DEVOURING HIS CHILDREN

Similar documents
Review Special Relativity. February 3, Absolutes of Relativity. Key Ideas of Special Relativity. Path of Ball in a Moving Train

Wallace Hall Academy

ALBERT EINSTEIN AND THE FABRIC OF TIME by Gevin Giorbran

Chapter S3 Spacetime and Gravity. Agenda. Distinguishing Crackpots

Chapter S3 Spacetime and Gravity Pearson Education, Inc.

E = mc 2. Inertial Reference Frames. Inertial Reference Frames. The Special Theory of Relativity. Slide 1 / 63. Slide 2 / 63.

Einstein s Gravity. Understanding space-time and the gravitational effects of mass

Chapter 26. Relativity

Chapter 5 Newton s Universe

EPGY Special and General Relativity. Lecture 4B

Black Holes. Over the top? Black Holes. Gravity s Final Victory. Einstein s Gravity. Near Black holes escape speed is greater than the speed of light

A100 Exploring the Universe: Black holes. Martin D. Weinberg UMass Astronomy

THE ORIGIN OF THE UNIVERSE AND BLACK HOLES

Correct Resolution of the Twin Paradox

The cause and development of cosmic background radiation

A100H Exploring the Universe: Black holes. Martin D. Weinberg UMass Astronomy

Unit 4. Greece and Rome

1 WHAT IS BIG HISTORY? WHY DO WE LOOK AT THINGS FROM FAR AWAY AND CLOSE UP?

We saw last time how the development of accurate clocks in the 18 th and 19 th centuries transformed human cultures over the world.

ACTIVITY 5. Figure 5-1: Simulated electron interference pattern with your prediction for the next electron s position.

Electronic Journal of Theoretical Physics. A-Temporal Universe. Amrit Sorli, Ilaria Sorli

Einstein s Relativity and Black Holes

Physics. Special Relativity

Abstract: Here, I use the basic principles of the McMahon field theory to explain the strong force and the weak force, as described for atoms.

22. Black Holes. Relativistic Length Contraction. Relativistic Time Dilation

Michael H. Shulman ( Is it possible to travel in Time?

Bell s spaceship paradox

Chapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Special Relativity. Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers.


BLACKHOLE WORMHOLE THEORY

Please pick up your midterms from front of class

Making Sense. Tom Carter. tom/sfi-csss. April 2, 2009

Atomic Theory. Introducing the Atomic Theory:

Special theory of relativity

Special Relativity: Derivations

The result is; distances are contracted in the direction of motion.

Free-Body Diagrams: Introduction

3 Newton s First Law of Motion Inertia. Forces cause changes in motion.

Time Dilation and the Twin Paradox Revisited

May the force be with you

Motivation. The Speed of Light. The Speed of Light. In Water Things Look Like This. Introduction to Special and General Relativity

GAMMA RAYS. 1 P a g e

Gravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force.

How to Understand the Twin Paradox

##FROM SPACE-TIME TO A-TEMPORAL PHYSICAL SPACE Amrit Sorli, SpaceLife Institute, Podere Petraiole, Chiusdino (SI), Italy

PHY1033C/HIS3931/IDH 3931 : Discovering Physics: The Universe and Humanity s Place in It Fall Prof. Peter Hirschfeld, Physics

Astronomy Ch. 22 Neutron Stars and Black Holes. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Chapter 4 Newton s Laws

The Problem of Slowing Clocks in Relativity Theory

CHAPTER 9 THE ARROW OF TIME

Physics 141 Dynamics 1 Page 1. Dynamics 1

Lecture 18 : Black holes. Astronomy 111

18.3 Black Holes: Gravity's Ultimate Victory

Syllabus and Schedule for ASTRO 210 (Black Holes)

Elements of Physics II

Transformation of velocities

Gravitational Interactions

Survey of Astrophysics A110

Understanding the Universe S TA R T ING WITH EARTH A ND B E YO ND

Test 3 results B A. Grades posted in Learn

The Physics of Impossible Things Benjamin Schumacher Kenyon College

Q25: Record the wavelength of each colored line according to the scale given.

Today. Review. Momentum and Force Consider the rate of change of momentum. What is Momentum?

Distant Stars and a Young Earth?

Gravity: What s the big attraction? Dan Wilkins Institute of Astronomy

7/5. Consequences of the principle of equivalence (#3) 1. Gravity is a manifestation of the curvature of space.

A Brief Guide to Our Cosmic Context

CHAPTER 2. FORCE and Motion. CHAPTER s Objectives

MATH1014 Calculus II. A historical review on Calculus

Today in Astronomy 102: time machines

Simultaneity And Time Dilation

Today HW#4 pushed back to 8:00 am Thursday Exam #1 is on Thursday Feb. 11

The interpretation is that gravity bends spacetime and that light follows the curvature of space.

Be able to explain retrograde motion in both the current and Ptolemy s models. You are likely to get an essay question on a quiz concerning these.

The passengers ride in capsules. Each capsule moves in a circular path and accelerates.

GRAVITATIONAL COLLAPSE

Mr Casey Ray McMahon, B.Sci (Hons), B.MechEng (Hons) Copyright Version: 17 th May, 2015 Page: 1 of 8 String theory explained via McMahon field theory.

In the 1860s, Louis Pasteur showed through

Lecture Outlines. Chapter 22. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Astronomy- The Original Science

The Riddle of Gravitation A New Solution Proposal By Josef Kemény, 2008

Einstein s Space and Time

Black Holes -Chapter 21

The Scientific Revolution & The Age of Enlightenment. Unit 8

The Science of Life in the Universe (Chap 2 Bennett/Shostak) Overview of Chapter 2. Overview of Chapter 2. Example Question

Def. 1. A time travel spacetime is a solution to Einstein's equations that admits closed timelike curves (CTCs).

You Might Also Like. I look forward helping you focus your instruction while saving tons of time. Kesler Science Station Lab Activities 40%+ Savings!

Unit 2 - Linear Motion and Graphical Analysis

Today: Start Ch. 18: Cosmology. Homework # 5 due next Wed. (HW #6 is online)

BEFORE YOU READ. Forces and Motion Gravity and Motion STUDY TIP. After you read this section, you should be able to answer these questions:

Lesson 12 Relativity

Gravity and Spacetime: Why do things fall?

Chapter 2 The Copernican Revolution

What If We Had No Moon?

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER

Observing the Solar System 20-1

Special Theory of Relativity. A Brief introduction

The History of Astronomy

Lorentz Transformations and the Twin Paradox By James Carter

Transcription:

WHAT IS TIME? The fifth century Christian theologian Augustine wrote: What then is time? I know well enough what it is, provided that nobody asks me; but if I am asked what it is and try to explain, I am baffled. The passage of fifteen hundred years has, in fact, done little to clarify the real meaning of time. Throughout history, human beings have always puzzled over time's profound but seemingly vague nature. The subject of time has fascinated poets, writers, and philosophers of every generation. Modern science has given us a way of incorporating the concept of time into measurements of physical quantities. We know that time is a measure of change. We know that change involves the expenditure of energy. By the second law of thermodynamics, energy expenditure produces unwanted entropy. Thus time gets directly linked to the tendency of physical systems to disorder. Time involves irreversibility. SATURN DEVOURING HIS CHILDREN (1824) by the Spanish artist Francisco de Goya. http://cosmology.uwinnipeg.ca/cosmology/time.htm (1 of 9) [03/25/2002 1:43:05 PM]

Saturn was the roman name for Cronus, the god associated in late Greek mythology with time. He swallowed his children after being told that one of them would dethrone him. Only Zeus, who later did dethrone him, escaped. The painting symbolizes how time ravages and destroys all humans. Unlike Zeus, mere mortals cannot evade his clutches. The irreversibility of time does not hold on small scales. None of the major theories in physics seem to preferentially pick out a certain direction in time. On small scales processes are genuinely reversible. On large macroscopic scales, processes are unquestionably irreversible. How this switch over, from irreversibility to reversibility, occurs is a fundamental mystery. The irreversible direction of time was not always accepted by ancient civilizations. The cyclic character of time was a common feature in Greek cosmological thought. Aristotle wrote that 'there is a circle in all other things that have a natural movement and coming into being and passing away. This is because all other things are discriminated by time and end and begin as though conforming to a cycle; for even time itself is thought to be a circle.' The Stoics believed that when the planets returned to the same relative positions, as at the beginning of time, the cosmos would be renewed again and again. http://cosmology.uwinnipeg.ca/cosmology/time.htm (2 of 9) [03/25/2002 1:43:05 PM]

The reason for the acceptance of cyclic-time ideas was because time's arrow, a unique direction of time, aroused deep fear, even terror, amongst the thoughtful of ancient civilizations. A time direction implied instability, flux, and change. It was associated with the end of the world and not associated with rebirth and renewal. It was the Judeo-Christian tradition that imposed a 'linear' irreversible time in Western culture. Through the Christian belief in the birth and death of Christ and the Crucifixion as unique events, a direction of time was accepted. These events were assumed to be unrepeatable. Western civilization came to regard time as a linear path that stretches between past and future. Before the Christians, only the Hebrews and the Zoroastrian Persians had adopted this progressive view of time. Scientists became involved with the concept of time when Newton (1687) felt compelled to define time as being necessarily absolute. This meant that all events could be regarded as having a distinct and definite position in space and occur at a particular moment of time. This moment of time was taken to be the same for observers everywhere in the universe. Time was an unstretchable quantity, in terms of which, change in the whole universe could be uniquely described. Newton constructed a deterministic set of mathematical relations that allowed prediction of the future behavior of moving objects and allowed deduction of the past behavior of the moving objects. All that one needed in order to do this was data in the present regarding these moving objects. Einstein changed these ideas totally. In his special theory of relativity and his general relativity theory time became a relative concept. This meant that time varied from place to place. Time was stretchable. In special relativity time became stretched when you moved with any speed. The effect is biggest when you move at speeds close to one billion kilometers per hour. In general relativity time became stretched when you placed yourself into a gravitational field. This effect is biggest when the gravitational field is strong. In relativity we can draw diagrams, called spacetime diagrams, of the paths people take as they go forward in time. The path is called the world-line of the individual. World-line of a person walking to the right, stopping, and then walking back to the left. http://cosmology.uwinnipeg.ca/cosmology/time.htm (3 of 9) [03/25/2002 1:43:05 PM]

Note that the vertical displacement of the individual is the time elapsed since she started the journey. The individual cannot move in any way such that the vertical direction is traversed in the negative (down) direction. That direction would correspond to going backwards in time. On spacetime diagrams such as the one above, light rays will travel along paths always at 45 degree angles to the horizontal and vertical lines. Nothing can travel faster than these light paths. All objects having mass must move slower that the light rays. Consequently the motion of everyday objects falls within the 45 degree angled lines. These 45 degree lines form what is called the light cone. Paths outside the light cone are forbidden. They represent object paths corresponding to speeds greater that the speed of light. http://cosmology.uwinnipeg.ca/cosmology/time.htm (4 of 9) [03/25/2002 1:43:05 PM]

This is a diagram for the world-line of a particle that travels at less than the speed of light. The place where the two forbidden triangles meet is called the present. The future is the triangular shaped region at the top of the diagram. The past is the triangular shaped diagram at the bottom of the diagram. At no time can the particle divert into the forbidden regions (red triangles) without going faster than the speed of light. Every point along the world-line of the particle must never be greater than 45 degrees. To go backwards in time however this is exactly what the observer would have to do. Hence, special relativity predicts that you can only go backwards in time if you travel faster than the speed of light. http://cosmology.uwinnipeg.ca/cosmology/time.htm (5 of 9) [03/25/2002 1:43:05 PM]

The effect of gravity on light cones is to tip them in the direction of the gravitational curvature. Black holes tip the light cones of nearby particles so much that the future part of the light cones points directly into the black hole. In this case, no matter how the particle moves, its future lies trapped inside the black hole. Both the general and the special theory of relativity give a method for time travel into the future. In special relativity all one has to do is to leave the Earth behind and travel in a super fast space ship. Your time intervals will dilate, making your clocks run very slow compared with the clocks that remain fixed to the Earth's surface. When you return to the Earth, you will have aged a small fraction of the time that people who remained on the Earth have aged. In effect you have traveled to the future of the Earth in your fast 'time-machine' spaceship. In general relativity you leave the Earth and encircle a dense object such as a neutron star for a small amount of time. To increase the amount you travel into the future, you orbit closer to the neutron star. The gravitational field dilates http://cosmology.uwinnipeg.ca/cosmology/time.htm (6 of 9) [03/25/2002 1:43:05 PM]

your time intervals. When you finally leave the vicinity of the neutron star and return to the Earth, all inhabitants of the Earth will have aged much more than you have. You have effectively traveled to the future using a strong gravitational field to carry out the time travel. For short mpeg movies simulating trips to neutron stars and black holes click here. The laws of physics do not preclude time travel. They seem to work irrespective of the direction of time. There are, however, two logical objections to travel into the past in the same universe. They are as follows: 'Grandfather Paradox'- You cannot travel to the past and disrupt some event in such a way that you never existed in the first place. This is called the grandfather paradox because you can think of going backwards in time and killing your own grandfather. This is problematic, since if you really did kill your own grandfather, you shouldn't exist at all. 'No Free Lunch' Paradox'- Within the same universe time travelers should not be able to bring information and energy to the past that could be used to create new ideas and products. This would involve no creative energy on the part of the "inventor." Example: Imagine that the famous artist, Pablo Picasso, had traveled back in time to meet his younger self. He could give his younger self his portfolio containing copies of his art. If the young version of Picasso meticulously copied the reproductions, he could have affected the future of 20th century art at a very early age. His reproductions would exist because they were copied from the originals, and the originals would exist because they were copied from the reproductions. The time-traveling artist would have created masterpieces without ever having expended any energy in their creation. It is possible to construct time machines in general relativity that take you back into the past. These machines usually involve rapidly rotating dense objects which are dragging spacetime around with them. An example is the rotating massive cylinder shown below. You travel forwards in time if you go around the massive rotating cylinder in its direction of rotation. You travel backwards in time if you go around the cylinder in the opposite direction that it is rotating. http://cosmology.uwinnipeg.ca/cosmology/time.htm (7 of 9) [03/25/2002 1:43:05 PM]

Alternatively you can time travel using wormholes that connect our universe with itself at a earlier time (or some other universe that is a copy of our universe at a earlier time). To avoid the two logical problems given above, it is mandatory to allow for the existence of multiple worlds. It turns out that the theory of physics, called quantum mechanics, that governs all physical phenomena on the smallest scales can be interpreted literally as a theory of parallel universes. Hence, quantum theory is quite consistent with the idea that time travel can exist without logical difficulties. How is time viewed in a parallel universe scenario? Each moment of time is seen as a distinct universe recreated from the previous universe such that the rules of existence (the laws of thermodynamics) are obeyed. Below is a diagram of a stack of 2-D universes. Time proceeds from the bottom of the stack to the top of the stack. Time is then seen as just a universe label: Time 1 = Universe #1, Time 2 = Universe #2, Time 3 = Universe #3, etc. http://cosmology.uwinnipeg.ca/cosmology/time.htm (8 of 9) [03/25/2002 1:43:05 PM]

The recreation of the universe at any instant is done so rapidly that no experiment can pick up any part of the universe's recreation at that instant. If you have two or more adjacent stacks of universes then it is possible for time travel to be self-consistent. The time-traveler has to hop from a certain time in the left stack of universes to a different time in the right stack of copy universes. Click here for some resources on time travel: NOVA Time Travel http://cosmology.uwinnipeg.ca/cosmology/time.htm (9 of 9) [03/25/2002 1:43:05 PM]