Physical Foundations of Natural Science Vasily Beskin # 2-4.

Slides:



Advertisements
Similar presentations
Common Variable Types in Elasticity
Advertisements

What is displacement? A.Term correct B.Units Correct C.Quantity type correct. D.None correct Displacement of an object is a vector quantity representing.
Today’s topic: Some Celestial Mechanics F Numeriska beräkningar i Naturvetenskap och Teknik.
Sect. 8.2: Cyclic Coordinates & Conservation Theorems
The Beginning of Modern Astronomy
Numeriska beräkningar i Naturvetenskap och Teknik Today’s topic: Some Celestial Mechanics F.
Hot topics in Modern Cosmology Cargèse - 10 Mai 2011.
Objectivity – the role of space-time models Peter Ván HAS, RIPNP, Department of Theoretical Physics –Introduction – objectivity –Traditional objectivity.
Chapter 4 Work and Energy Additional Concepts For Describing Motion.
Extragalactic Astronomy & Cosmology First-Half Review [4246] Physics 316.
1 Vectors and Polar Coordinates Lecture 2 (04 Nov 2006) Enrichment Programme for Physics Talent 2006/07 Module I.
Lagrangian and Hamiltonian Dynamics
Mechanics of Rigid Bodies
Relative Velocity Two observers moving relative to each other generally do not agree on the outcome of an experiment However, the observations seen by.
Review (2 nd order tensors): Tensor – Linear mapping of a vector onto another vector Tensor components in a Cartesian basis (3x3 matrix): Basis change.
Stanford University Department of Aeronautics and Astronautics Introduction to Symmetry Analysis Brian Cantwell Department of Aeronautics and Astronautics.
Kinetics of Particles:
STATIC EQUILIBRIUM [4] Calkin, M. G. “Lagrangian and Hamiltonian Mechanics”, World Scientific, Singapore, 1996, ISBN Consider an object having.
Relativistic Classical Mechanics. XIX century crisis in physics: some facts Maxwell: equations of electromagnetism are not invariant under Galilean transformations.
QM 480 “On the Shoulders of Giants” An Introduction to Classical Mechanics.
Physics 430: Lecture 15 Lagrange’s Equations
MA4248 Weeks 1-3. Topics Coordinate Systems, Kinematics, Newton’s Laws, Inertial Mass, Force, Momentum, Energy, Harmonic Oscillations (Springs and Pendulums)
Advanced mechanics Physics 302. Instructor: Dr. Alexey Belyanin Office: MIST 426 Office Phone: (979)
Motion Summary.  Vectors & Scalars  Displacement, Velocity, Acceleration  Equations of motion  Relative motion.
A PPLIED M ECHANICS Lecture 01 Slovak University of Technology Faculty of Material Science and Technology in Trnava.
 Newtonian relativity  Michelson-Morley Experiment  Einstein ’ s principle of relativity  Special relativity  Lorentz transformation  Relativistic.
Gneral Physics I, Lecture Note, Part 1 (Lecture 1-11)1 General Physics I Instructor Tamer A. Eleyan 2009/2010.
Engineering Mechanics
General Relativity Physics Honours 2005 Dr Geraint F. Lewis Rm 557, A29
Wednesday, Feb. 28, 2007PHYS 5326, Spring 2007 Jae Yu 1 PHYS 5326 – Lecture #9 Wednesday, Feb. 28, 2007 Dr. Jae Yu 1.Quantum Electro-dynamics (QED) 2.Local.
KINETICS OF PARTICLES: ENERGY AND MOMENTUM METHODS s2s2 A1A1 A2A2 A s1s1 s drdr F  ds Consider a force F acting on a particle A. The work of F.
Action function of the electromagnetic field Section 27.
D’Alembert’s Principle the sum of the work done by
Four-potential of a field Section 16. For a given field, the action is the sum of two terms S = S m + S mf – Free-particle term – Particle-field interaction.
Physicists explore the universe. Their investigations, based on scientific processes, range from particles that are smaller than atoms in size to stars.
Physics 218 Lecture 15: Momentum Alexei Safonov.
General Relativity Physics Honours 2008 A/Prof. Geraint F. Lewis Rm 560, A29 Lecture Notes 9.
Hirophysics.com PATRICK ABLES. Hirophysics.com PART 1 TIME DILATION: GPS, Relativity, and other applications.
Phy 303: Classical Mechanics (2) Chapter 3 Lagrangian and Hamiltonian Mechanics.
Quantum Two 1. 2 Angular Momentum and Rotations 3.
A Mathematical Frame Work to Create Fluid Flow Devices…… P M V Subbarao Professor Mechanical Engineering Department I I T Delhi Development of Conservation.
The Meaning of Einstein’s Equation*
Work Readings: Chapter 11.
Hamiltonian Mechanics (For Most Cases of Interest) We just saw that, for large classes of problems, the Lagrangian terms can be written (sum on i): L.
The Hamiltonian method
Monday, Apr. 4, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #16 Monday, Apr. 4, 2005 Dr. Jae Yu Symmetries Why do we care about the symmetry?
PHYSICS 361 (Classical Mechanics) Dr. Anatoli Frishman Web Page:
Syllabus Note : Attendance is important because the theory and questions will be explained in the class. II ntroduction. LL agrange’s Equation. SS.
1 The law of gravitation can be written in a vector notation (9.1) Although this law applies strictly to particles, it can be also used to real bodies.
Celestial Mechanics IV Central orbits Force from shape, shape from force General relativity correction.
Fall 2011 PHYS 172: Modern Mechanics Lecture 7 – Speed of Sound in a Solid, Buoyancy Read 4.9 – 4.13.
Equations of motion of a charge in a field Section 17.
1 ECE Engineering Model The Basis for Electromagnetic and Mechanical Applications Horst Eckardt, AIAS Version 4.1,
Space-Time Symmetry.
Classical Mechanics Lagrangian Mechanics.
Schrodinger wave equation
Continuum Mechanics (MTH487)
Special Theory of Relativity
Hamiltonian Mechanics
Quantum One.
Astronomy before computers!.
Quantum Two.
Relativistic Classical Mechanics
Continuous Systems and Fields
Drawing and Examples (2-3) Dictionary Definition
Chapter 13 Gravitation In this chapter we will explore the following topics: -Newton’s law of gravitation that describes the attractive.
9. Gravitation 9.1. Newton’s law of gravitation
Chapter 13 Gravitation In this chapter we will explore the following topics: -Newton’s law of gravitation, which describes the attractive force between.
Physics 319 Classical Mechanics
Conservation Theorems Section 7.9
Presentation transcript:

Physical Foundations of Natural Science Vasily Beskin # 2-4

Gravitation and Astrophysics

School level Ready solutions of equations (many of which are not even formulated)

An example - Gravity What is the equation and that - the solution?

An example - Gravity What is the equation and that - the solution?

Scientific level The formulation of equations and their solution

A fundamental observation I.Newton ( ) Our world is described by equations of the second order Requires two initial conditions

Classiacal world (c, G) Fundamental generalizations Mechanics (Newton laws): Lorentz invariance, conservation laws are a consequence of the symmetry, integrated nature conservation laws, principle of least action (Lagrange) Hamiltonian formalism, from scalars to tensors.

Principle of least action W.Hamilton ( ) J.L.Lagrange ( ) coordinate x momentum p = m v velocity v

Principle of least action P.de Fermat ( ) P.L.de Maupertuis( ) L.Euler ( )

Principle of least action Fermat's principle x 1 x 2 x у

Principle of least action Action Equation of motion

Principle of least action The equations of motion can be derived from the principle of least (extreme) action.

Newton limit From school we know that

An example – the Gravity

Scalar potential Acceleration does not dependent on the mass The law of motion looks identical Right to left and left to right The theory of gravity is scalar

Certainly, the correct theory Prediction of the existence of planets Correctly describes the motion of the satellites etc.

What is wrong? Newton theory of gravity is not Lorentz-invariant. Observations! The motion of the perihelion of Mercury is not described by this law.

Intermediate results Correct theory must meet a certain set of fundamental properties (axioms). General relativity is actually not the only possible theory of gravity (generalizing - field theory). The question arises whether it is possible to determine the form of the theory (i.e. the form of the equations describing its basic laws), based only on general principles, that is, completely disregarding the observations.

Kinetic energy Is it possible:

Kinetic energy Is it possible: ?

Kinetic energy Is it possible:

Kinetic energy Is it possible:

An example: square latice

Intermediate results Correct theory must meet a certain set of fundamental properties (axioms). One of them - Lorentz invariance. General relativity is actually not the only possible theory of gravity (generalizing - field theory). In the limit of weak fields and low speeds we have to return to the old theory. A big role to play invariants.

Important conclusions General principles (symmetry, Lorentz invariance) can help limit the theory, but, in general, do not define it through. When extending the theory necessary to introduce dimensional constants (mass M, velocity c ), the values of which can only be determined from observations. In the limiting case (in the example above - at non-relativistic velocities v << c ) theory should be returned to well-known. One possible generalization - the transition from scalars (numbers) to tensors (tables).

An example – standard model

An example – (non)standard model

Appearing of tensors Quadratic forms kinetic energy metric Linear dependence Hooke's law Ohm’s law

Homogeneous media Hall current

Invariants of matrices '‘Square'' of symmetric matrix The sum of the diagonal elements - the so-called 'Trace' (in German 'Spur')

Problem Show that a square matrix is independent of the angle 

Metric

Cartesian Cylindrical Spherical

Metric Arbitrary

Metric En example – oblique grid Problem

And what with the invariants? For orthogonal coordinate (i.e. for the diagonal matrices)