Online Encyclopedia
Force
- For other uses, see Force (disambiguation).
In physics, a net force acting on a body causes that body to accelerate; that is, to change its velocity. The concept appeared first in the second law of motion of classical mechanics. It is usually expressed by the equation
F = m · a
where
F is the force, measured in newtons
m is the mass, measured in kilograms
a is the acceleration, measured in metre per second squared
The concept is much used in engineering, although scientists have developed more accurate concepts. Force is not a fundamental quantity in physics, despite the tendency to introduce students to physics via this concept. More fundamental are momentum, energy and stress. Force is rarely measured directly and is often confused with related concepts such as tension and stress.
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Forces in applications
Types of forces
Engineers uses many types of force: Coulomb's force between 2 electrical charges, gravity between 2 masses, magnetic force, friction, spring force, ...
Yet, scientists consider that there are only 3 fundamental forces of nature, with which every observed phenomenon can be explained: the strong nuclear force, the electromagnetic force, and the weak nuclear force. Gravity is not really a force, in the sense that it cannot be adequately modelled using advanced versions of Newton's laws: general relativity is used instead.
Pressure is a force applied over a surface. Some forces are conservative, others not.
Properties of force
Forces have an intensity and direction.
Forces can be added together using parallelogram of force. When two forces act on an object, the resulting force (called the resultant) is the vector sum of the original forces. The magnitude of the resultant varies from zero to the sum of the magitudes 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, and the object moves at a constant speed (possibly, but not necessarily zero).
While forces can be added together, they can also be resolved into components. For example, an horizontal force acting in the direction of northeast can be split into two forces along the north and east directions respectively. The sum of these component forces is equal to the original force.
Units of measure
The SI unit used to measure force is the newton (symbol N), which is equivalent to kg·m·s^{−2}
Imperial units of force and mass
The relationship F=m·a mentioned above may also be used with non-metric units. If those units do not form a consistent set of units, the more general form F=k·m·a must be used, where the constant k is a conversion factor dependent upon the units used.
For example, in imperial engineering units, F is in "pounds force" or "lbf", m is in "pounds mass" or "lb", and a is in feet per second squared. However, in this particular system, you need 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 pounds-force and kilograms-force (an old non-SI 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 pounds-force (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 [Kilogram force|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:
- 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
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
<to be completed>
Forces in theory
Force, usually represented with the symbol F, is a vector quantity.
Forces in theoretical physics
It is very important to mention that it is impossible to define force. All attempts in history failed because of definitions in circles. This is a reason why modern physics theories don't operate with the forces as the source or symptom of interaction. General relativity uses a conception of curved spacetime and Quantum field theory talks about exchanging of intermediate particles like photons, W and Z bosons or gluons. Both theories don't need force. However, because it is easy to imagine forces, one can compute them from these theories. But we must not forget, that correct definition of this concept does not exist.
Fields of study
See also engineering mechanics:
- Statics Where the sum of the forces acting on a body in static equilibrium (motionless) is zero. F=m·a=0
- Dynamics The sum of the forces acting on a body or system over time is non-zero with a resulting set of accelerations defined by detailed analysis of equations derived from F=m·a=0.
Formula
Newton's second law of motion can be formulated as follows:
- F = m · a
where
F is the force, measured in newtons
m is the mass, measured in kilograms
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:
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:
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:
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:
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.
Non-SI usage of force and mass units
The kilogram-force is a unit of force that was used in various fields of science and technology. In 1901, the CGPM made kilogram-force well defined, by adopting a standard acceleration of gravity for this purpose, making the kilogram-force equal to the force exerted by a mass of 1 kg when accelerated by 9.80665 m/s². The kilogram-force 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, non-scientific 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 (kilogram-force 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://www.sengpielaudio.com/ConvForc.htm