Force

 For other uses, see Force (disambiguation).
In physics, as defined by Asimov, a force is that which can impose a change of velocity on a material body. This concept first appeared in Newton's second law of motion of classical mechanics, and is usually expressed by the equation:
 F = m · a
where
 F is the force, measured in newtons;
 m is the mass, measured in kilograms; and
 a is the acceleration, measured in metres per second squared.
Force has been, however, more accurately defined as being the derivative of momentum.
A prevailing misconception, furthered by physics teachers, is that force is a fundamental quantity in physics. There are, however, more fundamental quantities, such as momentum, energy and stress, which force is sometimes confused with. Unlike these basic quantities, force itself is rarely measured.
Contents 
Applications of force
Types of force
Many forces exist: Coulomb's force (the force between electrical charges), gravitational force (force between masses), magnetic force, friction, and spring force, to name a few.
Despite the many forces, only four fundamental forces of nature are considered. These fundamental forces describe every observable phenomenon; these forces are the strong nuclear force, the electromagnetic force, the weak nuclear force, and the gravitational force. The quantum field theory accurately models the first three fundamental forces; it does not, however, model quantum gravity. Quantum gravity on a large scale can, however, be described by general relativity.
These forces can be further classified into conservative forces and nonconservative forces. Conservative forces, which can be written as the gradient of a potential, include gravity, electromagnetic force, and spring force. Nonconservative forces include friction and drag.
Properties of force
Forces can be represented as a vector with two properties: intensity and direction.
Forces can be added together using parallelogram of force. When two forces act on an object, the resulting force, the resultant, is the vector sum of the original forces. The magnitude of the resultant varies from zero to the sum of the magnitudes of the two forces, depending on the angle between their lines of action. If the two forces are equal, but opposite, the resultant is zero. This condition is called static equilibrium, where the object moves at a constant speed (potentially, but not necessarily zero).
While forces can be added together, they can also be broken down. For example, a horizontal force pointing northeast can be split into two forces, one pointing north, and one pointing east. Summing these component forces, using vector addition, yields the original force.
Units of measurement
The SI unit used to measure force is the newton (symbol N); it is equivalent to kg·m·s^{−2}
Imperial units of force and mass
The F=m·a relationship can be used with any consistent units (MKS or CGS). If these units aren't consistent, a more general form, F=k·m·a, can be used, where the constant k is a conversion factor dependent upon the units being used.
For example, in imperial engineering units, F is measured in "pounds force" or "lbf", m in "pounds mass" or "lb", and a in feet per second squared. In this particular system, one needs to use the more general form above, usually written F=m·a/g_{c} with the constant normally used for this purpose g_{c} = 32.174 lb·ft/(lbf·s^{2}) equal to the reciprocal of the k above.
As with the kilogram, the pound is colloquially used as both a unit of mass and a unit of force. 1 lbf is the force required to accelerate 1 lb at 32.174 ft per second squared, since 32.174 ft per second squared is the standard acceleration due to terrestrial gravity.
Another imperial unit of mass is the slug, defined as 32.174 lb. It is the mass that accelerates by one foot per second squared when a force of one lbf is exerted on it.
When the acceleration of free fall is equal to that used to define pounds force (now usually 9.80665 m/s²), the magnitude of the mass in pounds equals the magnitude of the force due to gravity in pounds force. However, even at sea level on Earth, the actual acceleration of free fall is quite variable, over 0.53% more at the poles than at the equator. Thus, a mass of 1.0000 lb at sea level at the Equator exerts a force due to gravity of 0.9973 lbf, whereas a mass of 1.000 lb at sea level at the poles exerts a force due to gravity of 1.0026 lbf. The normal average sea level acceleration on Earth (World Gravity Formula 1980) is 9.79764 m/s², so on average at sea level on Earth, 1.0000 lb will exert a force of 0.9991 lbf.
The equivalence 1 lb = 0.453 592 37 kg is always true, anywhere in the universe. If you borrow the acceleration which is official for defining kilograms force to define pounds force as well, then the same relationship will hold between poundsforce and kilogramsforce (an old nonSI unit which we still see used). If a different value is used to define pounds force, then the relationship to kilograms force will be slightly different—but in any case, that relationship is also a constant anywhere in the universe. What is not constant throughout the universe is the amount of force in terms of poundsforce (or any other force units) which 1 lb will exert due to gravity.
By analogy with the slug, there is a rarely used unit of mass called the "metric slug". This is the mass that accelerates at one metre per second squared when pushed by a force of one kgf. An item with a mass of 10 kg has a mass of 1.01972661 metric slugs (= 10 kg divided by 9.80665 kg per metric slug). This unit is also known by various other names such as the hyl, TME (from a German acronym), and mug (from metric slug).
Another unit of force called the poundal (pdl) is defined as the force that accelerates 1 lbm at 1 foot per second squared. Given that 1 lbf = 32.174 lb times one foot per second squared, we have 1 lbf = 32.174 pdl.
In conclusion, we have the following conversions:
 1 kgf (kilopond kp) = 9.80665 newtons
 1 metric slug = 9.80665 kg
 1 lbf = 32.174 poundals
 1 slug = 32.174 lb
 1 kgf = 2.2046 lbf
Forces in everyday life
Forces are part of everyday life, with examples such as:
 gravity: objects fall, even after being thrown upwards, objects slide and roll down
 friction: floors and objects are not extremely slippery
 spring force, objects resist tensile stress, compressive stress and/or shear stress, objects bounce back.
 electromagnetic force: attraction of magnets
 movement created by force: the movement of objects when force is applied.
Forces in industry
<to be completed>
Forces in the laboratory
Founding experiments
 Galileo Galilei uses rolling balls to disprove the Aristotelian theory of motion (1602  1607)
 Henry Cavendish's torsion bar experiment measured the force of gravity between 2 masses (1798)
Instruments to measure forces
spring ,forcemeter and spring balance
Forces in theory
Force, usually represented with the symbol F, is a vector quantity.
Newton's second law of motion can be formulated as follows:
 F = m · a
where
 F is the force, measured in newtons
 a is the acceleration, measured in metre per second squared
The total (Newtonian) force, in newtons, on an object at any given time is defined as the rate of change of the object's velocity multiplied by the object's mass:
 <math>\mathbf{F} = \lim_{T \rightarrow 0 } \frac{m\mathbf{v}  m\mathbf{v}_0}{T}<math>
where
 m is the inertial mass of the particle (measured in kilograms)
 v_{o} is its initial velocity (measured in metres per second)
 v is its final velocity (measured in metres per second)
 T is the time from the initial state to the final state (measured in seconds);
 Lim T→0 is the limit as T tends towards zero.
Force was so defined in order that its reification would explain the effects of superimposing situations: If in one situation, a force is experienced by a particle, and if in another situation another force is experienced by that particle, then in a third situation, which (according to standard physical practice) is taken to be a combination of the two individual situations, the force experienced by the particle will be the vector sum of the individual forces experienced in the first two situations. This superposition of forces, and the definition of inertial frames and inertial mass, are the empirical content of Newton's laws of motion.
The content of above definition of force can be further explicated. First, the mass of a body times its velocity is designated its momentum (labeled p). So the above definition can be written:
 <math>\textbf{F}={\Delta \textbf{p} \over \Delta t}<math>
If F is not constant over Δt, then this is the definition of average force over the time interval. To apply it at an instant we apply an idea from Calculus. Graphing p as a function of time, the average force will be the slope of the line connecting the momentum at two times. Taking the limit as the two times get closer together gives the slope at an instant, which is called the derivative:
 <math>\textbf{F}={d\textbf{p}\over dt}<math>
With many forces a potential energy field is associated. For instance, the gravitational force acting upon a body can be seen as the action of the gravitational field that is present at the body's location. The potential field is defined as that field whose gradient is minus the force produced at every point:
 <math>\textbf{F}=\nabla U<math>
While force is the name of the derivative of momentum with respect to time, the derivative of force with respect to time is sometimes called yank. Higher order derivates can be considered, but they lack names, because they are not commonly used.
In most expositions of mechanics, force is usually defined only implicitly, in terms of the equations that work with it. Some physicists, philosophers and mathematicians, such as Ernst Mach, Clifford Truesdell and Walter Noll, have found this problematic and sought a more explicit definition of force.
NonSI usage of force and mass units
The kilogramforce is a unit of force that was used in various fields of science and technology. In 1901, the CGPM made kilogramforce well defined, by adopting a standard acceleration of gravity for this purpose, making the kilogramforce equal to the force exerted by a mass of 1 kg when accelerated by 9.80665 m/s². The kilogramforce is not a part of the modern SI system, but vestiges of its use can still occur in:
 Thrust of jet and rocket engines
 Spoke tension of bicycles
 Draw weight of bows
 Torque wrenches in units such as "meter kilograms" or "kilogram centimetres" (the kilograms are rarely identified as unit of force)
 Engine torque output (kgf·m expressed in various word order, spelling, and symbols)
 Pressure gauges in "kg/cm²" or "kgf/cm²"
In colloquial, nonscientific usage, the "kilograms" used for "weight" are almost always the proper SI units for this purpose. They are units of mass, not units of force.
The symbol "kgm" for kilograms is also sometimes encountered. This might occasionally be an attempt to disintinguish kilograms as units of mass from the "kgf" symbol for the units of force. It might also be used as a symbol for those obsolete torque units (kilogramforce metres) mentioned above, used without properly separating the units for kilogram and metre with either a space or a centered dot.
History
Force was first described by Archimedes.
See also
External link
 Calculation: force F  English and American units to metric units (http://jumk.de/calc/force.shtml)
 Online Unit Converter  Conversion of many different units (http://calc.skyrocket.de/en/)bg:????
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