Quantum Flashcards

(77 cards)

1
Q

Photon

A

discrete packet of energy of electromagnetic radiation. The energy of one photon is directly proportional to the frequency of electromagnetic radiation.

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2
Q

Photoelectric effect

A

emission of electrons when electromagnetic radiation of high-enough frequency is incident on a cold metal surface

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3
Q

Work function

A

The work function of a metal is the minimum energy needed to remove the least tightly bound electron from the metal’s surface.

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4
Q

Threshold frequency

A

The threshold frequency is the minimum frequency of electromagnetic radiation for electrons to be removed from the metal’s surface

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5
Q

Stopping Potential

A

The stopping potential is the minimum potential difference between the emitting metal and the collector that prevents the most energetic photoelectrons from reaching the collector plate, thus resulting in 0 photoelectric current.

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6
Q

Evidence/observations from photoelectric emission that provide evidence for particulate nature of electromagnetic radiation

A
  1. Emission of electrons only when electromagnetic radiation is above a minimum frequency regardless of intensity
  2. Maximum kinetic energy of electrons depends on frequency of electromagnetic radiation
    Maximum kinetic energy of electrons is independent of intensity
  3. Instantaneous emission of electrons when electromagnetic radiation is above a certain frequency
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7
Q

Absorption Spectra

A

An absorption spectra is a continuous spectrum crossed by dark lines.

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8
Q

Emission Spectra

A

An emission spectra is discrete bright lines of different colours on a dark background.

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9
Q

De Broglie Wavelength

A

The De Broglie Wavelength is the wavelength of the matter wave that is associated with a moving particle.

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10
Q

Excitement of atoms

A

When atoms are excited, an orbiting electron takes in energy to move to a higher energy level.

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11
Q

Heisenberg’s Uncertainty Principle

A

If a measurement of position is made with precision Δx and a simultaneous measurement of momentum is made with precision Δp the product of those two uncertainties can never be smaller than the Planck constant. (ΔxΔp≥h)

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12
Q

Spectra as proof of discrete energy levels in the atom

A
  1. Each coloured/dark line corresponds to one wavelength or frequency,
  2. representing photons of a specific energy given by E=hf
  3. that is emitted/absorbed when orbital electrons undergo energy changes
  4. when de-exciting/exciting between discrete energy levels in the atom.
    (Absorbed photons are then re-emitted in all directions shortly when the unstable, excited atom de-excites.)
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13
Q

Broad Continuous Background in X-ray spectrum (Braking Radiation)

A

X-ray photons are produced when the electrons/charged particles are stopped or decelerated suddenly. When electrons/charged particles strike the target metal, they experience a range of decelerations, so photons possess a continuous distribution of energies, and hence have a continuous distribution of wavelengths.

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14
Q

Minimum wavelength appears as a sharp cut-off

A

The minimum wavelength corresponds to the most energetic photons, which are produced when all kinetic energy of one electron/charged particle is converted into one X-ray photon.

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15
Q

Characteristic peaks in X-ray Spectrum

A

When bombarding electrons collide with orbiting inner shell electrons of the metal atoms with sufficient energy, the inner shell electron is ejected. Outer shell electrons will transit to the lower energy level, releasing an X-ray photon of photon energy exactly equal to the difference between the two energy levels.

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16
Q

N1L

A

An object will continue to be in a state of rest or move with constant velocity, unless acted upon by a net external force.

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17
Q

N2L

A

The rate of change of momentum of a body is directly proportional to the resultant force acting on it, and takes place in the direction of the resultant force.

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18
Q

N3L

A

When object A exerts a force on object B, object B will exert an oppositely directed force of the same type of equal magnitude on object A.

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19
Q

Impulse

A

The impulse of a force is the product of the average force and the time interval during which the force acts. or
The impulse of a force is the integral of a force over the time interval during which the force acts.

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20
Q

PCM

A

The total linear momentum of an isolated system of interacting bodies before and after collision remains constant provided that no net external force acts on the system.

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21
Q

Diffraction

A

Diffraction is the spreading of waves towards the geometric shadow after passing through an aperture.

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22
Q

Interference

A

Interference is the phenomenon observed when waves from two (or more) coherent sources overlap and, in accordance to the Principle of Superposition, produces a pattern of maximas and minimas.

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23
Q

Coherent

A

Sources are coherent if they produce waves that have a constant phase difference.

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24
Q

Principle of Superposition

A

The Principle of Superposition states that when two or more waves of the same type meet, the resultant displacement at any point is the vector sum of the individual displacements that each wave would cause at that point.

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25
Rayleigh Criterion
The limit for which the two objects can be just distinguishable occurs when the first minima of the diffraction pattern of one source coincides with the central maxima of the diffraction pattern of the other source.
26
Formation of Interference pattern
For steady and observable interference patterns, the following conditions must be met: 1. The waves must overlap. (For superposition to occur) 2. The waves from the sources must have constant phase difference (of the same type, have same wavelength and frequency). (For interference pattern to be formed) 3. The waves must have approximately the same amplitude. (For good contrast between maximas and minimas) 4. For transverse waves, they must either be unpolarised, or polarised in the same plane. (For good contrast between maximas and minimas) 5. Same nature of wave (1 and 2 make the pattern observable, point 3 and 4 give it good contrast)
27
Simple Harmonic Motion
Simple Harmonic Motion is a type of oscillatory motion where: 1) the magnitude of the acceleration is always directly proportional to the displacement from the reference point, and 2) the acceleration is directed opposite to its displacement.
28
Critical Damping
The point at which no complete oscillation takes place, and the time taken for the oscillating body to come to rest is the shortest.
29
Resonance
The phenomenon in which there is maximum transfer of energy from the driver to the oscillator when the driving frequency matches the natural frequency of the undamped oscillator. The oscillations will achieve maximum amplitude.
30
Equilibrium Position
Equilibrium Position is the natural position of the mass where no net force acts on the oscillating mass.
31
Free oscillations
constant vibration amplitude of oscillating body without energy loss (due to lack of resistance forces or external applied forces)
32
Angular Frequency (⍵)
Angular frequency is the rate of change of phase of the oscillating mass.
33
Phase difference
Phase difference is a measure of how much an oscillation is out of step with itself at 2 different instances in time, or how much 2 oscillations are out of step with each other at the same instant in time.
34
Phase
Phase is an angular measure of the fraction of a cycle that has been completed by the oscillating mass.
35
Frequency
Frequency is the number of complete to-and-fro oscillations per unit time made by the oscillating mass.
36
Displacement
Displacement is the position vector of the oscillating mass measured from its equilibrium position at a particular instant.
37
Amplitude
Amplitude is the maximum displacement of the oscillating mass from the equilibrium position in either direction.
38
Period
Period is the time taken for one complete oscillation of the oscillating mass.
39
Random error
Measured readings are scattered about the mean value with no fixed pattern.
40
Systematic error
Measurements that are consistently higher or lower than the actual value.
41
Accuracy
The degree to which a reading on an instrument approaches the true value of the quantity being measured.
42
Precision
How close the experimental values are to each other. OR The smallest interval to which an instrument can measure.
43
Displacement, Velocity, Acceleration
Displacement Shortest distance, in a specific direction, from a reference point. Velocity Rate of change of displacement. Acceleration Rate of change of velocity.
44
Elastic, inelastic, p. elastic collision
Elastic collision A perfectly elastic collision is one in which the total kinetic energies of the colliding bodies are conserved(remains constant before and after the collision). Inelastic collision An inelastic collision is one in which the sum of kinetic energies of the colliding bodies are not conserved. Total Kinetic energy after the collision is lesser than before it. Perfectly inelastic collision A perfectly inelastic collision is one in which the colliding bodies stick together and move off with the same velocity.
45
Hooke’s Law
The change in length, x, of a material, is directly proportional to the force applied to it, F, provided the limit of proportionality is not exceeded.
46
Archimedes’ Principle
When a body is wholly or partially immersed in a fluid, it is buoyed by an upthrust equal in magnitude and opposite in direction to the weight of fluid displaced by the body.
47
Centre of gravity
The point where all the weight seems to act.
48
Couple
A couple is a pair of forces acting on the same body, which are of equal magnitude and opposite in direction and whose lines of action do not coincide.
49
Upthrust
Upthrust is the upward force exerted by a fluid on an object submerged fully or partially in the fluid due to the difference in pressure exerted by the fluid on the upper and lower surfaces of the object. It acts through the centre of mass of the displaced fluid and is equal in magnitude and opposite in direction to the weight of fluid displaced by the body.
50
Conditions for Equilibrium
Translational Equilibrium: The vector sum of forces acting on the body must be 0 along all directions. Rotational Equilibrium: The net torque acting on the body must be 0 about all axes.
51
Principle of Moments
For an object in rotational equilibrium, the sum of clockwise moments acting on the object about any point must be equal to the sum of anticlockwise moments acting on the object about the same point.
52
Work
The work done on a body by a force is the product of the force and the displacement of the body in the direction of the force.
53
Law of conservation of energy
Energy can be converted from one form to another but cannot be created or destroyed. The total energy of an isolated system is always constant.
54
Power
Rate of work done.
55
Radian, Ang disp, ang vel
Radian The radian is the angle subtended at the centre of a circle by an arc whose length is equal to the radius of the circle. Angular displacement The angular displacement is the angle swept out by the radius, in a specific direction from the original position. Angular velocity Angular velocity is the rate of change of angular displacement.
56
How uniform circular motion arises
Force* always perpendicular to motion of the object no displacement in the direction of the force and hence no work done by force and the KE of the object is constant thus, the force being constant in magnitude merely provides centripetal force required for the object to undergo uniform circular motion.
57
Why is there no work done during circular motion
Force* that provides centripetal force for the object to undergo uniform circular motion is always perpendicular to the motion of the object. As such, there is no displacement in the direction of the force and hence, there is no work done.
58
Gravitational Field
A gravitational field is a region of space in which a mass experiences a gravitational force.
59
Gravitational Potential
Work done per unit mass (by an external force) in bringing a small test mass from infinity to that point in the field.
60
Gravitational Potential Energy at a point
The work done by an external force in bringing the mass from infinity to that point in the field.
61
Gravitational Field Strength
The gravitational force per unit mass experienced by a small test mass at that point in the field. (Small and test are important because they highlight the idea that the mass should not distort the pre-existing gravitational field. Similar idea for E-field: small test charge.)
62
Newton’s Law of Gravitation
The gravitational force of attraction between any two masses is directly proportional to the product of their masses and inversely proportional to the square of the distance between them [magnitude] and acts along the line joining the two point masses [direction]
63
Geostationary
A geostationary satellite is one which always remains at a fixed point above the Earth’s surface. Properties: Orbital axis coincides with that of earth’s rotation. Same orbital period as earth (24 hours) Orbits around the equator in the west to east direction.
64
Relationship between Gravitational potential and gravitational field strength.
Gravitational field strength at a point is numerically equal to the gravitational potential gradient at that point and directed towards lower potential.
65
The acceleration of free fall at the Equator is not equal to the acceleration of free fall at the poles. Explain why they are different.
At the equator, part of the acceleration of free fall provides centripetal force for circular motion. Since the radius of circular motion at the equator is larger, an object experiences greater centripetal force, so the acceleration of free fall is lower than at the poles.
66
By reference to lines of gravitational force near to the surface of the Earth, explain why the gravitational field strength g close to the Earth’s surface is approximately constant.
At the surface, lines of gravitational force are radial Earth has a large radius, so lines are equally spaced and approximately parallel near the surface Parallel lines means there is constant field strength
67
Why gravitational potential is a negative value for an isolated mass.
Gravitational potential at infinity is defined as zero. Gravitational forces are attractive, so work done by an external force is opposite to displacement. (Work is done by the external force against the field) Work done per unit mass by the external agent is negative/Loss in gravitational potential energy when moving from infinity to the point. (Since the mass begins at 0 gravitational potential energy, a loss in gravitational potential energy results in a negative value for gravitational potential.)
68
The acceleration of free fall at the Equator is not equal to the acceleration of free fall at the poles. Explain why they are different.
At the equator, part of the acceleration of free fall provides centripetal force for circular motion. Since the radius of circular motion at the equator is larger, an object experiences greater centripetal force, so the acceleration of free fall is lower than at the poles.
69
Explain, in terms of energy, the impact of atmospheric drag on the subsequent trajectory of geostationary satellites.
Work is done against drag, total energy (-GMm2r) decreases. Gravitational potential energy (-GMmr) decreases, satellite lowers in height. Kinetic energy (GMm2r) increases, satellite’s linear speed increases. Satellite spirals to Earth with increasing speed.
70
Explain why the centripetal force acting on 2 stars has the same magnitude.
Gravitational force provides centripetal force for their circular motion By Newton’s 3rd Law, both stars experience the same magnitude of gravitational force
71
It is then required to reposition the satellite at an orbit closer to the Sun than that in (d). State and explain whether the work done on the satellite is positive, negative, or zero to change the position of the satellite to a lower orbit. Effect of orbital radius on total energy
Changing satellite to a lower orbit, the gain in KE is less than the loss in PE OR Total energy decreases. Hence Negative work is done. -GMmr+GMm2r=-GMm2r(PE+KE=Total Energy, r decreases, total energy decreases.)
72
Thermal equilibrium
When two bodies are in thermal equilibrium, there is no net flow of heat between them when they are in thermal contact.
73
Avogadro’s Number
Avogadro’s number is the number of atoms in 12g of carbon-12.
74
Absolute zero
Absolute zero is defined as the zero point on the absolute temperature scale.
75
Ideal Gas
An ideal gas obeys the equation of state: PV=nRT, at all pressures P, at all volumes V, for all moles of the gas n, at all temperatures T, where R is the molar gas constant.
76
Heat
Heat is thermal energy that flows from a region of higher temperature to a region of lower temperature.
77
Thermometric property
A thermometric property of a substance is one which varies with temperature.