Visual Physics Online - School of Physics · VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are...

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1 VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are essential part of physics, without them, we can’t start to explain our physical world and make predictions. An equation tells a story – a collection of a few symbols contains a wealth of information. Many examination questions can be answered by having an in-depth understanding of equations. To help you maximize your examination marks, you should use the equation mindmaps to gain this in-depth understanding. You need to commit to memory much of the information contained in the equation mindmaps so that you can appreciate the story told by each equation.

Transcript of Visual Physics Online - School of Physics · VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are...

Page 1: Visual Physics Online - School of Physics · VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are essential part of physics, without them, we can’t ... Newton’s Second Law …

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VISUAL PHYSICS ONLINE

EQUATION MINDMAPS

Equations are essential part of physics, without them, we can’t

start to explain our physical world and make predictions. An

equation tells a story – a collection of a few symbols contains a

wealth of information. Many examination questions can be

answered by having an in-depth understanding of equations. To

help you maximize your examination marks, you should use the

equation mindmaps to gain this in-depth understanding. You

need to commit to memory much of the information contained

in the equation mindmaps so that you can appreciate the story

told by each equation.

Page 2: Visual Physics Online - School of Physics · VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are essential part of physics, without them, we can’t ... Newton’s Second Law …

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MECHANICS (Kinematics and Dynamics)

av

rv

t

x

dxv

dt

avg

v v ua

t t

dva

dt

Average velocity

Instantaneous velocity in X direction

Average acceleration

Instantaneous acceleration in X direction

F m a

Fa

m

F m g

2

C

vF m

r

2

c

C

F va

m r

Newton’s Second Law

acceleration

Weight of an object

Centripetal force: uniform circular motion

Centripetal acceleration

AB BA

F F Newton’s Third Law

Page 3: Visual Physics Online - School of Physics · VISUAL PHYSICS ONLINE EQUATION MINDMAPS Equations are essential part of physics, without them, we can’t ... Newton’s Second Law …

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rocket gasesF F

eg rocket propulsion

p mv

impulse J F t

J F t mv mu

0 0F p

Momentum of a moving object

Impulse of a force F acting for a time interval t

Impulse = change in momentum

Law of Conservation of momentum

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W F s

212K

E K mv

2 21 12 2

W F s mv mu

W qV

212K

E K mv e V

Work done by a force during a displacement (force and displacement in same direction [1D]

Kinetic energy of a moving object

Work done = change in KE [1D] only

Work done on a charge in an electric field

Gain in KE electron due to a constant accelerating voltage

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0

212

2 22

2

2

av

av

v u a t u v

s u t a t

v u a s

u vv

u vs v t t

Equation for uniform accelerated motion in one-dimension a = constant

2 2

212

0

cos

sin

2

2

x

x

x x x

y

y

y y y

y y y

y y

y y

a

u u

v u x u t

a g

u u

v u a t

v u a y

y u t a t

u vy t

2 2 2

2 2 2

tan

tan

y

x y s

x

y

x y v

x

ss s s

s

vv v v

v

Equations for

Projectile Motion

g = 9.8 m.s-2

ay = - g = - 9.8 m.s-1

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1 2

2

G m mF

r

planet

planet

planet

G Mg

R

1 2

p

m mE U G

r

pE U m g h

22

E E

E

G M G Mg

r R h

2L

Tg

Gravitational force

Acceleration due to gravity at surface of a planet

Gravitational potential energy

Gravitational potential energy near Earth’s surface

Acceleration due to gravity (Earth)

Period of pendulum g

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3

2 24

r G M

T

3 3

1 2

2 2

1 2

r r

T T

32

3 3

1 2

2 2

1 2

22 1

1

r r

T T

rT T

r

orb

G Mv

r

2

orb

rT

v

2esc

G Mv

r

Kepler’s Third Law for satellite motion

orbital velocity

orbital period

geostationary satellite T = 24 hours

escape velocity

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SPECIAL RELATIVITY

2

2

1

1

v

cv

c

0

02

21

tt t

v

c

2

0

0 21

LvL L

c

2E mc

2

21

mvp mv

v

c

2 2 2 2 4 2 2 2

0E p c m c p c E

22

02

21

mcK E E mc

v

c

212

K mv

00

EE E p c p

c

mass m is a constant time dilation length contract total energy momentum total energy kinetic energy kinetic energy v << c

photon

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ELECTRICITY

VR

I

P V I

Energy V I t

Resistance

Electrical power

Electrical energy

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MAGNETISM

1 2I IF

kL d

sinF B I L

0

2

IB

r

cos

F d

n B I A

Magnetic force between two parallel conductors

Magnetic force on a

conductor

Magnetic field surrounding a long straight conductor

Torque Torque on a coil in a magnetic field

cosB

B A

B

t

Bd

dt

cos

sin

BB A t t

B A t

battery backI R

Magnetic flux

average induced emf

induced emf

electric motor: back

emf back

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p p

s s

V n

V n

ps

s p s p

p s

nnV V I I

n n

s p s s p pP P V I V I

2

lossP I R

Transformer equation: step up or step down voltages

ideal transformer

Power loss (eddy currents – transformer, induction heating; transmission lines)

sinF qv B

FE

q

VE

d

Force on a charged particle moving in a magnetic field

Electric field

Electric field (constant) between two parallel charged plates

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NATURE OF LIGHT

E h f

c f

Energy of a photon

Speed of light Speed of electromagnetic radiation

212mv eV

212

21max min2

21max min2

h f m v W

h f m v W

m v h f W

21max2

min

s

s

eV mv

Wh fV

e e

21max2

min

min

0s

c c

eV mv

Wh f W f

h

Gain in KE of electron due to accelerating voltage

Photoelectric Effect

Stopping voltage

Cut-off (critical)

frequency

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THE ATOM

sinn d

2 2

1 1 1

f i

Rn n

2 1E E h f

2

hL mv r

1

1213.6 eV

n

EE E

n

2 11

1 15.29 10 m

nr r n r

Bragg’s Law – crystal structure (constructive interference)

Hydrogen atom -

spectrum

Energy levels

Bohr Model of atom

Angular momentum quantized

n = 1, 2, 3, … Energy levels hydrogen atom

Allowed orbits for

electrons in hydrogen

atom

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h

mv

hE h f c f p

h hp

p

4

hx p

de Broglie wavelength de Broglie relationship

Photon

Matter wave

Heisenberg Uncertainty Principle

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The NUCLUES

products reactantsm M M

2E mc

9 4 12

4 2 6

1

0Be He C n

Beta minus decay

en p e

232 228 4

90 88 2

4

2

Th Ra He

He

Mass defect

Einstein – mass/energy

Chadwick discovers neutron

Beta decay Pauli & Fermi neutrino

Alpha decay

Beta plus decayp+ n + e+ + e

19Ne10 19F9 + e+ + e

e+ +

p[d(-1/3) u(+2/3) u(+2/3)] n[d(-1/3) u(+2/3) d(-1/3)]

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Standard model

Proton

Neutron

Nuclear fission

protond (-1/2)u (+2/3)u (+2/3)

neutrond (-1/3)u (+2/3)d (-2/3)

235U92 + 1n0

236U92* 136Xe56 + 88Sr36 + 121n0