal Gravitation
Presentation transcript:

Theory of relativity: Special Relativity and General Relativity By: Tomas Bayas and Sebastian Naranjo

What Does it State The theory of relativity encompasses two theories within that are called the Special Relativity and General Relativity Theories. They both have different components that make up that Theory of Relativity as a whole. According to the theory everything can be relative with a few exceptions.

Discovery In the year 1687 Isaac Newton published a paper where determined his Theory of Gravitation. In it he stated that “The forces which keep the planets in their orbs must reciprocally be the squares of their distances from the centers about which they revolve”

The theory worked quite well and even lead to the discovering of Neptune but there was a flaw. The theory couldn’t pinpoint accurately the orbit of Mercury and there were no explanations for this. Nearly 200 years later Einstein managed to discover what was wrong. Through his Theory of Relativity, which was published in 1905, he determined that the laws of motion determined by Newton were correct except when velocities reached the speed of light

In his Theory of General Relativity, published in 1915, he determined that the Law of Gravitation proposed by Newton was also almost correct except that he determined that in the presence of strong gravitational fields, things changed, hence the orbit of Mercury couldn’t be determined before. Prior to Einstein discovery space and interactions that occurred in space where seen in a very different way and he provided a gateway to understanding interactions in space.

Description of General Relativity Theory This part of the theory addresses gravity It considers gravity as a geometric property in spacetime. An object with mass can “curve” space and create an orbit so nearby objects follow that path. According to Einstein gravity can curve space and time.

Description of Theory of Special Relativity This is a special case because it refers only to the possibility when two objects are moving at constant speeds relative to each other. The Special Relativity Theory states: The laws of physics are the same for objects moving at constant speed frames of reference. Speed of light is constant in a vacuum regardless of the motion or speed of the observers.

Spacetime We normally consider that there three dimensions in this world but Einstein’s work allowed to determine there is a fourth dimension which is spacetime; the combination of time and space into one interwoven continuum. Time cannot be separated from the dimensions of space because it depends on the velocity of an object and as already stated velocity (as well as other measurements) is relative.

Example of General Relativity Imagine you can set a large body in the middle of a trampoline. The body would press down and alter the surface causing a hole. If you place a marble on the edge of the trampoline it would approach the large body. This is similar to the force a planet can exert on a rock in space, bending the spacetime.

Impact on Society Even today the relativity theory plays its main role in the astronomical domain It helped to understand black holes, gravity waves and cosmic big bangs. Theorists have been using general relativity with other interactions, using concepts such as branes and string that are actually helping to prove the modern theories such as strings theory.

Relativity plays a major role in a multi-billion dollars industry centered around Global Positioning system (GPS). Besides all the military uses, GPS is finding applications in airplane navigation, oil exploration, wilderness recreation, bridge construction, sailing and many more. To determine its location, the GPS receiver uses the time at which each signal from a satellite was emitted. This together with the speed of light the distance between the receiver and the satellites can be calculated. As the orbit of each satellite is known accurately, with this it is a simple geometry problem to compute the receiver’s location, both in space and time.

Bibliography Arora, Hans. "Helix Magazine." Einstein's Theory Of Relativity: Implications Beyond Science? N.p., 20 Oct. 2008. Web. 28 Feb. 2014. <http://helix.northwestern.edu/article/einsteins-theory-relativity-implications-beyond-science>. O’Connor, J J and Robertson, E F. "General Relativity." General Relativity. N.p., n.d. Web. 02 Mar. 2014. <http://www-groups.dcs.st-and.ac.uk/history/HistTopics/General_relativity.html>. Perkowitz, Sidney. "Relativity (physics)." Encyclopedia Britannica Online. Encyclopedia Britannica, n.d. Web. 02 Mar. 2014. <http://www.britannica.com/EBchecked/topic/496904/relativity>.

Unknown. "The Equation That Changed The World | Quantum Science Philippines." The Equation That Changed The World | Quantum Science Philippines. N.p., n.d. Web. 02 Mar. 2014. <http://www.quantumsciencephilippines.com/69/the-equation-that-changed-the-world/>. Williams, Clifford M. "Einstein's Relativity and Everyday Life." Physics Central. N.p., n.d. Web. 02 Mar. 2014. <http://physicscentral.com/explore/writers/will.cfm>. Zimmerman Jones, Andrew and Robbins, Daniel. "Einstein's Special Relativity." - For Dummies. N.p., n.d. Web. 01 Mar. 2014. <http://www.dummies.com/how-to/content/einsteins-special-relativity.html>.

Background pictures taken from Google Images, “Relativity-google search”. Web. 02. Mar. 2014. https://www.google.com/search?biw=1366&bih=667&noj=1&tbm=isch&oq=+relativity&gs_l=img.3..0l10.105340.106076.0.106517.8.4.0.0.0.1.175.409.2j2.4.0....0...1c.1.36.img..5.3.296.WjFFu-AilV8&q=relativity