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In classical mechanics, momentum (pl. momenta; SI unit kg·m/s, or, equivalently, N·s) is the product of the mass and velocity of an object (p = mv). For more accurate measures of momentum, see the section "modern definitions of momentum" on this page. It is sometimes referred to as linear momentum to distinguish it from the related subject of angular momentum. Linear momentum is a vector quantity, since it has a direction as well as a magnitude. Angular momentum is a pseudovector quantity because it gains an additional sign flip under an improper rotation. The total momentum of any group of objects remains the same unless outside forces act on the objects (law of conservation of momentum).

Momentum is a conserved quantity, meaning that the total momentum of any closed system (one not affected by external forces) cannot change. This law is also true in special relativity.

The mōmentum was not merely the motion, which was mōtus, but was the power residing in a moving object, captured by today's mathematical definitions. A mōtus, "movement", was a stage in any sort of change, while velocitas, "swiftness", captured only speed. The Romans, due to limitations inherent in the Roman numeral system, were unable to go further with the perception.

The concept of momentum in classical mechanics was originated by a number of great thinkers and experimentalists. The first of these was Ibn Sina (Avicenna) circa 1000, who referred to impetus as proportional to weight times velocity. René Descartes later referred to mass times velocity as the fundamental force of motion. Galileo in his Two New Sciences used the Italian word "impeto."

The question has been much debated as to what Isaac Newton's contribution to the concept was. The answer is apparently nothing, except to state more fully and with better mathematics what was already known. The first and second of Newton's Laws of Motion had already been stated by John Wallis in his 1670 work, Mechanica slive De Motu, Tractatus Geometricus: "the initial state of the body, either of rest or of motion, will persist" and "If the force is greater than the resistance, motion will result". Wallis uses momentum and vis for force.

Newton's Philosophiæ Naturalis Principia Mathematica, when it was first published in 1686, showed a similar casting around for words to use for the mathematical momentum. His Definition II defines quantitas motus, "quantity of motion", as "arising from the velocity and quantity of matter conjointly", which identifies it as momentum. Thus when in Law II he refers to mutatio motus, "change of motion", being proportional to the force impressed, he is generally taken to mean momentum and not motion.

It remained only to assign a standard term to the quantity of motion. The first use of "momentum" in its proper mathematical sense is not clear but by the time of Jenning's Miscellanea in 1721, four years before the final edition of Newton's Principia Mathematica, momentum M or "quantity of motion" was being defined for students as "a rectangle", the product of Q and V where Q is "quantity of material" and V is "velocity", s/t.

Some languages, such as Italian, still lack a single term for momentum, and use a phrase such as the literal translation of "quantity of motion".

If an object is moving in any reference frame, then it has momentum in that frame. It is important to note that momentum is frame dependent. That is, the same object may have a certain momentum in one frame of reference, but a different amount in another frame. For example, a moving object has momentum in a reference frame fixed to a spot on the ground, while at the same time having 0 momentum in a reference frame attached to the object's center of mass.

The amount of momentum that an object has depends on two physical quantities: the mass and the velocity of the moving object in the frame of reference. In physics, the usual symbol for momentum is a small bold p (bold because it is a vector); so this can be written

- $mathbf\{p\}=\; m\; mathbf\{v\}$

Example: a model airplane of 1 kg travelling due north at 1 m/s in straight and level flight has a momentum of 1 kg m/s due north measured from the ground. To the dummy pilot in the cockpit it has a velocity and momentum of zero.

According to Newton's second law the rate of change of the momentum of a particle is proportional to the resultant force acting on the particle and is in the direction of that force. In the case of constant mass, and velocities much less than the speed of light, this definition results in the equation

- $sum\{mathbf\{F\}\}\; =\; \{mathrm\{d\}mathbf\{p\}\; over\; mathrm\{d\}t\}\; =\; m\{mathrm\{d\}mathbf\{v\}\; over\; mathrm\{d\}t\}\; =\; mmathbf\{a\}$

or just simply

- $mathbf\{F\}=\; m\; mathbf\{a\}$

Example: a model airplane of 1 kg accelerates from rest to a velocity of 1 m/s due north in 1 s. The thrust required to produce this acceleration is 1 newton. The change in momentum is 1 kg m/s. To the dummy pilot in the cockpit there is no change of momentum. Its pressing backward in the seat is a reaction to the unbalanced thrust, shortly to be balanced by the drag.

- $mathbf\{P\}=\; sum\_\{i\; =\; 1\}^n\; m\_i\; mathbf\{v\}\_i\; =\; m\_1\; mathbf\{v\}\_1\; +\; m\_2\; mathbf\{v\}\_2\; +\; m\_3\; mathbf\{v\}\_3\; +\; cdots\; +\; m\_n\; mathbf\{v\}\_n$

It can be shown that, in the center of mass frame the momentum of a system is zero. Additionally, the momentum in a frame of reference that is moving at a velocity v_{cm} with respect to that frame is simply:

- $mathbf\{P\}=\; Mmathbf\{v\}\_text\{cm\}$

- $M=sum\_\{i\; =\; 1\}^n\; m\_i$.

The linear momentum of a system of particles can also be defined as the product of the total mass $M$ of the system times the velocity of the center of mass $mathbf\{v\}\_\{cm\}$

- $sum\{mathbf\{F\}\}\; =\; \{mathrm\{d\}mathbf\{P\}\; over\; mathrm\{d\}t\}=\; M\; frac\{mathrm\{d\}mathbf\{v\}\_\{cm\}\}\{mathrm\{d\}t\}=Mmathbf\{a\}\_\{cm\}$

This is commonly known as Newton's second law.

For a more general derivation using tensors, we consider a moving body (see Figure), assumed as a continuum, occupying a volume $V$ at a time $t$, having a surface area $S$, with defined traction or surface forces $T\_i^\{(n)\}$ acting on every point of the body surface, body forces $F\_i$ per unit of volume on every point within the volume $V$, and a velocity field $v\_i$ prescribed throughout the body. Following the previous equation, The linear momentum of the system is:

- $int\_S\; T\_i^\{(n)\}dS\; +\; int\_V\; F\_i\; dV\; =\; int\_V\; rho\; frac\{d\; v\_i\}\{dt\}\; ,\; dV$

By definition the stress vector is $T\_i^\{(n)\}\; =sigma\_\{ij\}n\_j$, then

- $int\_S\; sigma\_\{ij\}n\_j\; ,\; dS\; +\; int\_V\; F\_i\; ,\; dV\; =\; int\_V\; rho\; frac\{d\; v\_i\}\{dt\}\; ,\; dV$

Using the Gauss's divergency theorem to convert a surface integral to a volume integral gives

- $int\_V\; sigma\_\{ij,j\}\; ,\; dV\; +\; int\_V\; F\_i\; ,\; dV\; =\; int\_V\; rho\; frac\{d\; v\_i\}\{dt\}\; ,\; dV$

- $int\_V\; sigma\_\{ij,j\}\; +\; F\_i\; -\; rho\; frac\{d\; v\_i\}\{dt\},\; dV\; =\; 0$

For an arbitrary volume the integrand itself must be zero, and we have the Cauchy's equation of motion

- $sigma\_\{ij,j\}\; +\; F\_i\; =\; rho\; frac\{d\; v\_i\}\{dt\}$

If a system is in equilibrium, the change in momentum with respect to time is equal to 0, as there is no acceleration.

- $sum\{mathbf\{F\}\}\; =\; \{mathrm\{d\}mathbf\{P\}\; over\; mathrm\{d\}t\}=\; Mmathbf\{a\}\_\{cm\}=\; 0$

or using tensors,

- $sigma\_\{ij,j\}\; +\; F\_i\; =\; 0$

These are the equilibrium equations which are used in solid mechanics for solving problems of linear elasticity. In engineering notation, the equilibrium equations are expressed in Cartesian coordinates as

- $frac\{partial\; sigma\_x\}\{partial\; x\}\; +\; frac\{partial\; tau\_\{yx\}\}\{partial\; y\}\; +\; frac\{partial\; tau\_\{zx\}\}\{partial\; z\}\; +\; F\_x\; =\; 0$

- $frac\{partial\; tau\_\{xy\}\}\{partial\; x\}\; +\; frac\{partial\; sigma\_y\}\{partial\; y\}\; +\; frac\{partial\; tau\_\{zy\}\}\{partial\; z\}\; +\; F\_y\; =\; 0$

- $frac\{partial\; tau\_\{xz\}\}\{partial\; x\}\; +\; frac\{partial\; tau\_\{yz\}\}\{partial\; y\}\; +\; frac\{partial\; sigma\_z\}\{partial\; z\}\; +\; F\_z\; =\; 0$

Conservation of momentum is a mathematical consequence of the homogeneity (shift symmetry) of space (position in space is the canonical conjugate quantity to momentum). So, momentum conservation can be philosophically stated as "nothing depends on location per se".

In an isolated system (one where external forces are absent) the total momentum will be constant: this is implied by Newton's first law of motion. Newton's third law of motion, the law of reciprocal actions, which dictates that the forces acting between systems are equal in magnitude, but opposite in sign, is due to the conservation of momentum.

Since position in space is a vector quantity, momentum (being the canonical conjugate of position) is a vector quantity as well - it has direction. Thus, when a gun is fired, the final total momentum of the system (the gun and the bullet) is the vector sum of the momenta of these two objects. Assuming that the gun and bullet were at rest prior to firing (meaning the initial momentum of the system was zero), the final total momentum must also equal 0.

In an isolated system with only two objects, the change in momentum of one object must be equal and opposite to the change in momentum of the other object. Mathematically,

$Delta\; mathbf\{p\}\_1\; =\; -Delta\; mathbf\{p\}\_2$

Momentum has the special property that, in a closed system, it is always conserved, even in collisions and separations caused by explosive forces. Kinetic energy, on the other hand, is not conserved in collisions if they are inelastic. Since momentum is conserved it can be used to calculate an unknown velocity following a collision or a separation if all the other masses and velocities are known.

A common problem in physics that requires the use of this fact is the collision of two particles. Since momentum is always conserved, the sum of the momenta before the collision must equal the sum of the momenta after the collision:

- $m\_1\; mathbf\; u\_\{1\}\; +\; m\_2\; mathbf\; u\_\{2\}\; =\; m\_1\; mathbf\; v\_\{1\}\; +\; m\_2\; mathbf\; v\_\{2\}\; ,$

- u signifies vector velocity before the collision

- v signifies vector velocity after the collision.

Usually, we either only know the velocities before or after a collision and would like to also find out the opposite. Correctly solving this problem means you have to know what kind of collision took place. There are two basic kinds of collisions, both of which conserve momentum:

- Elastic collisions conserve kinetic energy as well as total momentum before and after collision.
- Inelastic collisions don't conserve kinetic energy, but total momentum before and after collision is conserved.

- $begin\{matrix\}frac\{1\}\{2\}end\{matrix\}\; m\_1\; v\_\{1,i\}^2$

Since the 1/2 factor is common to all the terms, it can be taken out right away.

- $v\_\{1,f\}\; =\; left(frac\{m\_1\; -\; m\_2\}\{m\_1\; +\; m\_2\}\; right)\; v\_\{1,i\}\; +\; left(frac\{2\; m\_2\}\{m\_1\; +\; m\_2\}\; right)\; v\_\{2,i\}\; ,$

- $v\_\{2,f\}\; =\; left(frac\{2\; m\_1\}\{m\_1\; +\; m\_2\}\; right)\; v\_\{1,i\}\; +\; left(frac\{m\_2\; -\; m\_1\}\{m\_1\; +\; m\_2\}\; right)\; v\_\{2,i\}\; ,$

which can then easily be rearranged to

- $m\_\{1\}\; cdot\; v\_\{1,f\}\; +\; m\_\{2\}\; cdot\; v\_\{2,f\}\; =\; m\_\{1\}\; cdot\; v\_\{1,i\}\; +\; m\_\{2\}\; cdot\; v\_\{2,i\},$

Now consider the case when the mass of one body, say m_{1}, is far greater than that of the other, m_{2} (m_{1}>>m_{2}).
In that case, both m_{1}+m_{2} and m_{1}-m_{2} are approximately equal to m_{1}.

Using these approximations, the above formula for $v\_\{2,mathrm\{f\}\}$ reduces to $v\_\{2,mathrm\{f\}\}=2v\_\{1,mathrm\{i\}\}-v\_\{2,mathrm\{i\}\}$. Its physical interpretation is that in the case of a collision between two bodies, one of which is much more massive than the other, the lighter body ends up moving in the opposite direction with twice the original speed of the more massive body.

Another special case is when the collision is between two bodies of equal mass.

Say body m1 moving at velocity v_{1} strikes body m_{2} that is at rest (v_{2}).
Putting this case in the equation derived above we will see that after the collision, the body that was moving (m_{1}) will start moving with velocity v_{2} and the mass m_{2} will start moving with velocity v_{1}. So there will be an exchange of velocities.

Now suppose one of the masses, say m_{2}, was at rest. In that case after the collision the moving body, m_{1}, will come to rest and the body that was at rest, m_{2}, will start moving with the velocity that m_{1} had before the collision.

Note that all of these observations are for an elastic collision.

This phenomenon is demonstrated by Newton's cradle, one of the best known examples of conservation of momentum, a real life example of this special case.

For example, in a two-dimensional collision, the momenta can be resolved into x and y components. We can then calculate each component separately, and combine them to produce a vector result. The magnitude of this vector is the final momentum of the isolated system.

- $m\_1\; mathbf\; v\_\{1,i\}\; +\; m\_2\; mathbf\; v\_\{2,i\}\; =\; left(m\_1\; +\; m\_2\; right)\; mathbf\; v\_f\; ,$

In case of Inelastic collision, there is a parameter attached called coefficient of restitution (denoted by small 'e' or 'c' in many text books). It is defined as the ratio of relative velocity of separation to relative velocity of approach. It is a ratio hence it is a dimensionless quantity.

When we have an elastic collision the value of e (= coefficient of restitution) is 1, i.e. the relative velocity of approach is same as the relative velocity of separation of the colliding bodies. In an elastic collision the Kinetic energy of the system is conserved.

When a collision is not elastic (e<1) it is an inelastic collision. In case of a perfectly inelastic collision the relative velocity of separation of the centre of masses of the colliding bodies is 0. Hence after collision the bodies stick together after collision. In case of an inelastic collision the loss of Kinetic energy is maximum as stated above.

In all types of collision if no external force is acting on the system of colliding bodies, the momentum will always be preserved.

http://www.glenbrook.k12.il.us/gbssci/phys/Class/momentum/u4l2e.html

In the exploding cannon demonstration, total system momentum is conserved. The system consists of two objects - a cannon and a tennis ball. Before the explosion, the total momentum of the system is zero since the cannon and the tennis ball located inside of it are both at rest. After the explosion, the total momentum of the system must still be zero. If the ball acquires 50 units of forward momentum, then the cannon acquires 50 units of backwards momentum. The vector sum of the individual momenta of the two objects is 0. Total system momentum is conserved.

See the inelastic collision page for more details.

- $mathbf\{p\}\; =\; gamma\; m\_0mathbf\{v\}$

- $m\_0,$ is the invariant mass of the object moving,

- $gamma\; =\; frac\{1\}\{sqrt\{1\; -\; frac\{v^2\}\{c^2\}\}\}$ is the Lorentz factor

- $v,$ is the relative velocity between an object and an observer

- $c,$ is the speed of light.

Relativistic momentum can also be written as invariant mass times the object's proper velocity, defined as the rate of change of object position in the observer frame with respect to time elapsed on object clocks (i.e. object proper time). Relativistic momentum becomes Newtonian momentum: $mmathbf\{v\}$ at low speed $big(mathbf\{v\}/c\; rightarrow\; 0\; big)$.

Relativistic four-momentum as proposed by Albert Einstein arises from the invariance of four-vectors under Lorentzian translation. The four-momentum is defined as:

- $left(\{E\; over\; c\}\; ,\; p\_x\; ,\; p\_y\; ,p\_z\; right)$

where

- $p\_x,$ is the $x,$ component of the relativistic momentum,

- $E\; ,$ is the total energy of the system:

- $E\; =\; gamma\; m\_0c^2\; ,$

The "length" of the vector is the mass times the speed of light, which is invariant across all reference frames:

- $(E/c)^2\; -\; p^2\; =\; (m\_0c)^2,$

Momentum of massless objects

Objects without a rest mass, such as photons, also carry momentum. The formula is:

- $p\; =\; frac\{h\}\{lambda\}\; =\; frac\{E\}\{c\}$

- $h,$ is Planck's constant,

- $lambda,$ is the wavelength of the photon,

- $E,$ is the energy the photon carries and

- $c,$ is the speed of light.

Generalization of momentum

Momentum is the Noether charge of translational invariance. As such, even fields as well as other things can have momentum, not just particles. However, in curved space-time which is not asymptotically Minkowski, momentum isn't defined at all.

For a single particle with no electric charge and no spin, the momentum operator can be written in the position basis as

- $mathbf\{p\}=\{hbarover\; i\}nabla=-ihbarnabla$

where:

- $nabla$ is the gradient operator;
- $hbar$ is the reduced Planck constant;
- $i$, defined as $i^2\; =\; -1$, is the imaginary unit.

This is a commonly encountered form of the momentum operator, though not the most general one.

- $P\_\{static\}\; =\; \{W\}=\; left[\{epsilon\_0\; epsilon\}\{frac\{\{mathbf\; E\}^2\; \}\{\; \{2\}\}\}\; +\{frac\{\; 1\; \}\{\; \{mu\_0\; mu\}\; \}\}\; \{frac\{\{mathbf\; B\}^2\}\}\; right],$

Light (visible, UV, radio) is an electromagnetic wave and also has momentum. Even though photons (the particle aspect of light) have no mass, they still carry momentum. This leads to applications such as the solar sail.

Momentum is conserved in an electrodynamic system (it may change from momentum in the fields to mechanical momentum of moving parts). The treatment of the momentum of a field is usually accomplished by considering the so-called energy-momentum tensor and the change in time of the Poynting vector integrated over some volume. This is a tensor field which has components related to the energy density and the momentum density.

The definition canonical momentum corresponding to the momentum operator of quantum mechanics when it interacts with the electromagnetic field is, using the principle of least coupling:

- $mathbf\; P\; =\; mmathbf\; v\; +\; qmathbf\; A$,

- $mathbf\; p\; =\; mmathbf\; v$,

- $mathbf\; A$ is the electromagnetic vector potential

- $m$ the charged particle's invariant mass

- $mathbf\; v$ its velocity

- $q$ its charge.

- Halliday, David; Robert Resnick
*Fundamentals of Physics*. John Wiley & Sons. - Serway, Raymond; Jewett, John (2003). Physics for Scientists and Engineers (6 ed.). Brooks Cole. ISBN 0-534-40842-7
- Stenger, Victor J. (2000). Timeless Reality: Symmetry, Simplicity, and Multiple Universes. Prometheus Books. Chpt. 12 in particular.
- Tipler, Paul (1998). Physics for Scientists and Engineers: Vol. 1: Mechanics, Oscillations and Waves, Thermodynamics (4th ed.). W. H. Freeman. ISBN 1-57259-492-6
- 'H C Verma' 'Concepts of Physics, Part 1' 'Bharti Bhawan'
- For numericals refer 'IE Irodov','Problems in General Physics'

- Conservation of momentum - A chapter from an online textbook
- Demonstration of calculation of Momentum
- Planck units expressed as geometry of momentum

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Last updated on Thursday October 09, 2008 at 18:55:36 PDT (GMT -0700)

View this article at Wikipedia.org - Edit this article at Wikipedia.org - Donate to the Wikimedia Foundation

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