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- Introduction Quantities and units - ( 4 - 6 )
- Introduction to mechanics - ( 7 - 23 )
- Forces on a car bumper - ( 24 - 43 )
- Equilibrium of rigid bodies - ( 44 - 50 )
- Moment of a force about a point - ( 51 - 52 )
- Direction of Mo - ( 53 - 67 )
- Opening a cellar Door - ( 68 - 69 )
- Positive and negitive Area - ( 70 - 74 )
- The Free body Diagram - ( 75 - 84 )
- Stability and determinacy - ( 85 - 119 )
- Magnitude and centroid - ( 120 - 125 )
- Multiple shapes - ( 126 - 132 )
- Friction and elements of rigid body dynamics - ( 133 - 151 )

Topic:

1. Introduction
Isaac Newton (1643-1727)
painted by Godfrey Kneller, National Portrait Gallery London, 1702
In the early stages of scientific development, ―physics‖ mainly consisted of mechanics and
astronomy. In ancient times CLAUDIUS PTOLEMAEUS of Alexandria (*87) explained the
motionsof the sun, the moon, and the five planets known at his time. He stated that the
planets and the sun orbit the Earth in the order Mercury, Venus, Sun, Mars, Jupiter, Saturn.
This purely phenomenological model could predict the positions of the planets accurately
enough for naked-eye observations. Researchers like NIKOLAUS KOPERNIKUS (1473-1543),
TYCHO BRAHE (1546-1601) and JOHANNES KEPLER (1571-1630) described the movement of
celestial bodies by mathematical expressions, which were based on observations and a
universalhypothesis (model). GALILEO GALILEI (1564-1642) formulated the laws of free fall
of bodies and other laws of motion. His ―discorsi" on the heliocentric conception of the world
encountered fierce opposition at those times.
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After the renaissance a fast development started, linked among others with the names
CHRISTIAAN HUYGENS (1629-1695), ISAAC NEWTON (1643-1727), ROBERT HOOKE (16351703) and LEONHARD EULER (1707-1783). Not only the motion of material points was
investigated, but the observations were extended to bodies having a spatial dimension. With
HOOKE’s work on elastic steel springs, the first material law was formulated. A general theory
of the strength of materials and structures was developed by mathematicians like JAKOB
BERNOULLI (1654-1705) and engineers like CHARLES AUGUSTIN COULOMB (1736-1806) and
CLAUDE LOUIS MARIE HENRI NAVIER (1785-1836), who introduced new intellectual concepts
likestress and strain.
The achievements in continuum mechanics coincided with the fast development in
mathematics: differential calculus has one of its major applications in mechanics, variational
principlesare used in analytical mechanics.
These days mechanics is mostly used in engineering practice. The problems to be solved are
manifold:
• Is the car’s suspension strong enough?
• Which material can we use for the aircraft’s fuselage?
• Will the bridge carry more the 10 trucks at the same time?
• Why did the pipeline burst and who has to pay for it?
• How can we redesign the bobsleigh to win a gold medal next time?
• Shall we immediately shut down the nuclear power plant?
For the scientist or engineer, the important questions he must find answers to are:
• How shall I formulate a problem in mechanics?
• How shall I state the governing field equations and boundary conditions?
• What kind of experiments would justify, deny or improve my hypothesis?
• How exhaustive should the investigation be?
• Where might errors appear?
• How much time is required to obtain a reasonable solution?
• How much does it cost?
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One of the most important aspects is the load–deformation behaviour of a structure. This
question is strongly connected to the choice of the appropriate mathematical model, which is
used for the investigation and the chosen material. We first have to learn something
aboutdifferent models as well as the terms motion, deformation, strain, stress and load and their
mathematical representations, which are vectors and tensors.
Figure 1-1: Structural integrity is commonly not tested like this
The objective of the present course is to emphasise the formulation of problems in
engineering mechanics by reducing a complex "reality" to appropriate mechanical and
mathematical models. In the beginning, the concept of continua is expounded in comparison
to real materials.. After a review of the terms motion, displacement, and deformation,
measures for strains and the concepts of forces and stresses are introduced. Next, the basic
governing equations of continuum mechanics are presented, particularly the balance
equationsfor mass, linear and angular momentum and energy. After a cursory introduction
into the principles of material theory, the constitutive equations of linear elasticity are
presented for small deformations. Finally, some practical problems in engineering, like
stresses and deformation of cylindrical bars under tension, bending or torsion and of
pressurised tubes are presented.
A good knowledge in vector and tensor analysis is essential for a full uptake of continuum
mechanics. A respective presentation
will not be provided during the course, but the
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nomenclature used and some rules of tensor algebra and analysis as well as theorems on
properties of tensors are included in the Appendix.
Physical Quantities and Units
Definitions
Physical quantities are used for the qualitative and quantitative description of physical
phenomena. They represent measurable properties of physical items, e.g. length, time, mass,
density, force, energy, temperature, etc.
Every specific value of a quantity can be written as the product of a number and a unit. This
product is invariant against a change of the unit.
Examples: 1 m3 = 1000 cm3, 1 m/s = 3,6 km/h
Physical quantities are denoted by symbols.
Examples: Length l, Area A, velocity v, force F
l = 1 km, A = 100 m2, v = 5 m/s F = 10 kN
Base quantities are quantities, which are defined independently from each other in a way that
all other quantities can be derived by multiplication or division.
Examples: Length, l, time, t, and mass, m, can be chosen as base quantities in dynamics.
The unit of a physical quantity is the value of a chosen and defined quantity out of all
quantities of equal dimension.
Example: 1 meter is the unit of all quantities having the dimension of a length (height,
width, diameter, ...)
The numerical value of a quantity G is denoted as {G}, its unit as [G].
The invariance relation is hence G = {G} [G]
Base units are the units of base quantities. The number of base units hence always equals the
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