Physics Definition Flashcards

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1
Q

Newton’s first law

A

A body will continue in a state of rest or uniform motion unless acted on by an external force.

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2
Q

Newton’s second law

A

The rate of change of momentum is directly proportional to the unbalanced force applied to a body.

Simplified to:The acceleration of a body is proportional to the force applied and inversely proportional to the mass.
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3
Q

Newton’s third law

A

If body A exerts a force on body B, then body B will exert and equal and opposite force to body A.

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4
Q

Impulse

A

The change of momentum by the average resultant force applied during a time interval.

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5
Q

Elastic/Inelastic collision

A

An elastic collision conserves all KE, an inelastic one doesn’t.

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6
Q

Temperature

A

The absolute temperature is a measure of the average random kinetic energy of particles.

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7
Q

Absolute zero

A

The temperature at which all random motion of molecules stops, 0K.

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8
Q

Specific heat capacity

A

The amount of energy needed to increase the temperature of 1kg of a substance by 1K

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9
Q

Thermal capacity

A

The amount of energy needed to increase the temperature of a body by 1 K

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10
Q

Specific latent heat

A

The energy needed to change the phase of 1kg of a substance without change in temperature.

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11
Q

Ideal gas

A

A gas that has no intermolecular forces or potential energy. Undergoes elastic collisions. Has negligible volume compared to its container.

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12
Q

Boyle’s law

A

The pressure of a fixed mass of gas at constant temperature is inversely proportional to its volume.

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13
Q

Charle’s law

A

The volume of a fixed mass of gas at constant pressure is directly proportional to its temperature in Kelvin.

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14
Q

Pressure law

A

The pressure of a fixed mass of gas at constant volume is directly proportional to its temperature in Kelvin.

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15
Q

Newton’s law of gravitation

A

Every point mass attracts every other point mass with a force that is inversely proportional to the square of their separation.

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16
Q

Gravitational field

A

A region where a mass will experience an attractive force.

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17
Q

Gravitational field strength

A

The force per unit mass on a small point mass placed in the field.

18
Q

Gravitational potential energy

A

Energy possessed by a mass in a field.

The work done taking a mass from infinity (zero PE) to its position in a field.

19
Q

Gravitational potential

A

The work done per unit mass taking a point mass from infinity (zero PE) to its position in a field.

20
Q

Simple harmonic motion

A

Motion where the acceleration is proportional to the displacement and directed in the opposite direction.

21
Q

Phase difference

A

The angular difference between two identical points on two waves.

22
Q

Path difference

A

The distance between two identical points on two waves.

23
Q

Superposition

A

The addition of two or more waves.

24
Q

Standing waves

A

The result when two traveling waves of the same wavelength from opposite directions superpose, creating nodes and antinodes.

25
Q

Diffraction

A

The spreading when a travelling wave passes through or around a barrier.

26
Q

Coulomb’s law

A

The force experienced by two point charges is directly proportional to the product of their charge and inversely proportional to the square of their separation.

27
Q

Potential difference

A

The work done per unit charge taking a small positive charge from A to B.

28
Q

Ohm’s law

A

The current through an ohmic conductor is directly proportional to the p.d. across it at constant temperature.

29
Q

EMF

A

The energy converted from chemical to electrical potential when one unit charge flows, or the workdone taking unit charge from one terminal to the other.

30
Q

One Ampere

A

Defined as the current that would cause a force of 2×10-7N per metre between two long parallel conductors, separated by 1 m in a vacuum.

31
Q

Half life

A

The time taken for half the nuclei to decay (or activity to halve).

32
Q

Decay constant

A

The probability of decay in one second. Gives the rate of decay for a given number of nuclei.

33
Q

Baryon

A

Made of 3 quarks – proton, neutron.

34
Q

Meson

A

Made of 2 quarks – pi meson

35
Q

Leptons

A

Electron, muon, tau, and their neutrinos.

36
Q

Exchange bosons

A

Responsible for the interactions between particles.

37
Q

Moderator

A

Material (e.g. graphite) used to slow down neutrons so they are absorbed by fissile 235U.

38
Q

Control rods

A

Used to absorb neutrons to slow down the reaction – e.g. boron.

39
Q

Black body

A

A body that re-emits all energy it absorbs.

40
Q

Emissivity

A

The ratio of energy radiated by a body to the energy radiated by a perfect black body at same temperature.

41
Q

The greenhouse effect

A

The Earth radiates EM radiation in the IR region of the spectrum. This is absorbed by the greenhouse gases in the atmosphere and re-radiated in all directions.

42
Q

Enhanced greenhouse effect

A

Burning fossil fuels increases CO2 concentration leading to temperature increase.