Lecture 1 and 2
Saif Ahmed (SfA)
Lecturer, Department of Mathematics and Physics
             North South University
Measurement
• We discover physics by learning how to measure the quantities
  involved in physics. Among these quantities are length, time, mass,
  temperature, pressure, and electric current.
• We measure each physical quantity in its own units, by comparison
  with a standard. The unit is a unique name we assign to measures of
  that quantity—for example, meter (m) for the quantity length. The
  standard corresponds to exactly 1.0 unit of the quantity
Base Quantities
• There are so many physical quantities that it is a problem to organize them.
  Fortunately, they are not all independent; for example, speed is the ratio of
  a length to a time. Thus, what we do is pick out—by international
  agreement—a small number of physical quantities, such as length and time,
  and assign standards to them alone. We then define all other physical
  quantities in terms of these base quantities and their standards (called base
  standards). Speed, for example, is defined in terms of the base quantities
  length and time and their base standards.
• Base standards must be both accessible and invariable. If we define the
  length standard as the distance between one’s nose and the index finger on
  an outstretched arm, we certainly have an accessible standard—but it will,
  of course, vary from person to person. The demand for precision in science
  and engineering pushes us to aim first for invariability.
The International System of Units
• In 1971, the 14th General Conference on Weights and Measures
  picked seven quantities as base quantities, thereby forming the basis
  of the International System of Units, abbreviated SI from its French
  name and popularly known as the metric system.
Changing Units
• We often need to change the units in which a physical quantity is
  expressed. We do so by a method called chain-link conversion. In this
  method, we multiply the original measurement by a conversion
  factor (a ratio of units that is equal to unity).
Length
• In 1792, the newborn Republic of France established a
  new system of weights and measures. Its cornerstone
  was the meter, defined to be one ten-millionth of the
  distance from the north pole to the equator. Later, for
  practical reasons, this Earth standard was abandoned
  and the meter came to be defined as the distance
  between two fine lines engraved near the ends of a
  platinum–iridium bar, the standard meter bar, which
  was kept at the International Bureau of Weights and
  Measures near Paris. Accurate copies of the bar were
  sent to standardizing laboratories throughout the world.
  These secondary standards were used to produce other,
  still more accessible standards, so that ultimately every
  measuring device derived its authority from the
  standard meter bar through a complicated chain of
  comparisons.
Time
Time has two aspects. For civil and some scientific purposes, we want
to know the time of day so that we can order events in sequence. In
much scientific work, we want to know how long an event lasts. Thus,
any time standard must be able to answer two questions: “When did it
happen?” and “What is its duration?”
Mass
• The SI standard of mass is a cylinder of platinum
  and iridium that is kept at the International bureau
  of weights and measures near Paris and assigned
  by international agreements, a mass of 1 kilogram.
• The masses of atoms can be compared with one
  another more precisely than they can be
  compared with the standard kilogram. For this
  reason, we have a second mass standard. It is the
  carbon-12 atom, which, by international
  agreement, has been assigned a mass of 12 atomic
  mass units (u)
Motion
• The world, and everything in it, moves. Even seemingly stationary
  things, such as a roadway, move with Earth’s rotation, Earth’s orbit
  around the Sun, the Sun’s orbit around the center of the Milky Way
  galaxy, and that galaxy’s migration relative to other galaxies.
1. Motion is along a straight line
2. Forces cause motion
3. The moving object is either a particle or and object that moves like
    a particle
Position and Displacement
• To locate an object means to
  find its position relative to
  some reference point, often
  the origin (or zero point) of an
  axis such as the x axis. The
  positive direction of the axis is
  in the direction of increasing
  numbers (coordinates), which
  is to the right. The opposite is
  the negative direction.
Position and Displacement
• Displacement is an example of a vector quantity, which is a quantity
  that has both a direction and a magnitude. (1) Its magnitude is the
  distance (such as the number of meters) between the original and
  final positions. (2) Its direction, from an original position to a final
  position, can be represented by a plus sign or a minus sign if the
  motion is along a single axis.
  Average velocity
Actually, several quantities are associated with the phrase
“how fast.” One of them is the average velocity vavg, which
is the ratio of the displacement x that occurs during a
particular time interval  t to that interval:
Average Speed
          Average speed savg is a different way of describing “how
          fast” a particle moves. Whereas the average velocity
          involves the particle’s displacement  x, the average
          speed involves the total distance covered (for example,
          the number of meters moved), independent of direction;
          that is,
Example
Instantaneous Velocity and Speed
• You have now seen two ways to describe how fast something moves:
  average velocity and average speed, both of which are measured over
  a time interval  t. However, the phrase “how fast” more commonly
  refers to how fast a particle is moving at a given instant—its
  instantaneous velocity (or simply velocity) v.
• The velocity at any instant is obtained from the average velocity by
  shrinking the time interval  t closer and closer to 0. As  t dwindles,
  the average velocity approaches a limiting value, which is the velocity
  at that instant:
Acceleration
Constant Acceleration
In many types of motion, the acceleration is either
constant or approximately so. For example, you might
accelerate a car at an approximately constant rate when a
traffic light turns from red to green
Free Fall acceleration
• If you tossed an object either up or
  down and could somehow eliminate
  the effects of air on its flight, you
  would find that the object
  accelerates downward at a certain
  constant rate. That rate is called the
  free-fall acceleration, and its
  magnitude is represented by g. The
  acceleration is independent of the
  object’s characteristics, such as
  mass, density, or shape; it is the
  same for all objects.