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Mass

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Mass

From Wikipedia, the free encyclopedia.

Mass is a property of physical objects which, roughly speaking, measure the amount of matter contained in an object. It is a central concept of classical mechanics and related subjects. In the SI system of measurement, mass is measured in kilograms.

Strictly speaking, mass refers to two quantities:

Inertial mass is a measure of an object's inertia, which is its resistance to changing its state of motion when a force is applied. An object with small inertial mass changes its motion more readily, and an object with large inertial mass does so less readily.
Gravitational mass is a measure of the strength of an object's interaction with the gravitational force. Within the same gravitational field, an object with a smaller gravitational mass experiences a smaller force than an object with a larger gravitational mass. (This quantity is sometimes confused with weight.)

Inertial and gravitational mass have been experimentally shown to be equivalent, as accurately as we can measure, although they are conceptually quite distinct. Below, we will discuss the definitions and implications of each of these two quantities.

Inertial Mass

Inertial mass is determined using Newton's second and third laws of motion (see classical mechanics.) Given an object with a known inertial mass, we can obtain the inertial mass of any other object by making the two objects exert a force on each other. According to Newton's third law, the forces experienced by each object will have equal magnitude. This allows us to study how the two objects resist similar applied forces.

Suppose we have two objects, A and B, with inertial masses m_A (which is known) and m_B (which we wish to determine.) We will assume these masses to be constant. We isolate the two objects from all other physical influences, so that the only forces present are the force exerted on A by B, which we denote F_AB, and the force exerted on B by A, which we denote F_BA. According to Newton's second law,

F_AB = m_Aa_A

F_BA = m_Ba_B.

where a_A and a_B are the accelerations of A and B respectively. To proceed, we must ensure that these accelerations are non-zero, i.e. that the forces between the two objects are non-zero. This may be done, for example, by having the two objects collide and performing our measurements during the collision.

Newton's third law states that the two forces are equal and opposite, i.e.

F_AB = - F_BA.

When substituted into the above equations, this yields the mass of B as

$m_B = {a_A \over a_B} m_A$ .

Thus, measuring a_A and a_B allows us to determine m_A in terms of m_B, as desired. Note that our above requirement, that a_B be non-zero, allows this equation to be well-defined.

In the above discussion, we assumed that the masses of A and B are constant. This is a fundamental assumption, known as the conservation of mass, and is based on the expectation that matter can never be created or destroyed, only split up or recombined. (The implications of special relativity are discussed below.) It is sometimes useful to treat the mass of an object as changing with time: for example, the mass of a rocket decreases as the rocket fires. However, this is an approximation based on ignoring pieces of matter which enter or leave the system. In the case of the rocket, these pieces correspond to the ejected propellent; if we were to measure the total mass of the rocket and its propellent, we would find that it is conserved.

Gravitational Mass

Consider two objects A and B with gravitational masses M_A and M_B, at a distance of |r_AB| apart. Newton's law of gravitation states that the magnitude of the gravitational force which each object exerts on the other is

$|F| = {G M_A M_B \over |r_{AB}|}$

where G is the universal gravitational constant. The above statement may be reformulated in the following way: given the acceleration g of a reference mass in a gravitational field (such as the gravitational field of the Earth), the gravitational force on an object with gravitational mass M has magnitude

| F | = Mg.

This is the basis by which masses are determined by weighing. In simple bathroom scales, for example, the force |F| is proportionate to the displacement of the spring beneath the weighing pan (see Hooke's law), and the scales are calibrated to take g into account, allowing the mass M to be read off.

Equivalence of Inertial and Gravitational Masses

Experiments have found inertial and gravitational mass to be equal, to a high level of precision. These experiments are essentially tests of the well-known phenomenon, first observed by Galileo, that objects fall at a rate irrespective of their masses (in the absence of factors such as friction.) Suppose we have an object with inertial and gravitational masses m and M respectively. If gravity is the only force acting on the object, the combination of Newton's second law and gravitational law gives its acceleration a as

$a = {M \over m}g$

Therefore, all objects in the same gravitational field fall at the same rate if and only if the ratio of gravitational and inertial mass is always equal to some fixed constant. We may as well take this ratio to be 1, by definition.

Consequences of Relativity

In the special theory of relativity, "mass" refers to the inertial mass of an object as measured in the frame of reference in which it is at rest (which is known as its "rest frame".) The above method for determining inertial masses remains valid, provided we ensure that the speed of the object is always much smaller than the speed of light, so that classical mechanics is valid.

Historically, the term "mass" was used for the quantity E/c². This was called the "relativistic mass", and m called the "rest mass". This terminology is now discouraged by physicists, because there is no need for two terms for the energy of a particle, and because it creates confusion when speaking of "massless" particles. In this article, we will always mean the rest mass whenever we refer to "mass". For more details, see the Usenet Relativity FAQ in the External Links.

In relativistic mechanics, the mass of a free particle is related to its energy and momentum by the following equation:

${E^2 \over c^2} = m^2 c^2 + p^2$ .

This equation can be rearranged in the following way:

$E = mc^2 \sqrt{1 + ({p \over mc})^2}$

The classical limit corresponds to the situation in which the momentum p is much smaller than mc, in which case we can Taylor expand the square root, resulting in

$E = mc^2 + {p^2 \over 2m} + ...$

The leading term, which is the largest, is the rest energy of the particle. Provided the mass is non-zero, a particle always has this minimum amount of energy regardless of its momentum. The rest energy is normally inaccessible, but it can be tapped by splitting or combining particles, as is done during nuclear fusion and fission. The second term is simply the classical kinetic energy, which can be demonstrated by using the classical definition of momentum

p = mv

and substituting it into the above to give:

$E = mc^2 + {mv^2 \over 2} + ...$

The relativistic energy-mass-momentum relation can also account for particles that are massless, which is an ill-defined concept in classical mechanics. When m = 0, the relation can be simplified to

E = pc

where p is the relativistic momentum.

This equation governs the mechanics of massless particles such as photons, the particles of light.

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