Chapter 4-6 Flashcards

1
Q

Conservative Force

A

any force (f) for which a potential energy function (V) can be defined such that: F(x) = -dV/dx

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2
Q

Work (W) Done By a Conservative Force

A

W = integral from x sub 0 to x of F dot dx = - delta V

  1. W is independent of the path taken (only depends on the initial and final positions)
  2. W = 0 for a closed path
  3. If F violates W = 0, then it violates W = -delta V (W depends on the path taken!) and F is called a “nonconservative” force and V cannot be defined (ex: friction)
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3
Q

Test for a Conservative Force

A

The curl of F (del cross F) = 0

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4
Q

Del Operator

A

Del = ihat (d/dx) + jhat(d/dy) + khat(d/dz)

where d is a partial derivative

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5
Q

Gradient of a Scalar

A

Del V = dV/dx ihat + dV/dy jhat + dV/dz khat

(where d is a partial derivative)

produces a vector

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6
Q

Divergence of a Vector

A

Del dot F = d(F sub x)/dx + d(F sub y)/dy + d(F sub z)/dz

(where d is a partial derivative)

produces a scalar

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7
Q

Curl of a Vector

A

(on equation sheet)

produces a vector

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8
Q

Conservation of Energy (E)

A

The total energy of an isolated system must remain constant

  1. If only conservative forces are present: Ta + Va = Tb + Vb (where T + V = E = Total energy)
  2. If both conservative forces and nonconservative forces are present: Ta + Va + integral from a to b of Fnc dot dr = Tb + Vb (work done by c forces are included in V with Fc = -dV/dx and work done by nc forces must be calculated directly since V doesn’t exist for them with Fnc != -dV/dx)
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9
Q

Separable Force

A

a force where each component only contains that particular coordinate (ex: x-comp only contains “x”)

F = Fx(x) ihat + Fy(y) jhat + Fz(z) khat

all separable forces are conservative

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10
Q

Steps to solving Projectile Motion in 3D

A

trajectory: (g/2v0^2cos^2(alpha))x^2 -(tan(alpha))x + z = 0

zmax = v0^2sin^2(alpha)/2g

range = v0^2sin(2alpha)/g

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11
Q

Isotropic Harmonic Oscillator

A

restoring force is the same in all directions

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12
Q

Nonisotropic Harmonic Oscillator

A

restoring force is not the same in all directions

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13
Q

Constrained Motion of a Particle

A

motion in which a particle is constrained to move along a definite surface or curve

F + R = ma

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14
Q

Reference Frame

A

a coordinate system used to describe an object’s position and motion

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15
Q

Inertial Reference Frame

A

reference frame in which Newton’s 1st Law is obeyed (If the net force on an object is zero, then a = 0)

any reference frame that moves at a constant velocity with respect to an inertial reference frame is also an inertial reference frame

laws of physics look the same in all inertial reference frames

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16
Q

Noninertial Reference Frame

A

reference frames in which Newton’s 1st Law is not obeyed (object accelerates with Fnet = 0)

all accelerating reference frames are noninertial reference frames

laws of physics do not look the same in all inertial reference frames

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17
Q

Inertial Forces

A

“fictitious forces” that are not due to interactions with real objects. They are always present when motion is described from a noninertial reference frame (to force the laws of physics to have the same mathematical form)

18
Q

Transverse Force

A

created when O’ has an angular acceleration

directed perpendicular to r

Ftrans = -m(omega_dot cross r)

19
Q

Coriolis Force

A

created when particle moves in O’ (unless v’ is ll to omega)

directed perpendicular to v and omega

Fcor = -2m(omega cross v)

20
Q

Centrifugal Force

A

created when r is not ll to omega (otherwise omega cross r = 0)

directed outward from rotational axis

Fcent = -m omega cross (omega cross r)

21
Q

Centripetal Acceleration

A

inward acceleration that an object experiences when it moves in a circle of radius r at a constant speed v

a = v^2/r

22
Q

Centripetal Force

A

Real inward force that keeps an object moving in a circle of radius r at constant speed v

F = mv^2/r

23
Q

The Foucault Pendulum

A

a spherical pendulum free to swing in any direction that is affected by the Earth’s rotation

24
Q

Kepler’s 1st law

A

the orbit of each planet is an ellipse with sun at a focus point

25
Q

Kepler’s 2nd Law

A

a line drawn between sun and planet sweeps equal areas in equal times

26
Q

Kepler’s 3rd Law

A

the square of a planet’s sidereal period (tal) is directly proportional to the cube of semimajor axis (a) of orbit

tal^2 = ka^3

27
Q

Sidereal Period

A

(tal) time for a planet to orbit once about the sun relative to stars

28
Q

Newton’s Law of Universal Gravitation

A

every object in the universe attracts ever other object with a force that is directly proportional to the product of their masses, inversely proportional to the square of the distance between them, and points along the line connecting them

29
Q

Point Mass

A

an object whose mass is concentrated at a single point in space and has no volume

30
Q

Central Force

A

a force that is directed toward or away from a single point and magnitude only depends on the distance from this point

F = f(r) rhat

31
Q

Angular Momentum

A

(L) cross product of a particle;s position vector (r) and linear momentum (p)

L = r cross p

32
Q

Torque

A

(Tal) any influence that can cause an object to rotate (accelerate angularly)

Tal = r cross F

33
Q

Conservation of Angular Momentum

A

if tal external = 0 then dL/dt = 0 and L is constant

  1. L is constant for all central forces
  2. if a particle has L = constant, it is confined to the plane formed by r cross p
34
Q

Area of a Parallelogram

A

Area = absolute value of c cross d

35
Q

Ellipse

A

set of all points whose total distance from 2 foci (f and f’ is constant)

36
Q

Pericenter of an Orbit

A

distance at which objects are closest together

rmin = a(1-epsilon) or rmin = alpha/1+epsilon

perihelion for solar orbits and perigee for earth orbits

37
Q

Apocenter of an Orbit

A

distance at which objects are farthest apart

rmax = alpha/1-epsilon or rmax = a(1+epsilon)

aphelion for solar orbits and apogee for earth orbits

38
Q

Conic Section

A

figure formed by the intersection of plane and cone

  1. Circle epsilon = 0
  2. Ellipse 0 1
39
Q

Escape Velocity

A

the value of v that makes rmax = infinity

40
Q

Rutherford Scattering

A

describes the motion of a particle that experience an inverse square repulsive electrical force

41
Q

Impact Parameter

A

(b) perpendicular distance from the origin (scattering center = nucleus) to the initial line of motion of the projectile (alpha particle)

42
Q

Solid Angle

A

2D angle in 3D space that an object subtends at a point (dimensionless unit = steradians)