Preliminary formula Sheet for LSU Physics 2101, Exam 3 ... · PDF filePreliminary formula...
Transcript of Preliminary formula Sheet for LSU Physics 2101, Exam 3 ... · PDF filePreliminary formula...
Preliminary formula Sheet for LSU Physics 2101, Exam 3, Fall ’12
Units:1m = 39.4 in = 3.28 ft 1 mi = 5280 ft 1min = 60 s, 1 day = 24 h 1 rev = 360 = 2π rad
1 atm = 1.013×105 Pa T =(
1K
1C
)TC + 273.15K TF =
(9 F5C
)TC + 32F
Constants:g = 9.8 m/s2 REarth = 6.37× 106 m MEarth = 5.98×1024 kgG = 6.67×10−11 m3/(kg·s2) RMoon = 1.74× 106 m MMoon = 7.36×1022 kgEarth-Sun distance = 1.50×1011 m MSun = 1.99×1030 kg Earth-Moon distance = 3.82×108 m
Quadratic formula: for ax2 + bx + c = 0, x1,2 =−b ± √
b2 − 4ac
2a
Magnitude of a vector: |~a| =√
a2x + a2
y + a2z
Dot Product: ~a ·~b = axbx + ayby + azbz = |~a|∣∣∣~b
∣∣∣ cos(φ) (φ is smaller angle between ~a and ~b)
Cross Product: ~a ×~b = (aybz − azby)ı + (azbx − axbz) + (axby − aybx)k,∣∣∣~a ×~b
∣∣∣ = |~a|∣∣∣~b
∣∣∣ sin(φ)
Equations of Constant Acceleration:
linear equation along x missing missing rotational equationvx = vox + axt x − xo θ − θo ω = ωo + αxt
x − xo = voxt +1
2axt2 vx ω θ − θo = ωot +
1
2αt2
v2x = v2
ox + 2ax(x − xo) t t ω2 = ω2o + 2α(θ − θo)
x − xo =1
2(vox + vx)t ax α θ − θo =
1
2(ωo + ω)t
x − xo = vxt − 1
2axt2 vox ωo θ − θo = ωt − 1
2αt2
Vector Equations of Motion for Constant Acceleration: ~r = ~ro + ~vot +1
2~at2, ~v = ~vo + ~at
Projectile Motion: (with + direction pointing up from Earth)
x − xo = (vo cos θo)t y − yo = (vo sin θo)t − 1
2gt2
vx = vo cos θo vy = (vo sin θo) − gt
y = (tan θo)x − gx2
2(vo cos θo)2v2
y = (vo sin θo)2 − 2g(y − yo)
Newton’s Second Law:∑
~F = m~a
Uniform circular motion: Fc = mac =mv2
r, T =
2 π r
v
Force of Friction: Static: fs ≤ fs,max = µsFN , Kinetic: fk = µkFN
Spring (elastic) Force: Hooke’s Law Fspring = −kx (k = spring (force) constant)
Kinetic Energy: Translational K =1
2mv2
Work: W =∫ xf
xi
F (x)dx (variable 1D force), W =∫ rf
ri
~F (~r) · d~r (variable 3D force),
W = ~F · ~d (constant force)
Work - Kinetic Energy Theorem: W = ∆K = Kf − Ki
Work done by weight (gravity close to the Earth surface): W = m ~g · ~d = −m g ∆y
Work Done by a Spring Force: Ws = −k
(x2
f
2− x2
i
2
)
Power: Average: Pavg =W
∆t, P = ~F · ~vavg (constant force)
Instantaneous: P =dW
dt, P = ~F · ~v (constant force)
Potential Energy Change: ∆U = −W
Gravitational Potential Energy: Ug(y) = mgy
Elastic (Spring) Potential Energy: Us =1
2kx2 (relative to the relaxed spring)
Potential-Force Relation: F (x) = −dU(x)
dxMechanical Energy: Emec = K + U
Change of Mechanical Energy due to Non-Conservative (nc) Forces:
Wnc = ∆Emec = (Kf + Uf) − (Ki + Ui)
Conservation of Energy: Wext = ∆K + ∆U + ∆Eth + ∆Eint, Wext is the net, external work done byexternal forces on the system, ∆Eth = −Wfk is the thermal energy change, ∆Eint is the internal energy change
Center of mass: M =N∑
i=1
mi, xcom =1
M
N∑
i=1
mixi, ycom =1
M
N∑
i=1
miyi, zcom =1
M
N∑
i=1
mizi
~rcom =1
M
N∑
i=1
mi~ri ~vcom =1
M
N∑
i=1
mi~vi ~acom =1
M
N∑
i=1
mi~ai =1
M
N∑
i=1
~Fi
Definition of Linear Momentum: one particle: ~p = m~v, system of particles: ~P =N∑
i=1
~pi = M~vcom
Newton’s 2nd Law for a System of Particles: ~Fnet = M~acom =d ~P
dt
Conservation of Linear Momentum of an Isolated System:∑
~pi =∑
~pf
Impulse - Linear Momentum Theorem: ∆~p1 = ~J12 =∫ t2
t1
~F12(t)dt = ~Favg,12∆t
Elastic Collision (1 Dim): v1f =m1 − m2
m1 + m2v1i +
2m2
m1 + m2v2i v2f =
2m1
m1 + m2v1i +
m2 − m1
m1 + m2v2i
Linear and Angular Variables Related:
s = rθ v = ωr at = αr ar =v2
r= ω2r (magnitude of the radial or centripetal acceleration)
Rotation: Rotational Inertia (Icom) for Simple Shapes: see next page
Rotational Inertia: Descrete particles: I =N∑
i=1
Ii Continuous object: I =∫
r2dm
Parallel Axis Theorem: I = Icom + Mh2
Torque: ~τ = ~r × ~F τ = rFt = r⊥F = rF sin φ
Angular Momentum: rigid body, fixed axis: ~L = I~ω point-like particle: ~L = ~r × ~p
Newton’s 2nd Law: ~τnet = I~α ~τnet =d~L
dtConservation Law (isolated system,
∑τ = 0):
∑ ~Li =∑ ~Lf
Rotational Work: W =∫ θf
θi
τdθ = τavg∆θ Kinetic Energy: K =1
2Iω2
Rotational Power: Instantaneous: P =dW
dt= τω Average: Pavg =
W
t= τavgωavg
Rolling: vcom = ωR acom = αR
Kinetic Energy of Rolling: K =1
2mv2
com +1
2Icomω2
Static equilibrium: ~Fnet = 0 ~τnet = 0
Gravity:
Newton’s law: |~F | = Gm1m2
r2Gravitational acceleration (planet of mass M): ag =
GM
r2
Law of periods: T 2 =
(4π2
GM
)r3 Potential Energy: U = −G
m1m2
r
Potential Energy of a System (more than 2 masses): U = −(
Gm1m2
r12+ G
m1m3
r13+ G
m2m3
r23+ ...
)
Static Fluids:
Density: ρ =∆m
∆VPressure: p =
∆F
∆AAbsolute Pressure: p = po + ρgh
Pressure Variation with Height or Depth: p2 = p1 + ρ g (y1 − y2) Gauge pressure: p − po
Archimedes’ Principle: Fb = ρfVdisplacedg = mfg weightapparent= mg − Fb
Simple Harmonic Motion (SHM): T =1
f=
2π
ωLinear: x(t) = xm cos(ωt + φ) Angular: Θ(t) = Θm cos(ωt + φ)
v(t) = −xmω sin(ωt + φ) Ω(t) = −Θmω sin(ωt + φ)a(t) = −xmω2 cos(ωt + φ) = −ω2x(t) α(t) = −Θmω2 cos(ωt + φ) = −ω2Θ(t)
Linear Oscillator: Spring-Block: ω =
√k
mHorizontal Spring-Block: Emec =
1
2kx2
m
Pendulums: Torsion: ω =√
κ
ISimple: ω =
√g
LPhysical: ω =
√mgh
ITorsion torque: τ = −κΘ