A Boot Camp to Special Theory of Relativity
- Description
- Curriculum
- FAQ
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This course begins with the history of developments in human understanding of the motion of inanimate objects from the time of Socrates and Aristotle to the Present time (Einstein). here we intent to cover the most common topics in this subject that are in the undergraduate curriculum of most of the universities. While setting in the armed chair at home we shall roll through the course of the developments since BC350. in this course we shall derive the energy-mass equivalence relation which has given unique fame to Albert Einstein. In this course, we shall derive Gallio’s Transformation Equations, Lorentz’s Transformation Equation, mass dependence on velocity, dropper shift, and equation for relativistic energy of the particle. Also, the light will be thrown upon the other off-shoots of special Relativity like; Time dilation, length contraction, twin paradox, the meaning of simultaneity, relativistic Doppler effect while obeying the principle of causality. This course will enable us to visualize through Mathematical simulation software MAPLE.
The course opens with fundamental definitions from Principia Mathematica, followed by the derivation of Gallian transformation. Einstein modified the theory of relativity by adding an axiom of absoluteness of speed of light to the basic principle of relativity. this leads to Lorentz’s transformation. the course further takes care of exploration of Lorentz transformation equitation in a smooth way to derive E=mc^2. Use of animations has also been explored to explain various concepts.
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1IntroductionVideo lesson
Lecture 1 will offer glimpses of the history of the development of the subject from the time of Aristotle till the time of Galileo & Newton. Relativity is being talked about since the time of Newton offers Galilean Transformations. In this lecture, we shall discuss Aristotelian Science through his methods, four attributes of objects.
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2Quiz-1Quiz
Quiz based on the Lecture 1 of Section 1.
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3Newton's approach from Principia MathematicaVideo lesson
Lecture 2 will introduce Galileo and Newton's approach through natural philosophy, definitions of space and time from Newton's famous book Principia Mathematica. Newton's three laws of motion will be reviewed. The Principle of relativity will be elaborated along with the definition of an inertial frame of reference.
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4Quiz 2Quiz
Quiz 2 based on Lecture 2 of Section 1.
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5Newtonian Relativity & Galilean TransformationsVideo lesson
In Lecture 3 students will learn (i) to derive Galilean Transformation Equations and their limitations and (ii) high-speed test of GT through experiment.
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6Quiz 3Quiz
Quiz 3 is based on Lecture 3 - Newtonian Relativity and Galilean Transformations.
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7Ether HypothesisVideo lesson
Lecture 4 opens the Luminiferous Ether hypothesis that people supposed facilitates em wave propagation. Here we shall study the proposed properties of Ether and its non-existence forfeited Newtonian Relativity.
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8Quiz 4Quiz
It is based on Lecture 4: Ether Hypothesis
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9Michelson-Morley ExperimentVideo lesson
Lecture 5 presents the famous Michelson-Morley experiment that measured fringe shift to compare with the theoretical prediction of its value. The disparity in experimental and theoretical values advocates rejection of the Ether Hypothesis. And the beginning of the new era of Physics that reformulates basic understanding as homogeneity of space and time while revealing to Universality of the speed of light.
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10Quiz 5Quiz
Based on Michelson Morley Experiment
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11Einstein's PostulatesVideo lesson
This video Lecture 6 explains Einstein's TWO postulates of Special Theory of Relativity in view of his new perception of time.
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12Quiz 6Quiz
This quiz is based on Einstein's postulates of Special Theory of Relativity.
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13Derivation of Lorentz TransformationsVideo lesson
This Lecture 7 depicts that Circular Trigonometry does not support Light equations in the space-time continuum. Rather the Hyperbolic trigonometry supports it and then yields transformation equations which are known as Lorentz Transformation Equations.
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14Quiz 7Quiz
Quiz 7 is based on Lecture 7.
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15Alternate Derivation of Lorentz TransformationVideo lesson
In this Lecture 8, an alternate (algebraic) approach of deriving the Lorentz Transformation equation is depicted with animation.
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16Quiz 8Quiz
Quiz on derivation of Lorentz Transformation by the Algebraic Method
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17Inverse Lorentz TransformationVideo lesson
In Lecture 9, Inverse Lorentz Transformation (ILT) equations are derived.
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18Quiz 9Quiz
Based on Inverse Lorentz Transformations.
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19How this Gamma behavesVideo lesson
The Lorentz transformation equations offer a linear dependence on the factor γ. In Lecture 10, we shall learn the behaviour of this factor γ with relative velocity.
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20Quiz-10Quiz
Based on lecture 10.
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21Space-time diagrams (PART-I)Video lesson
The present video lecture 11 describes drawing space-time diagrams for moving and steady objects in reference to Galilean Transformation equations. Moreover, the definition of the Inertial Frame and the non-inertial frame is also explained using ST-diagrams.
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22Quiz 11Quiz
Based on Video Lecture 11
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23Physical Meaning of Moving Bodies and Moving ClocksVideo lesson
Lecture 12 deals with the fact that the factor of gamma involved in Lorentz Transformation equations contracts the space and dilates the time.
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24Quiz 12Quiz
Based on Video Lecture 11
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25Experimental proof for time dilationVideo lesson
Lecture 13 is dedicated to explaining the proof of time dilation in Earth's frame of reference while the observer in Muons frame will see contracted length travelled by Muon. The findings of the Muon experiment puzzled scientists at that time as to how can Muons travel 100 km distance in the span of 2.2 microseconds. Experimental proof for time dilation and space contraction was realized in the Muon experiment that formed evidence for Einstein's Special Theory of Relativity.
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26Quiz 13Quiz
Based on Lecture 13
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27Simultaneity is RelativeVideo lesson
Lecture 14 opens with the discussion on Simultaneity in frames S and S'. Simultaneous events in one of the frames do not guarantee simultaneity in all other inertial frames. This is technically known as "simultaneity is relative".
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28Quiz 14Quiz
Based on Video Lecture 14
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29Space-Time diagrams under LT (PART-II)Video lesson
Lecture 15 deals with the second part of drawing space-time diagrams under Lorentz Transformations. After assimilating the concept of drawing space-time diagrams for both observers S and S', you will be able to draw such space-time diagrams on your own.
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30Space Time Diagrams (PART-III) of Physical Bodies in MotionVideo lesson
Lecture 16 is again dedicated to the drawing of space-time diagrams. In this third part (i) length contraction and (ii) time dilation is expressed using space-time diagrams. These s-t diagrams are drawn to the scale using Maple forms a delightful experience when we look at numerical values of contraction and dilations taking place due to relative speed between inertial frames.
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31Assignment 1Text lesson
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32Space Time Diagrams (PART-IV) Simultaneity in frames S & S’Video lesson
Lecture 17 is dedicated to part four of space-time diagrams wherein the concept of "simultaneity is relative" can be visualized.
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33Area of Space Time CellVideo lesson
Lecture 18 is dedicated to the proof that the unit cell area of the space-time diagram is conserved for all inertial observers.
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34Time Dilation in the Space Time diagramVideo lesson
This lecture 19 will tell you a story of twins celebrating their birthdays and once sending messages while being in their respective frames of reference. This is a very interesting example wherein time dilation is explained using a space-time diagram in an interactive way.
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35QuizQuiz
Based on issues of time dilation
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36Draw a space-time diagram for two observers.Text lesson
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37The Principle of CausalityVideo lesson
Lecture 20 advocates the preservation of the Causality Principle in STR. Causality (cause and effect) is influenced by which one event, process, state or object (a cause) contributes to the production of another event, process, state or object (an effect) where the cause is partly responsible for the effect, and the effect is partly dependent on the cause. Special Theory of Relativity preserves this Principle of Causality until the second axiom by Einstein is valid.
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38QuizQuiz
This quiz is based on the Causality principle.
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