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Very good review cheat sheet for your Physics exam with formulas
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d t t
v t
a
d t t
v t
a
A
B
R A B
R
The Best Dang Regents Physics Review Sheet Ever!
Math, Graphs, and Vectors:
Kinematics (Study of Motion):
Forces, mass, Newton’s Laws and Gravity:
Uniform Circular Motion, Momentum, Impulse, Friction:
3 A 2 A
1 or 5 A
(before) q 1 + q 2 + … = q 1 ' + q 2 ' + … (after) Signs matter!
Current and Circuits:
Magnetism and Electromagnetism (E&M):
Vibrations and Waves:
m
F 1
F 2
R
- R = equilibrant
Fnet = w
ax= ay =
fired with a certain vi
fired with a speed 2vi
slope = c^2
900
R =diagonal
1800
R = difference = minimum
vtop ≠ 0
00
R = sum = maximum
w
wperp = wcos
wll = wsin
reactant 1 + reactant 2 + …. product 1 + product 2 + … + ENERGY Add up reactants, add up products, then subtract represents energy released (aka “mass defect”)
Diagrams:
dropped ball
CW
v
F, a
v
v
F, a
F, a
F, a (^) CCW
F, a
v
v
F, a (^) F, a v
v
F, a
ET = PE + KE = constant Loss of KE gain of PE Loss of PE gain of KE
PE KE
b/ by induction:
positive charge:
negatively charged object:
a/ by contact:
neutral conductor Touching^ –^ equal q on each. (If 1 sphere bigger more q)
separate
neutral conductor: charges separate ground
Remove ground, then remove the charged object. Note: charges now opposite original charged object.
charged object
charged conductor
g ~ 1/r^2 for a point mass: Earth w
Fg (weight) or g as a function of distance from Earth:
1Re 2Re
1Re 2Re 3Re 4Re
3Re 4 Re
5Re from center
w 4
w 9
w 16
w 25
from surface
9. Conservation of Energy for a freely falling object or a pendulum with no friction: 5. Forces:
Fx = Fcos
Fy = Fsin
F
d F W = Fd
6. Work:
Fnet = 0 a = 0 at rest OR const. v
d
W = Fxd = Fcos d
F
Fnet ≠ 0 a to right vel. can be pos. or neg.
F
w = FN w = T
slightly curved at edges
FN
d
F W = 0 d^ b/c^ = 90^0
F W = Fd
At rest:
g = 9.81 m/s^2 is constant at Earth’s surface:
7. Gravitational **fields g:
string
w + F
Before:
e-^ at rest
photon at v = c
e-^ now has KE
Eph is less, so longer, but v still = c
around an obstacle:
around a corner:
Bigger or smaller d: More diffraction
22. Refraction of Light:
wavefronts:
incident waves with v 1 , f 1 , A 1 (reflected wave not shown)
transmitted waves with v 2 , f 2 , A 2
faster
slower
smaller n
bigger n
If rays 1 and 2 are parallel, then n 1 = n 2 (same v)
slowest
1
2
1
2
fastest
fastest
slowest
same same
fastest
Bigger angle, faster v, and vice versa. Same angle, same v:
wave- fronts:
rays:
Through an opening:
Images in a flat mirror m: Same size Same distance
i =^ r
always same as on other side of barrier
m
d
boundary
v 1 v 2
n 1 n 2
meson: s u
hadrons & leptons (which occur by themselves)
baryon:
u d u
Some of photon E and momentum are transferred to e-. ET and pT are conserved e-^ gains what photon loses
uud = (+2/3)e + (+2/3)e + (-1/3)e = +1e (a proton)
24. Standard model: All matter is made of…
su = (- 1 /3)e + (- 2 /3)e = - 1e
The antiparticles are: uud = - 1e and su = +1e They have the same mass as their antimatter.
i (^) r
o (^) i
specular:
diffuse:
**19. Diffraction:
Compare: v 1 > v 2 (given), n 2 > n 1 , A 1 > A 2 (some reflected), 1 > 2 , but f 1 = f 2 (same frequency!)
23. Photon-electron collisions (Compton Effect) Light acting like a particle:
After:
Smaller or bigger d: Less diffraction