Physics For Scientists And Engineers 6th Edition Tipler Pdf Free Download UPDATED

Physics For Scientists And Engineers 6th Edition Tipler Pdf Free Download

Process of free energy transfer to an object via force application through displacement

Piece of work
Baseball pitching motion 2004.jpg

A baseball pitcher does positive work on the ball by applying a force to information technology over the distance it moves while in his grip.

Common symbols

Westward
SI unit joule (J)

Other units

Foot-pound, Erg
In SI base units 1 kg⋅grand2⋅s−ii

Derivations from
other quantities

Due west = Fs
W = τ θ
Dimension M L 2 T −2

In physics, work is the energy transferred to or from an object via the awarding of force forth a displacement. In its simplest form, it is often represented as the product of strength and displacement. A force is said to do positive work if (when practical) it has a component in the management of the displacement of the betoken of awarding. A force does negative work if information technology has a component opposite to the direction of the displacement at the betoken of application of the strength.[ane]

For example, when a ball is held to a higher place the footing and and so dropped, the work washed by the gravitational force on the ball every bit it falls is equal to the weight of the brawl (a forcefulness) multiplied by the distance to the ground (a deportation). When the strength F is constant and the angle between the force and the displacement southward is θ, and then the work done is given by:

W = F s cos θ {\displaystyle W=Fs\cos {\theta }}

Work is a scalar quantity,[ii] so it has only magnitude and no direction. Piece of work transfers energy from one place to some other, or 1 course to another. The SI unit of work is the joule (J), the aforementioned unit as for energy.

History [edit]

The aboriginal Greek agreement of physics was limited to the statics of uncomplicated machines (the residuum of forces), and did non include dynamics or the concept of work. During the Renaissance the dynamics of the Mechanical Powers, as the simple machines were chosen, began to be studied from the standpoint of how far they could lift a load, in add-on to the force they could utilize, leading eventually to the new concept of mechanical work. The complete dynamic theory of elementary machines was worked out by Italian scientist Galileo Galilei in 1600 in Le Meccaniche (On Mechanics), in which he showed the underlying mathematical similarity of the machines equally force amplifiers.[three] [iv] He was the starting time to explain that simple machines do not create free energy, just transform it.[iii]

According to Jammer,[five] the term work was introduced in 1826 past the French mathematician Gaspard-Gustave Coriolis[half-dozen] as "weight lifted through a height", which is based on the use of early on steam engines to lift buckets of water out of flooded ore mines. According to Rene Dugas, French engineer and historian, it is to Solomon of Caux "that we owe the term piece of work in the sense that information technology is used in mechanics now".[7] Although work was not formally used until 1826, similar concepts existed before then. In 1759, John Smeaton described a quantity that he chosen "power" "to signify the exertion of strength, gravitation, impulse, or pressure, as to produce motion." Smeaton continues that this quantity tin be calculated if "the weight raised is multiplied by the height to which it can be raised in a given time," making this definition remarkably similar to Coriolis'.[8]

Units [edit]

The SI unit of work is the joule (J), named later on the 19th-century English physicist James Prescott Joule, which is divers equally the work required to exert a force of i newton through a displacement of one metre.

The dimensionally equivalent newton-metre (N⋅thou) is sometimes used as the measuring unit for work, but this can exist confused with the measurement unit of torque. Usage of Northward⋅m is discouraged past the SI dominance, since information technology can lead to confusion every bit to whether the quantity expressed in newton metres is a torque measurement, or a measurement of work.[9]

Not-SI units of work include the newton-metre, erg, the foot-pound, the human foot-poundal, the kilowatt hr, the litre-atmosphere, and the horsepower-60 minutes. Due to work having the same physical dimension equally rut, occasionally measurement units typically reserved for heat or energy content, such every bit therm, BTU and calorie, are utilized as a measuring unit.

Work and energy [edit]

The work West done by a abiding strength of magnitude F on a betoken that moves a deportation s in a straight line in the direction of the force is the product

W = F s . {\displaystyle W=Fs.}

For example, if a force of x newtons ( F = 10 N) acts forth a bespeak that travels ii metres ( s = 2 g), then West = Fs = (10 N) (2 chiliad) = twenty J. This is approximately the work washed lifting a i kg object from footing level to over a person's head against the force of gravity.

The work is doubled either past lifting twice the weight the same distance or past lifting the aforementioned weight twice the altitude.

Work is closely related to free energy. The piece of work–energy principle states that an increase in the kinetic energy of a rigid body is caused by an equal amount of positive work washed on the torso past the resultant force acting on that trunk. Conversely, a decrease in kinetic free energy is caused past an equal amount of negative work washed by the resultant force. Thus, if the net piece of work is positive, then the particle'southward kinetic energy increases by the corporeality of the piece of work. If the net work done is negative, then the particle's kinetic free energy decreases by the corporeality of work.[10]

From Newton'south 2d police force, it can be shown that work on a free (no fields), rigid (no internal degrees of freedom) body, is equal to the change in kinetic energy Ek corresponding to the linear velocity and angular velocity of that torso,

W = Δ E k . {\displaystyle Westward=\Delta E_{m}.}

The work of forces generated by a potential role is known as potential energy and the forces are said to be conservative. Therefore, work on an object that is simply displaced in a bourgeois forcefulness field, without alter in velocity or rotation, is equal to minus the change of potential free energy Ep of the object,

W = Δ Due east p . {\displaystyle W=-\Delta E_{p}.}

These formulas show that work is the energy associated with the activeness of a force, so work subsequently possesses the physical dimensions, and units, of energy. The work/energy principles discussed here are identical to electric piece of work/energy principles.

Constraint forces [edit]

Constraint forces determine the object'due south displacement in the system, limiting it within a range. For instance, in the instance of a slope plus gravity, the object is stuck to the slope and, when attached to a taut string, it cannot move in an outwards direction to make the string any 'tauter'. It eliminates all displacements in that direction, that is, the velocity in the direction of the constraint is limited to 0, so that the constraint forces do not perform work on the system.

For a mechanical system,[xi] constraint forces eliminate motility in directions that characterize the constraint. Thus the virtual work washed past the forces of constraint is nothing, a result which is only true if friction forces are excluded.[12]

Fixed, frictionless constraint forces exercise non perform work on the organisation,[13] equally the angle between the motion and the constraint forces is always 90°.[13] Examples of workless constraints are: rigid interconnections between particles, sliding move on a frictionless surface, and rolling contact without slipping.[14]

For example, in a pulley system like the Atwood machine, the internal forces on the rope and at the supporting pulley do no piece of work on the system. Therefore, work demand only be computed for the gravitational forces interim on the bodies. Another instance is the centripetal strength exerted inwards by a string on a ball in uniform circular motion sideways constrains the ball to circular move restricting its motility away from the centre of the circle. This forcefulness does cypher work because it is perpendicular to the velocity of the ball.

The magnetic force on a charged particle is F = q v × B , where q is the charge, five is the velocity of the particle, and B is the magnetic field. The result of a cross product is ever perpendicular to both of the original vectors, so Fv . The dot product of two perpendicular vectors is ever nil, so the work West = Fv = 0, and the magnetic force does not do work. It can change the management of motion just never alter the speed.

Mathematical calculation [edit]

For moving objects, the quantity of work/time (power) is integrated along the trajectory of the point of awarding of the force. Thus, at any instant, the rate of the work done by a force (measured in joules/2nd, or watts) is the scalar production of the force (a vector), and the velocity vector of the point of awarding. This scalar product of forcefulness and velocity is known equally instantaneous power. Just as velocities may be integrated over time to obtain a total distance, by the central theorem of calculus, the full work along a path is similarly the time-integral of instantaneous power applied along the trajectory of the indicate of awarding.[xv]

Work is the result of a force on a point that follows a curve X, with a velocity v, at each instant. The small-scale amount of piece of work δW that occurs over an instant of fourth dimension dt is calculated equally

δ West = F d s = F v d t {\displaystyle \delta West=\mathbf {F} \cdot d\mathbf {southward} =\mathbf {F} \cdot \mathbf {v} dt}

where the F5 is the ability over the instant dt. The sum of these modest amounts of work over the trajectory of the point yields the work,

West = t 1 t two F v d t = t 1 t 2 F d s d t d t = C F d s , {\displaystyle W=\int _{t_{1}}^{t_{2}}\mathbf {F} \cdot \mathbf {five} dt=\int _{t_{1}}^{t_{two}}\mathbf {F} \cdot {\tfrac {d\mathbf {s} }{dt}}dt=\int _{C}\mathbf {F} \cdot d\mathbf {s} ,}

where C is the trajectory from x(t 1) to x(t 2). This integral is computed along the trajectory of the particle, and is therefore said to exist path dependent.

If the force is e'er directed forth this line, and the magnitude of the forcefulness is F, then this integral simplifies to

Westward = C F d s {\displaystyle West=\int _{C}F\,ds}

where southward is deportation along the line. If F is abiding, in addition to being directed along the line, then the integral simplifies further to

Due west = C F d s = F C d southward = F south {\displaystyle W=\int _{C}F\,ds=F\int _{C}ds=Fs}

where s is the displacement of the point along the line.

This calculation tin can exist generalized for a constant strength that is not directed forth the line, followed past the particle. In this case the dot product Fd s = F cos θ ds , where θ is the angle between the force vector and the direction of motility,[15] that is

W = C F d s = F s cos θ . {\displaystyle Westward=\int _{C}\mathbf {F} \cdot d\mathbf {s} =Fs\cos \theta .}

When a force component is perpendicular to the displacement of the object (such every bit when a body moves in a round path under a central force), no work is washed, since the cosine of 90° is zippo.[10] Thus, no work can be performed by gravity on a planet with a circular orbit (this is platonic, equally all orbits are slightly elliptical). Also, no piece of work is done on a body moving circularly at a constant speed while constrained by mechanical force, such every bit moving at constant speed in a frictionless ideal centrifuge.

Piece of work done by a variable force [edit]

Calculating the work as "forcefulness times straight path segment" would only apply in the most elementary of circumstances, as noted above. If strength is changing, or if the body is moving along a curved path, perhaps rotating and non necessarily rigid, so merely the path of the application point of the forcefulness is relevant for the piece of work washed, and but the component of the force parallel to the application point velocity is doing work (positive work when in the same direction, and negative when in the opposite direction of the velocity). This component of force can be described by the scalar quantity called scalar tangential component ( F cos(θ), where θ is the angle between the strength and the velocity). And so the almost general definition of piece of work can be formulated every bit follows:

Piece of work of a force is the line integral of its scalar tangential component along the path of its application point.
If the force varies (e.one thousand. compressing a spring) nosotros demand to utilise calculus to discover the work done. If the strength is given by F(x) (a function of x) and so the work washed past the force along the x-axis from a to b is:
W = a b F ( southward ) d s {\displaystyle W=\int _{a}^{b}\mathbf {F(s)} \cdot d\mathbf {south} }

Torque and rotation [edit]

A force couple results from equal and opposite forces, interim on 2 different points of a rigid trunk. The sum (resultant) of these forces may cancel, simply their result on the trunk is the couple or torque T. The work of the torque is calculated as

d W = T ω d t , {\displaystyle dW=\mathbf {T} \cdot {\boldsymbol {\omega }}\,dt,}

where the T ω is the power over the instant δt. The sum of these pocket-sized amounts of work over the trajectory of the rigid body yields the work,

W = t 1 t 2 T ω d t . {\displaystyle W=\int _{t_{1}}^{t_{ii}}\mathbf {T} \cdot {\boldsymbol {\omega }}\,dt.}

This integral is computed forth the trajectory of the rigid body with an athwart velocity ω that varies with time, and is therefore said to exist path dependent.

If the athwart velocity vector maintains a constant direction, and then it takes the form,

ω = ϕ ˙ S , {\displaystyle {\vec {\omega }}={\dot {\phi }}\mathbf {South} ,}

where φ is the angle of rotation near the abiding unit vector S. In this case, the work of the torque becomes,

W = t 1 t 2 T ω d t = t 1 t 2 T South d ϕ d t d t = C T S d ϕ , {\displaystyle W=\int _{t_{1}}^{t_{2}}\mathbf {T} \cdot {\boldsymbol {\omega }}\,dt=\int _{t_{1}}^{t_{2}}\mathbf {T} \cdot \mathbf {S} {\frac {d\phi }{dt}}dt=\int _{C}\mathbf {T} \cdot \mathbf {S} \,d\phi ,}

where C is the trajectory from φ(t 1) to φ(t 2). This integral depends on the rotational trajectory φ(t), and is therefore path-dependent.

If the torque T is aligned with the athwart velocity vector so that,

T = τ Due south , {\displaystyle \mathbf {T} =\tau \mathbf {S} ,}

and both the torque and angular velocity are constant, and so the work takes the form,[2]

W = t one t 2 τ ϕ ˙ d t = τ ( ϕ 2 ϕ ane ) . {\displaystyle West=\int _{t_{one}}^{t_{ii}}\tau {\dot {\phi }}dt=\tau (\phi _{2}-\phi _{i}).}

A forcefulness of constant magnitude and perpendicular to the lever arm

This result can be understood more simply by considering the torque equally arising from a forcefulness of constant magnitude F, existence applied perpendicularly to a lever arm at a altitude r, equally shown in the effigy. This force will deed through the distance forth the circular arc southward = , and so the piece of work done is

W = F southward = F r ϕ . {\displaystyle W=Fs=Fr\phi .}

Innovate the torque τ = Fr , to obtain

Westward = F r ϕ = τ ϕ , {\displaystyle W=Fr\phi =\tau \phi ,}

as presented higher up.

Find that only the component of torque in the direction of the athwart velocity vector contributes to the work.

Work and potential energy [edit]

The scalar product of a force F and the velocity 5 of its point of awarding defines the power input to a arrangement at an instant of fourth dimension. Integration of this power over the trajectory of the point of application, C = ten(t), defines the piece of work input to the arrangement by the strength.

Path dependence [edit]

Therefore, the work done by a force F on an object that travels along a curve C is given by the line integral:

W = C F d ten = t 1 t two F v d t , {\displaystyle W=\int _{C}\mathbf {F} \cdot d\mathbf {x} =\int _{t_{1}}^{t_{2}}\mathbf {F} \cdot \mathbf {v} dt,}

where dx(t) defines the trajectory C and v is the velocity along this trajectory. In general this integral requires that the path along which the velocity is defined, and so the evaluation of work is said to exist path dependent.

The time derivative of the integral for work yields the instantaneous power,

d W d t = P ( t ) = F 5 . {\displaystyle {\frac {dW}{dt}}=P(t)=\mathbf {F} \cdot \mathbf {v} .}

Path independence [edit]

If the work for an practical forcefulness is independent of the path, then the work done by the force, past the gradient theorem, defines a potential function which is evaluated at the start and end of the trajectory of the point of application. This ways that there is a potential role U(10), that can be evaluated at the two points x(t ane) and 10(t 2) to obtain the work over any trajectory between these 2 points. Information technology is tradition to define this role with a negative sign so that positive work is a reduction in the potential, that is

W = C F d x = ten ( t 1 ) x ( t 2 ) F d x = U ( x ( t 1 ) ) U ( x ( t 2 ) ) . {\displaystyle West=\int _{C}\mathbf {F} \cdot \mathrm {d} \mathbf {10} =\int _{\mathbf {x} (t_{1})}^{\mathbf {x} (t_{2})}\mathbf {F} \cdot \mathrm {d} \mathbf {x} =U(\mathbf {x} (t_{1}))-U(\mathbf {10} (t_{2})).}

The function U(x) is chosen the potential energy associated with the practical force. The force derived from such a potential function is said to exist conservative. Examples of forces that have potential energies are gravity and leap forces.

In this case, the gradient of work yields

Westward = U = ( U x , U y , U z ) = F , {\displaystyle \nabla W=-\nabla U=-\left({\frac {\fractional U}{\partial x}},{\frac {\partial U}{\partial y}},{\frac {\partial U}{\partial z}}\right)=\mathbf {F} ,}

and the force F is said to exist "derivable from a potential."[16]

Because the potential U defines a forcefulness F at every point ten in space, the set of forces is called a force field. The power applied to a body by a strength field is obtained from the gradient of the work, or potential, in the direction of the velocity 5 of the torso, that is

P ( t ) = U 5 = F v . {\displaystyle P(t)=-\nabla U\cdot \mathbf {5} =\mathbf {F} \cdot \mathbf {five} .}

Piece of work past gravity [edit]

Gravity F = mg does work W = mgh forth any descending path

In the absence of other forces, gravity results in a constant downward acceleration of every freely moving object. Nigh Earth'southward surface the acceleration due to gravity is k = 9.8 m⋅s−two and the gravitational force on an object of mass thousand is F g = mg . It is convenient to imagine this gravitational forcefulness concentrated at the middle of mass of the object.

If an object with weight mg is displaced upward or downward a vertical altitude y 2y one , the work W washed on the object is:

W = F g ( y ii y one ) = F yard Δ y = thou thousand Δ y {\displaystyle West=F_{k}(y_{2}-y_{1})=F_{g}\Delta y=mg\Delta y}

where Fyard is weight (pounds in imperial units, and newtons in SI units), and Δy is the change in superlative y. Notice that the work done by gravity depends only on the vertical motion of the object. The presence of friction does not affect the work done on the object past its weight.

Work by gravity in space [edit]

The force of gravity exerted by a mass Thousand on some other mass k is given by

F = One thousand M m r 3 r , {\displaystyle \mathbf {F} =-{\frac {GMm}{r^{3}}}\mathbf {r} ,}

where r is the position vector from G to m.

Let the mass one thousand move at the velocity v; then the work of gravity on this mass as it moves from position r(t i) to r(t 2) is given by

Westward = r ( t 1 ) r ( t 2 ) K Grand m r 3 r d r = t 1 t 2 Thou M thou r iii r v d t . {\displaystyle W=-\int _{\mathbf {r} (t_{1})}^{\mathbf {r} (t_{2})}{\frac {GMm}{r^{3}}}\mathbf {r} \cdot d\mathbf {r} =-\int _{t_{1}}^{t_{2}}{\frac {GMm}{r^{3}}}\mathbf {r} \cdot \mathbf {v} dt.}

Discover that the position and velocity of the mass thou are given by

r = r e r , five = d r d t = r ˙ e r + r θ ˙ e t , {\displaystyle \mathbf {r} =r\mathbf {e} _{r},\qquad \mathbf {5} ={\frac {d\mathbf {r} }{dt}}={\dot {r}}\mathbf {e} _{r}+r{\dot {\theta }}\mathbf {e} _{t},}

where e r and e t are the radial and tangential unit vectors directed relative to the vector from M to m, and we employ the fact that d e r / d t = θ ˙ east t . {\displaystyle d\mathbf {east} _{r}/dt={\dot {\theta }}\mathbf {east} _{t}.} Utilise this to simplify the formula for work of gravity to,

W = t one t two Thousand m M r 3 ( r e r ) ( r ˙ e r + r θ ˙ e t ) d t = t one t 2 G k Thou r three r r ˙ d t = K M m r ( t 2 ) M M m r ( t 1 ) . {\displaystyle Due west=-\int _{t_{i}}^{t_{two}}{\frac {GmM}{r^{3}}}(r\mathbf {e} _{r})\cdot ({\dot {r}}\mathbf {e} _{r}+r{\dot {\theta }}\mathbf {eastward} _{t})dt=-\int _{t_{one}}^{t_{2}}{\frac {GmM}{r^{3}}}r{\dot {r}}dt={\frac {GMm}{r(t_{2})}}-{\frac {GMm}{r(t_{1})}}.}

This calculation uses the fact that

d d t r i = r ii r ˙ = r ˙ r two . {\displaystyle {\frac {d}{dt}}r^{-1}=-r^{-two}{\dot {r}}=-{\frac {\dot {r}}{r^{two}}}.}

The function

U = Grand M m r , {\displaystyle U=-{\frac {GMm}{r}},}

is the gravitational potential role, besides known as gravitational potential energy. The negative sign follows the convention that piece of work is gained from a loss of potential energy.

Work by a spring [edit]

Forces in springs assembled in parallel

Consider a spring that exerts a horizontal force F = (−kx, 0, 0) that is proportional to its deflection in the x direction independent of how a body moves. The work of this spring on a body moving along the space with the curve X(t) = (x(t), y(t), z(t)), is calculated using its velocity, 5 = (v x, v y, v z), to obtain

W = 0 t F v d t = 0 t k x v x d t = 1 2 one thousand x 2 . {\displaystyle W=\int _{0}^{t}\mathbf {F} \cdot \mathbf {v} dt=-\int _{0}^{t}kxv_{10}dt=-{\frac {1}{two}}kx^{ii}.}

For convenience, consider contact with the jump occurs at t = 0, then the integral of the product of the altitude ten and the ten-velocity, xv x dt, over time t is (1/ii)10 2. The work is the product of the altitude times the bound force, which is also dependent on distance; hence the ten ii issue.

Work past a gas [edit]

Due west = a b P d V {\displaystyle W=\int _{a}^{b}{P}dV}

Where P is force per unit area, Five is book, and a and b are initial and final volumes.

Work–free energy principle [edit]

The principle of work and kinetic energy (also known every bit the work–energy principle) states that the work done by all forces acting on a particle (the work of the resultant force) equals the change in the kinetic free energy of the particle. [17] That is, the work W washed past the resultant force on a particle equals the alter in the particle's kinetic free energy Due east yard {\displaystyle E_{m}} ,[ii]

West = Δ E m = i 2 yard v two two one 2 m v i two {\displaystyle W=\Delta E_{chiliad}={\frac {1}{2}}mv_{two}^{2}-{\frac {one}{2}}mv_{1}^{2}}

where v ane {\displaystyle v_{1}} and v 2 {\displaystyle v_{2}} are the speeds of the particle before and after the work is washed, and m is its mass.

The derivation of the work–energy principle begins with Newton'southward second police force of motion and the resultant force on a particle. Computation of the scalar product of the forces with the velocity of the particle evaluates the instantaneous ability added to the organisation.[18]

Constraints define the management of movement of the particle by ensuring there is no component of velocity in the direction of the constraint force. This also means the constraint forces exercise not add to the instantaneous power. The time integral of this scalar equation yields piece of work from the instantaneous power, and kinetic energy from the scalar product of velocity and acceleration. The fact that the work–free energy principle eliminates the constraint forces underlies Lagrangian mechanics.[xix]

This section focuses on the work–free energy principle as it applies to particle dynamics. In more than general systems work tin can modify the potential free energy of a mechanical device, the thermal energy in a thermal system, or the electrical free energy in an electric device. Work transfers energy from one place to another or one form to another.

Derivation for a particle moving along a direct line [edit]

In the case the resultant forcefulness F is constant in both magnitude and direction, and parallel to the velocity of the particle, the particle is moving with abiding acceleration a along a straight line.[twenty] The relation between the net strength and the acceleration is given by the equation F = ma (Newton's second law), and the particle displacement s can be expressed by the equation

s = v 2 two five 1 ii 2 a {\displaystyle southward={\frac {v_{ii}^{2}-v_{1}^{two}}{2a}}}

which follows from five ii 2 = v 1 2 + 2 a south {\displaystyle v_{two}^{two}=v_{1}^{two}+2as} (come across Equations of motion).

The work of the net strength is calculated every bit the product of its magnitude and the particle displacement. Substituting the above equations, one obtains:

W = F southward = one thousand a due south = g a v 2 2 v i two ii a = g v 2 ii 2 k v ane two ii = Δ East k {\displaystyle West=Fs=mas=ma{\frac {v_{2}^{2}-v_{1}^{ii}}{2a}}={\frac {mv_{two}^{2}}{two}}-{\frac {mv_{ane}^{2}}{2}}=\Delta E_{yard}}

Other derivation:

West = F s = m a s = m v 2 2 v one 2 two s s = 1 2 m 5 ii 2 1 2 thou 5 1 2 = Δ Due east k {\displaystyle W=Fs=mas=m{\frac {v_{2}^{ii}-v_{ane}^{2}}{2s}}due south={\frac {ane}{two}}mv_{two}^{2}-{\frac {1}{2}}mv_{1}^{2}=\Delta E_{k}}

In the general case of rectilinear motility, when the net force F is not abiding in magnitude, simply is abiding in direction, and parallel to the velocity of the particle, the piece of work must exist integrated along the path of the particle:

W = t i t 2 F v d t = t i t 2 F 5 d t = t one t 2 m a five d t = m t 1 t 2 v d 5 d t d t = g 5 one 5 2 v d v = 1 2 m ( 5 2 2 five 1 2 ) . {\displaystyle W=\int _{t_{i}}^{t_{2}}\mathbf {F} \cdot \mathbf {v} dt=\int _{t_{1}}^{t_{two}}F\,five\,dt=\int _{t_{1}}^{t_{ii}}ma\,v\,dt=m\int _{t_{one}}^{t_{2}}v\,{\frac {dv}{dt}}\,dt=m\int _{v_{1}}^{v_{2}}v\,dv={\tfrac {1}{ii}}thousand\left(v_{two}^{2}-v_{one}^{2}\right).}

General derivation of the work–energy theorem for a particle [edit]

For whatsoever net forcefulness acting on a particle moving forth whatever curvilinear path, it tin can exist demonstrated that its work equals the modify in the kinetic energy of the particle by a uncomplicated derivation analogous to the equation to a higher place. Some authors call this issue work–energy principle, simply it is more widely known every bit the piece of work–energy theorem:

Due west = t 1 t 2 F five d t = m t i t 2 a v d t = thousand 2 t i t 2 d 5 2 d t d t = chiliad two v 1 ii 5 2 2 d v 2 = m v two two two thousand 5 ane 2 2 = Δ East yard {\displaystyle Westward=\int _{t_{1}}^{t_{2}}\mathbf {F} \cdot \mathbf {five} dt=m\int _{t_{i}}^{t_{ii}}\mathbf {a} \cdot \mathbf {v} dt={\frac {thousand}{ii}}\int _{t_{ane}}^{t_{2}}{\frac {dv^{2}}{dt}}\,dt={\frac {m}{2}}\int _{v_{1}^{2}}^{v_{2}^{2}}dv^{2}={\frac {mv_{2}^{2}}{ii}}-{\frac {mv_{one}^{2}}{2}}=\Delta {E_{one thousand}}}

The identity a five = i 2 d 5 2 d t {\textstyle \mathbf {a} \cdot \mathbf {v} ={\frac {1}{2}}{\frac {dv^{2}}{dt}}} requires some algebra. From the identity v two = v v {\textstyle v^{2}=\mathbf {v} \cdot \mathbf {v} } and definition a = d v d t {\textstyle \mathbf {a} ={\frac {d\mathbf {5} }{dt}}} it follows

d five 2 d t = d ( v five ) d t = d v d t v + 5 d v d t = 2 d 5 d t 5 = 2 a v . {\displaystyle {\frac {dv^{2}}{dt}}={\frac {d(\mathbf {v} \cdot \mathbf {v} )}{dt}}={\frac {d\mathbf {v} }{dt}}\cdot \mathbf {v} +\mathbf {v} \cdot {\frac {d\mathbf {v} }{dt}}=2{\frac {d\mathbf {v} }{dt}}\cdot \mathbf {v} =two\mathbf {a} \cdot \mathbf {5} .}

The remaining part of the higher up derivation is simply simple calculus, same as in the preceding rectilinear case.

Derivation for a particle in constrained movement [edit]

In particle dynamics, a formula equating work applied to a organization to its change in kinetic energy is obtained every bit a offset integral of Newton's second law of motion. It is useful to notice that the resultant force used in Newton's laws can exist separated into forces that are applied to the particle and forces imposed by constraints on the motion of the particle. Remarkably, the work of a constraint force is zero, therefore simply the work of the applied forces need be considered in the work–energy principle.

To see this, consider a particle P that follows the trajectory 10(t) with a force F acting on information technology. Isolate the particle from its environment to expose constraint forces R, then Newton's Law takes the class

F + R = m X ¨ , {\displaystyle \mathbf {F} +\mathbf {R} =g{\ddot {\mathbf {X} }},}

where m is the mass of the particle.

Vector formulation [edit]

Annotation that n dots in a higher place a vector indicates its nth fourth dimension derivative. The scalar production of each side of Newton'south law with the velocity vector yields

F X ˙ = yard X ¨ X ˙ , {\displaystyle \mathbf {F} \cdot {\dot {\mathbf {10} }}=thousand{\ddot {\mathbf {Ten} }}\cdot {\dot {\mathbf {X} }},}

because the constraint forces are perpendicular to the particle velocity. Integrate this equation along its trajectory from the point 10(t 1) to the point X(t 2) to obtain

t 1 t 2 F Ten ˙ d t = m t one t 2 Ten ¨ X ˙ d t . {\displaystyle \int _{t_{ane}}^{t_{2}}\mathbf {F} \cdot {\dot {\mathbf {X} }}dt=chiliad\int _{t_{i}}^{t_{2}}{\ddot {\mathbf {X} }}\cdot {\dot {\mathbf {X} }}dt.}

The left side of this equation is the piece of work of the applied force as it acts on the particle along the trajectory from fourth dimension t ane to time t 2. This can also be written as

W = t one t 2 F Ten ˙ d t = Ten ( t 1 ) X ( t 2 ) F d X . {\displaystyle W=\int _{t_{1}}^{t_{two}}\mathbf {F} \cdot {\dot {\mathbf {X} }}dt=\int _{\mathbf {10} (t_{1})}^{\mathbf {X} (t_{2})}\mathbf {F} \cdot d\mathbf {Ten} .}

This integral is computed along the trajectory X(t) of the particle and is therefore path dependent.

The right side of the first integral of Newton's equations can exist simplified using the following identity

1 two d d t ( X ˙ Ten ˙ ) = X ¨ X ˙ , {\displaystyle {\frac {1}{ii}}{\frac {d}{dt}}({\dot {\mathbf {X} }}\cdot {\dot {\mathbf {X} }})={\ddot {\mathbf {10} }}\cdot {\dot {\mathbf {10} }},}

(see product rule for derivation). Now it is integrated explicitly to obtain the alter in kinetic energy,

Δ K = k t 1 t 2 X ¨ X ˙ d t = chiliad 2 t 1 t 2 d d t ( X ˙ X ˙ ) d t = one thousand ii X ˙ Ten ˙ ( t 2 ) grand 2 Ten ˙ X ˙ ( t i ) = 1 ii m Δ v ii , {\displaystyle \Delta Thou=m\int _{t_{i}}^{t_{2}}{\ddot {\mathbf {10} }}\cdot {\dot {\mathbf {X} }}dt={\frac {m}{2}}\int _{t_{1}}^{t_{two}}{\frac {d}{dt}}({\dot {\mathbf {X} }}\cdot {\dot {\mathbf {10} }})dt={\frac {1000}{2}}{\dot {\mathbf {10} }}\cdot {\dot {\mathbf {X} }}(t_{2})-{\frac {m}{two}}{\dot {\mathbf {10} }}\cdot {\dot {\mathbf {X} }}(t_{ane})={\frac {1}{2}}m\Delta \mathbf {v} ^{two},}

where the kinetic free energy of the particle is divers by the scalar quantity,

K = yard 2 10 ˙ X ˙ = 1 2 yard five 2 {\displaystyle K={\frac {1000}{two}}{\dot {\mathbf {X} }}\cdot {\dot {\mathbf {X} }}={\frac {1}{2}}m{\mathbf {v} ^{2}}}

Tangential and normal components [edit]

It is useful to resolve the velocity and acceleration vectors into tangential and normal components along the trajectory X(t), such that

X ˙ = v T and X ¨ = v ˙ T + v 2 κ Northward , {\displaystyle {\dot {\mathbf {X} }}=v\mathbf {T} \quad {\mbox{and}}\quad {\ddot {\mathbf {Ten} }}={\dot {v}}\mathbf {T} +v^{ii}\kappa \mathbf {Northward} ,}

where

v = | X ˙ | = 10 ˙ X ˙ . {\displaystyle 5=|{\dot {\mathbf {X} }}|={\sqrt {{\dot {\mathbf {X} }}\cdot {\dot {\mathbf {X} }}}}.}

Then, the scalar product of velocity with dispatch in Newton'southward second law takes the form

Δ Thou = m t 1 t 2 5 ˙ v d t = m 2 t 1 t ii d d t v ii d t = m 2 v ii ( t 2 ) m ii v 2 ( t 1 ) , {\displaystyle \Delta M=k\int _{t_{1}}^{t_{2}}{\dot {v}}5\,dt={\frac {chiliad}{2}}\int _{t_{ane}}^{t_{two}}{\frac {d}{dt}}five^{ii}\,dt={\frac {m}{ii}}v^{2}(t_{2})-{\frac {m}{two}}five^{2}(t_{1}),}

where the kinetic energy of the particle is defined by the scalar quantity,

One thousand = m 2 v two = m ii X ˙ X ˙ . {\displaystyle Grand={\frac {chiliad}{ii}}5^{2}={\frac {thousand}{2}}{\dot {\mathbf {X} }}\cdot {\dot {\mathbf {X} }}.}

The result is the work–free energy principle for particle dynamics,

West = Δ Thousand . {\displaystyle Westward=\Delta Chiliad.}

This derivation can be generalized to arbitrary rigid trunk systems.

Moving in a straight line (skid to a stop) [edit]

Consider the instance of a vehicle moving along a direct horizontal trajectory under the action of a driving force and gravity that sum to F. The constraint forces between the vehicle and the road define R, and nosotros accept

F + R = yard Ten ¨ . {\displaystyle \mathbf {F} +\mathbf {R} =m{\ddot {\mathbf {X} }}.}

For convenience let the trajectory exist along the X-axis, then X = (d, 0) and the velocity is 5 = (5, 0), then RV = 0, and F5 = F x v , where F x is the component of F along the X-axis, so

F 10 v = m v ˙ v . {\displaystyle F_{10}5=m{\dot {five}}five.}

Integration of both sides yields

t i t ii F x 5 d t = m two v 2 ( t 2 ) m 2 v 2 ( t i ) . {\displaystyle \int _{t_{one}}^{t_{2}}F_{x}vdt={\frac {m}{two}}five^{ii}(t_{2})-{\frac {k}{two}}v^{2}(t_{one}).}

If F x is constant forth the trajectory, so the integral of velocity is distance, so

F 10 ( d ( t ii ) d ( t 1 ) ) = m 2 v ii ( t 2 ) m 2 5 2 ( t ane ) . {\displaystyle F_{x}(d(t_{2})-d(t_{1}))={\frac {grand}{ii}}v^{2}(t_{2})-{\frac {m}{2}}v^{2}(t_{1}).}

As an case consider a car skidding to a stop, where k is the coefficient of friction and W is the weight of the car. Then the force along the trajectory is F x = −kW . The velocity v of the motorcar can be determined from the length s of the skid using the work–energy principle,

grand W s = W 2 g v 2 , or v = ii 1000 s m . {\displaystyle kWs={\frac {W}{2g}}v^{two},\quad {\mbox{or}}\quad 5={\sqrt {2ksg}}.}

Discover that this formula uses the fact that the mass of the vehicle is thousand = W/g .

Lotus type 119B gravity racer at Lotus 60th celebration.

Gravity racing championship in Campos Novos, Santa Catarina, Brazil, 8 September 2010.

Benumbed downwardly a mount road (gravity racing) [edit]

Consider the case of a vehicle that starts at residual and coasts down a mountain route, the work–energy principle helps compute the minimum distance that the vehicle travels to reach a velocity V, of say threescore mph (88 fps). Rolling resistance and air drag will slow the vehicle downwardly and so the actual altitude will be greater than if these forces are neglected.

Let the trajectory of the vehicle following the road be X(t) which is a bend in three-dimensional space. The strength acting on the vehicle that pushes it downwards the route is the constant force of gravity F = (0, 0, Westward), while the force of the route on the vehicle is the constraint force R. Newton'southward second law yields,

F + R = yard X ¨ . {\displaystyle \mathbf {F} +\mathbf {R} =1000{\ddot {\mathbf {X} }}.}

The scalar product of this equation with the velocity, Five = (five x, five y, 5 z), yields

Westward v z = grand V ˙ V , {\displaystyle Wv_{z}=yard{\dot {Five}}V,}

where V is the magnitude of V. The constraint forces betwixt the vehicle and the road cancel from this equation because RV = 0, which means they do no work. Integrate both sides to obtain

t 1 t 2 West 5 z d t = m 2 V 2 ( t ii ) one thousand 2 V 2 ( t 1 ) . {\displaystyle \int _{t_{1}}^{t_{2}}Wv_{z}dt={\frac {yard}{2}}V^{2}(t_{2})-{\frac {m}{2}}Five^{ii}(t_{1}).}

The weight strength West is abiding along the trajectory and the integral of the vertical velocity is the vertical distance, therefore,

Due west Δ z = m ii V 2 . {\displaystyle W\Delta z={\frac {m}{2}}V^{2}.}

Remember that Five(t 1)=0. Notice that this event does not depend on the shape of the road followed by the vehicle.

In order to decide the distance along the road assume the downgrade is 6%, which is a steep road. This means the altitude decreases half-dozen feet for every 100 feet traveled—for angles this small the sin and tan functions are approximately equal. Therefore, the distance s in feet down a half dozen% grade to reach the velocity V is at least

s = Δ z 0.06 = 8.three Five two g , or southward = 8.iii 88 2 32.2 2000 ft . {\displaystyle s={\frac {\Delta z}{0.06}}=8.3{\frac {V^{2}}{g}},\quad {\mbox{or}}\quad south=viii.3{\frac {88^{2}}{32.2}}\approx 2000{\mbox{ft}}.}

This formula uses the fact that the weight of the vehicle is Westward = mg .

Work of forces acting on a rigid body [edit]

The piece of work of forces acting at diverse points on a unmarried rigid body can be calculated from the work of a resultant force and torque. To see this, permit the forces F 1, F 2 ... F n act on the points Ten 1, X 2 ... 10 north in a rigid body.

The trajectories of X i , i = 1, ..., north are defined by the movement of the rigid body. This motility is given by the set of rotations [A(t)] and the trajectory d(t) of a reference point in the trunk. Let the coordinates 10 i i = one, ..., n define these points in the moving rigid body'due south reference frame M, so that the trajectories traced in the fixed frame F are given by

X i ( t ) = [ A ( t ) ] 10 i + d ( t ) i = i , , northward . {\displaystyle \mathbf {10} _{i}(t)=[A(t)]\mathbf {x} _{i}+\mathbf {d} (t)\quad i=1,\ldots ,n.}

The velocity of the points X i along their trajectories are

V i = ω × ( X i d ) + d ˙ , {\displaystyle \mathbf {V} _{i}={\vec {\omega }}\times (\mathbf {Ten} _{i}-\mathbf {d} )+{\dot {\mathbf {d} }},}

where ω is the angular velocity vector obtained from the skew symmetric matrix

[ Ω ] = A ˙ A T , {\displaystyle [\Omega ]={\dot {A}}A^{\mathrm {T} },}

known as the angular velocity matrix.

The small corporeality of work by the forces over the small displacements δ r i can exist determined past approximating the displacement past δ r = v δt then

δ Due west = F 1 V 1 δ t + F two Five 2 δ t + + F n V n δ t {\displaystyle \delta Due west=\mathbf {F} _{1}\cdot \mathbf {V} _{1}\delta t+\mathbf {F} _{2}\cdot \mathbf {V} _{two}\delta t+\ldots +\mathbf {F} _{n}\cdot \mathbf {V} _{north}\delta t}

or

δ W = i = one n F i ( ω × ( X i d ) + d ˙ ) δ t . {\displaystyle \delta W=\sum _{i=1}^{due north}\mathbf {F} _{i}\cdot ({\vec {\omega }}\times (\mathbf {10} _{i}-\mathbf {d} )+{\dot {\mathbf {d} }})\delta t.}

This formula can be rewritten to obtain

δ W = ( i = one n F i ) d ˙ δ t + ( i = one n ( X i d ) × F i ) ω δ t = ( F d ˙ + T ω ) δ t , {\displaystyle \delta Westward=\left(\sum _{i=one}^{n}\mathbf {F} _{i}\right)\cdot {\dot {\mathbf {d} }}\delta t+\left(\sum _{i=1}^{n}\left(\mathbf {X} _{i}-\mathbf {d} \right)\times \mathbf {F} _{i}\right)\cdot {\vec {\omega }}\delta t=\left(\mathbf {F} \cdot {\dot {\mathbf {d} }}+\mathbf {T} \cdot {\vec {\omega }}\correct)\delta t,}

where F and T are the resultant force and torque applied at the reference point d of the moving frame One thousand in the rigid trunk.

References [edit]

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Bibliography [edit]

  • Serway, Raymond A.; Jewett, John W. (2004). Physics for Scientists and Engineers (6th ed.). Brooks/Cole. ISBN0-534-40842-7.
  • Tipler, Paul (1991). Physics for Scientists and Engineers: Mechanics (3rd ed., extended version ed.). W. H. Freeman. ISBN0-87901-432-vi.

External links [edit]

  • Work–energy principle

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