component 2 Flashcards

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1
Q

Efficiency of a system

A

% efficiency = (useful work out) / (work put in) X 100

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2
Q

Potential difference (pd), V

A

Potential difference is the difference in the amount of energy that charge carriers have between two points in a circuit.

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3
Q

Ohm’s law

A

The current in a metal wire at constant temperature is

proportional to the pd across it.

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4
Q

Superconducting transition temperature, Tc

A

The temperature at which a material, when cooled, loses all its electrical resistance, and becomes super-conducting. Some materials (e.g. copper) never become superconducting however low the temperature becomes.

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5
Q

The law of conservation of charge

A

Electric charge cannot be created or destroyed, (though positive and negative charges can neutralise each other). Charge cannot pile up at a point in a circuit.

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6
Q

Emf, E

A

The emf of a source is the energy converted from some other form (e.g. chemical) to electrical potential energy per coulomb of charge flowing through the source.

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7
Q

Capacitor

A

A capacitor is a pair of conducting plates separated by an insulator. If a potential difference is placed across the plates, they acquire equal and opposite charges.

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8
Q

Dielectric

A

Insulator between the plates of a capacitor, also serving to make the capacitance larger than if there were just empty space.

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9
Q

Hooke’s law

A

The tension in a spring or wire is proportional to its extension from its natural length, provided the extension is not too great (doesn’t exceed elastic limit)

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10
Q

Ductile material

A

A material which can be drawn out into a wire. This implies that plastic strain occurs under enough stress.

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11
Q

Elastic limit

A

This is the point at which deformation ceases to be elastic. For a specimen it is usually measured by the maximum force, and for a material, by the maximum stress, before the strain ceases to be elastic.

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12
Q

Brittle material

A

Material with no region of plastic flow, which, under tension, fails by brittle fracture

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13
Q

Newton’s law of gravitation

A

The gravitational force between two particles is proportional to the product of their masses, m1 and m2, and inversely proportional to their separation squared, r^2

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14
Q

Coulomb’s law

A

The electrostatic force, F, between two small bodies is

proportional to the product of their charges, Q1 and Q2, and inversely proportional to their separation squared, r^2.

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15
Q

Electric field strength, E

A

The force experienced per unit charge by a small positive charge placed in the field. This is a vector quantity.

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16
Q

Gravitational field strength, g

A

The force experienced per unit mass by a mass placed in the field. This is a vector quantity

17
Q

Electric potential, VE

A

Electric potential at a point is the work done per unit charge in bringing a positive charge from infinity to that point. (scalar)

18
Q

Gravitational potential, Vg

A

Gravitational potential at a point is the work done per unit mass in bringing a mass from infinity to that point. (scalar)

19
Q

Black Body

A

A black body is a body (or surface) which absorbs all the electromagnetic radiation that falls upon it. No body is a better emitter of radiation at any wavelength than a black body at the same temperature.

20
Q

Absolute or kelvin temperature

A

At 0 K (-273.15°C) the energy of particles in a body is the lowest it can possibly be

21
Q

Boyle’s Law

A

pV is a constant : at constant temperature pressure and volume of a gas are inversely proportional

22
Q

Charles’s Law

A

V/T is constant : at constant pressure the volume of a gas is directly proportional to temperature

23
Q

Pressure Law

A

p/T is constant : at a constant volume the pressure of a gas is directly proportional to temperature

24
Q

Brownian Motion

A
  • particles suspended in a fluid move randomly as a result of collisions with fast randomly moving particles
  • random motion is where particles have a range of speeds and no preferred direction of movement
25
Q

Kepler’s laws of planetary motion: 1

A

Each planet moves in an ellipse with the Sun at its focus.

26
Q

Kepler’s laws of planetary motion: 2

A

The line joining a planet to the centre of the Sun sweeps out equal areas in equal times.

27
Q

Kepler’s laws of planetary motion: 3

A

T^2, the square of the period of the planet’s motion, is
proportional to r^3, in which r is the semi-major axis of its ellipse. [For orbits which are nearly circular, r may be taken as the mean distance of the planet from the Sun.]

28
Q

Kirchoff’s first law

A

Kirchhoff’s current law (1st Law) states that current flowing into a node (or a junction) must be equal to current flowing out of it. This is a consequence of charge conservation.

29
Q

Kirchoff’s second law

A

Kirchhoff’s voltage law (2nd Law) states that the sum of all voltages around any closed loop in a circuit must equal zero. This is a consequence of charge conservation and also conservation of energy.

sum of the EMF’s = sum of PD’s

30
Q

Current

A

Current is the rate of flow of charge, and travels in the direction that a positive test charge would