IB Physics - Ultimate Study Guide

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Orders of Magnitude

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40 Terms

1

Orders of Magnitude

A method to express large or small numbers using powers of ten (e.g., 10^4 for 10000).

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2

Significant Figures

The digits in a number that contribute to its precision, including all non-zero digits and any zeros between them.

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3

Uncertainty

An estimate of the difference between a measurement and the true value, influenced by random and systematic errors.

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4

Random Error

Unpredictable fluctuations in measurement readings due to uncontrolled factors.

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5

Systematic Error

Errors resulting from faulty systems or flaws in the experimental method.

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6

Absolute Uncertainty

Uncertainty expressed as a fixed quantity.

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7

Fractional Uncertainty

Uncertainty expressed as a fraction of the total measurement.

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8

Percentage Uncertainty

Uncertainty expressed as a percentage of the total measurement.

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9

Scalars

Quantities that have magnitude only (e.g., distance).

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10

Vectors

Quantities that have both magnitude and direction (e.g., displacement).

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11

Error Bars

Graphical representations of uncertainty in measurements on graphs.

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12

Lines of Best Fit

A straight line drawn to minimize the distance between data points on a graph.

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13

Kinematics

The study of motion, including concepts like distance, speed, and acceleration.

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14

Scalars vs

Scalars have only magnitude (e.g., speed), while vectors have both magnitude and direction (e.g., velocity).

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15

SUVAT Equations

Four kinematic equations used to describe motion with constant acceleration.

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16

Projectile Motion

Motion of an object under the influence of gravity, analyzed in vertical and horizontal components.

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17

Newton’s First Law

An object remains at rest or in uniform motion unless acted upon by a resultant force.

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18

Newton’s Second Law

The resultant force on an object is directly proportional to its acceleration (F=ma).

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19

Newton’s Third Law

For every action, there is an equal and opposite reaction.

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20

Contact Forces

Forces that act between objects in physical contact (e.g., friction).

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21

Non-Contact Forces

Forces that act at a distance (e.g., gravitational force).

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22

Hooke’s Law

The extension of a material is directly proportional to the applied force up to the limit of proportionality.

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23

Conservation of Linear Momentum

The total momentum before a collision equals the total momentum after, barring external forces.

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24

Impulse

The change in momentum of an object, equal to the force applied over time.

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25

Centripetal Force

The force required to keep an object moving in a circular path, directed towards the center of the circle.

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26

Thermal Equilibrium

A state where two objects share the same temperature, resulting in no net heat flow.

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27

Specific Heat Capacity

The amount of heat required to raise the temperature of 1 kg of a substance by 1 K.

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28

Phase Change

The transition of a substance from one state of matter to another (e.g., melting, boiling).

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29

Pressure

The force exerted per unit area, calculated as P = F/A.

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30

Ideal Gas Equation

PV = nRT, relating pressure, volume, temperature, and the number of moles of a gas.

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31

Kinetic Model of an Ideal Gas

Assumes perfectly elastic collisions and negligible molecular volume.

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32

Simple Harmonic Motion (SHM)

A type of periodic motion where the restoring force is proportional to the displacement.

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33

Wave Properties

Characteristics of waves, including amplitude, wavelength, frequency, and speed.

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34

Doppler Effect

The change in frequency or wavelength of a wave in relation to an observer moving relative to the source of the wave.

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35

Gravitational Field

A region where a mass experiences a force due to another mass.

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36

Electric Field

A region where a charge experiences a force due to another charge.

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37

Capacitance

The ability of a system to store charge per unit voltage.

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38

Electromagnetic Induction

The process of generating an electromotive force (EMF) through a changing magnetic field.

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39

Quantum Tunneling

A phenomenon where particles pass through a potential barrier they classically shouldn't be able to cross.

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40

Stellar Evolution

The process by which a star changes over time, including stages like main sequence, red giant, and supernova.

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