Term
Resistance of a resistor = |
|
Definition
Resistance = pL/A
Resistance is given by the equation R=pL/A, where p is resistivity, L is the length of the resistor, and A is the cross-sectional area of the resistor. |
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
Gravitational Force between two objects
|
|
Definition
[image] where:
- F is the force between the masses;
- G is the gravitational constant (6.674×10−11 N · (m/kg)2);
- m1 is the first mass;
- m2 is the second mass;
- r is the distance between the centers of the masses.
|
|
|
Term
|
Definition
First law: When viewed in an inertial reference frame, an object either remains at rest or continues to move at a constant velocity, unless acted upon by a force. Fnet = ma = 0
Second law: The vector sum of the forces F on an object is equal to the mass m of that object multiplied by the acceleration vector a of the object: Fnet = ma.
Third law:When one body exerts a force on a second body, the second body simultaneously exerts a force equal in magnitude and opposite in direction on the first body.
|
|
|
Term
Velcocity at time t when given initial velocity, aceleration and time |
|
Definition
|
|
Term
Displacement when given initial velocity, aceleration, and time |
|
Definition
displacement: d = v0t + (at2)/2 |
|
|
Term
Velocity when given intial velocity, aceleration, and position |
|
Definition
|
|
Term
Components of gravity on an inclined plane |
|
Definition
|
|
Term
|
Definition
The magnitude of the centripetal force on an object of mass m moving at tangential speed v along a path with radius of curvature r is:
- [image]
where [image] is the centripetal acceleration. |
|
|
Term
|
Definition
- [image] [image]
where
- [image] is the torque vector and [image] is the magnitude of the torque,
- r is the position vector (a vector from the origin of the coordinate system defined to the point where the force is applied)
- F is the force vector,
- × denotes the cross product,
- θ is the angle between the force vector and the lever arm vector.
|
|
|
Term
|
Definition
|
|
Term
Gravitational potential energy |
|
Definition
U = mgh
mass
gravitational constant
height |
|
|
Term
|
Definition
[image]
k = spring constant
Δx = magnitude of displacement from equilibrium |
|
|
Term
|
Definition
E = U + K
Total = potential + kinetic |
|
|
Term
Conservation of mechaincal energy
VS
Nonconservative work formula |
|
Definition
ΔE = ΔU + ΔK = 0
Wnonconservative = ΔE = ΔU + ΔK |
|
|
Term
|
Definition
W = F • d = Fdcos(θ)
W = Work
F = magnitude of the applied force
d = magnitude of the displacement through the force applied
θ = the angle between the applied force vector and the displacement vector |
|
|
Term
|
Definition
W = PΔV
Find the area under the curve with P on Y axis and V on the X.
Volume constant then no work.
Gas expands, W is positive
Gas compresses, W is negative |
|
|
Term
|
Definition
P = W/t = ΔE/t
Power equals work over time or the change in energy over time
Unit = J/sec |
|
|
Term
|
Definition
|
|
Term
|
Definition
If a and b are distances from the fulcrum to points A and B and if force FA applied to A is the input force and FB exerted at B is the output, the ratio of the velocities of points A and B is given by a/b, so the ratio of the output force to the input force, or mechanical advantage, is given by
- [image]
Because the power flow is constant, the torque TB and angular velocity ωB of the output gear must satisfy the relation
- [image]
which yields
- [image]
|
|
|
Term
|
Definition
Efficiency = W Out/ W In
=(load)(load distance)/(effort*effort distance) |
|
|
Term
|
Definition
|
|
Term
|
Definition
The change in the linear dimension can be estimated to be:
- [image]
This equation works well as long as the linear-expansion coefficient does not change much over the change in temperature [image], and the fractional change in length is small [image]. If either of these conditions does not hold, the equation must be integrated |
|
|
Term
|
Definition
If we already know the expansion coefficient, then we can calculate the change in volume
- [image]
where [image] is the fractional change in volume (e.g., 0.002) and [image] is the change in temperature (50 °C). |
|
|
Term
1st law of thermodynamics |
|
Definition
In a non-cyclic process, the change in the internal energy of a system is equal to net energy added as heat to the system minus thenet work done by the system, both being measured in mechanical units. Taking ΔU as a change in internal energy, one writes
- [image]
where Q denotes the net quantity of heat supplied to the system by its surroundings and W denotes the net work done by the system. This sign convention is implicit in Clausius' statement of the law given above. It originated with the study of heat engines that produce useful work by consumption of heat |
|
|
Term
Heat gained or lost with temp change |
|
Definition
|
|
Term
Heat gained or lost in phase change |
|
Definition
|
|
Term
|
Definition
ΔS = Qrev/t
S is change in entrhopy
Q heat change in the process
T = temp |
|
|
Term
|
Definition
Mathematically, density is defined as mass divided by volume:[1]
- [image]
where ρ is the density, m is the mass, and V is the volume. |
|
|
Term
Weight of a volume of fluid |
|
Definition
Fg = density * Volume * gravity constant
For fluids |
|
|
Term
|
Definition
Specific gravity is the ratio of the density of a substance to the density of a reference substance; equivalently, it is the ratio of the mass of a substance to the mass of a reference substance for the same given volume.
It can be shown that true specific gravity can be computed from different properties:
- [image]
|
|
|
Term
|
Definition
|
|
Term
|
Definition
The total pressure that is exerted on an object that is submerged in a fluid
Pressure = surface pressure + density*gravity acceleration*depth
P = P0 +ρgz |
|
|
Term
|
Definition
Pgauge = P-Patm = (p0+ρgz)-patm
ρ = density
g = acceleration due to gravity
z=depth |
|
|
Term
|
Definition
Seen in pistons
P = F1/A1 = F2/A2
F2=F1(A2/A1) |
|
|
Term
Archimedes Principle
Buoyancy |
|
Definition
Fbuoy = ρfluid*Vfluid displace*g
= ρfluid*Vsubmerged*g |
|
|
Term
Poiseuille equation
Flow through a pipe |
|
Definition
[image]
where:
- [image] is the pressure loss
- [image] is the length of pipe
- [image] is the dynamic viscosity
- [image] is the volumetric flow rate
- [image] is the radius
- [image] is the velocity
|
|
|
Term
|
Definition
[image]
Nr is a constant
η = viscosity
density
diameter |
|
|
Term
|
Definition
Q = Flow rate = v1A1 = v2A2 |
|
|
Term
|
Definition
|
|
Term
|
Definition
In its scalar form the law is:
- [image] ,
where ke is Coulomb's constant (ke = 8.99×109 N m2 C−2), q1 and q2are the signed magnitudes of the charges, the scalar r is the distance between the charges. |
|
|
Term
|
Definition
|
|
Term
Electrical Potential Energy |
|
Definition
-
where [image] is Coulomb's constant, r is the distance between the point charges q & Q, and q & Q are the signed values of the charges |
|
|
Term
Electrical Potential
From Potential Energy
vs
From Source Energy |
|
Definition
|
|
Term
|
Definition
|
|
Term
The potential of an electric dipole |
|
Definition
|
|
Term
|
Definition
|
|
Term
Electric field on the perpendicular bisector of a dipole |
|
Definition
|
|
Term
Torque on a dipole in an electric field |
|
Definition
|
|
Term
Magnetic field from a
Straight Wire
vs
Loop of wire |
|
Definition
B = (μ0I)/(2πr)
vs
B = (μ0I)/(2r) |
|
|
Term
Magnetic Force on a...
Moving point charge
vs
Current-carrying wire |
|
Definition
Fb = qvB*sin(θ)
vs
Fb = ILB*sin(θ) |
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|