Heat and Thermo Flashcards

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1
Q

What is the zeroth law of thermodynamics?

A

This law is related to the existence and definition of temperature.

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2
Q

What is the first law of thermodynamics?

A

This law is nothing more than a statement of the
conservation of energy. Basically it says that energy may be transferred into or out of a substance as either work or heat, but the total amount of energy remains constant.

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3
Q

What is the second law of thermodynamics?

A

At a technical level the second law is a statement about something called entropy. From a microscopic point of view entropy is related to randomness, disorder and probability.

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4
Q

What is temperature typically measured in and how do you convert it?

A

As you know, absolute zero is the coldest possible temperature. At absolute zero we have: Absolute zero: T = 0 K and TC = −273.15 ◦C

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5
Q

Thermoscope vs Thermometer

A

A thermometer – which is an instrument which measures
the actual temperature of a substance

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6
Q

Thermal Contact vs Thermally isolated vs Thermal Equalibrium

A

Then, two bodies are said to be in thermal contact with one another if heating just one of the bodies results in some macroscopic change in the other.
—————————————————————————————————-Two bodies are said to be thermally isolated from one another if
heating just one of the bodies results in no macroscopic change in the other.
—————————————————————————————————-
Two bodies are said to be in thermal equilibrium with one another if they are in thermal contact and no macroscopic changes occur in either body as time passes.

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7
Q

Example of bodies A, B and Z

A

The zeroth law of thermodynamics: If bodies A and B are each in thermal equilibrium with a body Z, then A and B are in thermal equilibrium with each other. Thus we can say that two bodies have the same temperature if they are in thermal equilibrium with each other.

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8
Q

Define Thermal Expansion

A

A well known property of almost all substances is their tendency to expand or grow in size as their temperature increases.

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9
Q

What is the equation of linear expansion?

A

This equation describes how measured lengths change as the temperature changes: ∆L = Liα∆T linear expansion where α is a constant called the coefficient of linear expansion which has the units of K^−1 or ◦C ^−1.

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10
Q

Example of Expansion using a ring/washer

A

If I increase the temperature of a ring or a washer, the hole gets bigger (not smaller as you might have guessed)

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11
Q

What is the equation of volume expansion?

A

Used when computing volume changes of either liquids or solid bodies: ∆V = Viβ∆T, where β is a constant called the coefficient of volume expansion -> for a solid β = 3a

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12
Q

What is the macroscopic state of a gas and what are the 3 state variables for gases?

A

The macroscopic state of a gas in thermal equilibrium is fully specified by its temperature, pressure and volume.

Temperature is denoted by the symbol T and has SI units of kelvin (K)

Pressure is denoted by the symbol p and has SI units of pascals or newtons per square metre (Pa or N m^−2)

Volume is is denoted by the symbol V and has SI units of cubic metres (m^3 )

Note: state variables are also known as s state parameters or thermodynamic variables.

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13
Q

What are the 2 equation for ideal gas law/ideal gas equation?

A

pV = nRT, where R = 8.314 J K^−1 mol^−1 is called the universal gas constant and pV = N kT, where N is the number of gas particles (molecules or atoms) and k = 1.381 × 10−23 J K^−1 is called Boltzmann’s constant

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14
Q

What is the equation of ideal gas law for a number of fixed particles?

A

pV/T = constant, typically written as p1V1 / T1 = p2V2 / T2

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15
Q

What are the the three special cases of ideal gas law and their equations?

A

Boyles Law: The temperature and the number of particles of the gas doesn’t change throughout a process -> p1V1 = p2V2

Charles Law : The pressure and the number of particles of the gas doesn’t change throughout a process -> V1 / T1 = V2 / T2

Gay-Lussac’s law: The volume and the number of particles of the gas doesn’t change throughout a process ->p1 / T1 = p2 / T

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16
Q

Why is it important that a gas must be in thermal equalibrium?

A

It is extremely important to understand that a gas must be in thermal equilibrium with its immediate surroundings for us to be able to talk about its pressure and temperature (and often volume too). This point was not stressed in the last section, but you need to be aware that p and T (and often V ) are not defined and cannot be measured if the gas is not in thermal equilibrium.

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17
Q

What is a quasi-static process?

A

A process which is carried out so slowly that equilibrium is established at all in-between points. A quasi-static process carried out at constant temperature is called isothermal - If you connect together all points on a pV diagram which have the same temperature you will form a smooth curve called an isotherm,

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18
Q

What is the kinetic theory of gases?

A
  1. Newton’s laws apply to the gas particles.
  2. The gas particles take up no volume (or are very tiny compared to the average distance between them) and are all identical.
  3. The gas particles are constantly moving in random directions with a distribution of speeds that are independent of the direction of motion.
  4. There are no attractive or repulsive forces acting between the gas particles or the surroundings. Except for collisions between other particles and the container walls the particles are free. They have no potential energy, just kinetic energy.
  5. The gas particles undergo elastic collisions with each other and the container walls. No kinetic energy is lost in collisions.
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19
Q

What is the formula for average transational kinetic energy?

A

K ave,trans = 1/2 mv^2 = 3/2 kT

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20
Q

What is the formula for the thermal speed of the particle in terms of the gas temperature and particle mass?

A

vth = sqrt(3kT / m)

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21
Q

Define ideal monatomic gas

A

An ideal gas consisting of point-like particles is said to be an ideal monatomic gas since the gas particles are just free atoms -> need to go over monatomic, diatomic and polyatomic…

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22
Q

System, Evironment and Boundary

A

The part of the universe that we are interested in is called the system. Everything else around the system which may interact with it in some way is called the environment. The two dimensional surface which separates the system and the environment – whether it be real or imagined – is called the boundary.

23
Q

Define Thermodynamic Process

A

The procedure by which you change a system from one state to another state, where

Open system: A system without any restrictions. It can exchange energy and matter with its environment.

Closed system: A system which can exchange energy with its environment, but not matter.

Isolated system: A system which cannot interact in any way with its environment. No energy or matter can be exchanged with its environment.

24
Q

If temperature is Ts and enviroment is Te what a the 3 cases?

A

Case I: If Ts = Te then nothing happens. The system and environment are in thermal equilibrium.

Case II: If Ts > Te then the system is hotter than the environment and energy will be transferred from the system to the environment.

Case III: If Ts < Te then the system is colder than the environment and energy will be transferred from the environment to the system.

25
Q

Define heat

A

The energy transferred across the boundary between a system and its environment due to a temperature difference between them

26
Q

Define work

A

The energy transferred between a system and its environment due to a force acting over some displacement. The work done on a system is denoted by W and is measured in joules

27
Q

What is the formula for heat capacity and define it?

A

Q = C∆T = C(Tf − Ti), where Tf and Ti can be measured in either ◦C or K.
Heat capacity: The constant C of proportionality between the heat added and the temperature change
.

28
Q

What is the formula for specific heat and define it?

A

Q = mc∆T -> the temperature change of the sample; m is the mass of the sample; and c and is measured in J kg^−1 K ^ −1or J kg^−1 ◦C ^−1

29
Q

What is the formula for molar specfic heat?

A

Q = nC∆T -> Molar specific heat has SI units of J mol−1 K^−1 or J mol^−1 ◦C ^−1
.

30
Q

Define Phase change/transition

A

When the state of the substance (i.e. solid, liquid or gas) is altered

Whenever we heat something, the energy transferred can either go into: (i) increased kinetic energy of the consistent atoms or molecules, which registers as an increase in temperature; (ii) overcoming attractive forces between the molecules (i.e. increasing the potential energy shared between molecules), which registers as a phase transformation; or simultaneously both (i) and (ii)

For pure substances (i.e. substances made from only one type of molecule or atom), (i) or (ii) can occur but never both at the same time. That is, for pure substances the temperature remains constant as it changes phase. For substances which are mixtures (i.e. not pure) the behaviour can be far more complicated

31
Q

Define heat transformation and give its formula

A

Where L can be: Lf - heat of fusion or heat of melting. If the phase transformation is from liquid to gas, L is denoted by Lv and is called the heat of vaporization. If the phase transformation is from solid to gas, L is denoted by Ls and is called the heat of sublimation.

32
Q

Define phase diagram and its components (triple points and critical point)

A

A phase diagram is a simple means of showing under which conditions a substance undergoes phases transitions, and under which conditions the substance is a solid, liquid or gas.

The so-called triple point is a point on the plot under which all three phases are in thermal equilibrium

The so-called critical point is the point at which the boundary between the gas and liquid phases terminates

33
Q

What are all the typical transitions?

A

constant pressure melting: solid −→ liquid (f −→ g)
constant pressure freezing: liquid −→ solid (g −→ f)
constant pressure sublimation: solid −→ gas (e −→ d)
constant pressure deposition: gas −→ solid (d −→ e)
constant temperature boiling: liquid −→ gas (a −→ c)
constant pressure boiling: liquid −→ gas (a −→ b)
constant temperature condensing: gas −→ liquid (c −→ a)
constant pressure condensing: gas −→ liquid (b −→ a)

34
Q

Name the three heat transfer mechanisms

A

Energy is transported from a hotter body to a colder
body: conduction, convection and radiation

35
Q

What is thermal conduction and give its formula?

A

Is heat transfer by direct physical contact. More specifically, at the microscopic level, conduction is an energy transferred from more
energetic particles to less energetic particles via continuous collisions between them -> H = kA * ((Th − Tc) / L)

36
Q

Thermal conduction and thermal resistance

A

R = L / kA, which changes thermal conduction to H = (Th − Tc) / R

37
Q

What is convection and explain its steps/process?

A

  1. The temperature of the part of the fluid in thermal contact with the hot substance
    will increase.
  2. In getting hotter, the part of the fluid which is in thermal contact with the hot substance will thermally expand and decrease in density.
  3. Having a lower density than the surrounding fluid, the hotter part of the fluid will rise due to buoyant forces.
  4. Some of the surrounding cooler and more dense fluid will move in to replace the upward moving hotter fluid.
  5. ## Some cooler fluid is now in thermal contact with the heat source and the process repeats.A macroscopic fluid flow will be established by convection which is called a convection current
38
Q

What is thermal radiation and give its formula

A

The final mechanism by which a system and its environment can exchange energy as heat is through electromagnetic radiation or light. Often the radiation exchanged between two bodies – or a system and its environment – due to a temperature difference is called thermal radiation -> Stefan-Boltzmann law: Pem = eσAT4

Here Pem is the total power emitted by the object in watts, σ = 5.67 × 10^−8 W m^−2 K&^−4 is the Stefan-Boltzmann constant and e is the emissivity of the object’s surface. The emissivity is a dimensionless number which has a value between 0 and 1 depending on the composition of the object. A perfect emitter – a so-called blackbody radiator – has an emissivity of e = 1

39
Q

Understanding work (done on and into)

A

we denote the work done on the system by the environment as W and the amount of heat transferred into the system from the environment by Q. Carefully note that in being defined this way, either of the two separate quantities Q and W might be positive, negative or zero depending on what exactly is going on.

40
Q

What is internal energy, the change in internal energy and the formlula for it?

A

if a system starts in an initial state i and has an initial internal energy Ui , and then has its state changed via some thermodynamic process and ends up in a final state f with a final internal energy Uf , then the change in internal energy of the system is:

∆U = Uf − Ui = Q + W

where Q is the heat transferred to the system and W the work done on the system during the process.

This is also the first law of thermodynamics

41
Q

What is the formula for infinitesimally small change in state?

A

dU = dQ + dW

42
Q

What is the formula for internal energy of a monatomic ideal gas?

A

U =3/2 * nRT

43
Q

What is the formula for monatomic ideal gas of any process

A

U =3/2 * nR∆T

44
Q

What is an important thing to remember any ideal gas

A

The internal energy of any ideal gas is a function only of its temperature and does not depend on any other variable. The internal energy of any ideal gas will not change if its temperature does not change.

45
Q

What is the formula for infinitesimal work done on a gas and total work done on a gas

A

Infinitesimal work done on a gas: dW = −pdV

Total work done on a gas: W = ∫dW = − Vf∫Vi pdV

Note that: The expressions above are always true for any gas as it undergoes any kind of quasi-static volume change

46
Q

Different paths – same change of internal energy

A

if we take a gas from a state i to f, the change of internal energy
is just ∆U = Uf − Ui. If we take this gas from i to f via different quasi-static paths, the change of internal energy will always be the same value no matter what the actual process is since internal energy is just the total energy stored in the gas. However, the work W done on the gas and the heat Q added to the gas do depend on the actual process or path taken. For this reason W and Q are said to be path-dependent quantities, whilst ∆U is said to be a path-independent quantity. THUS we say that heat and work are path-dependent quantities, whereas the internal energy is path-independent.

47
Q

What are the 5 process, their characteristics, the first law relationship, work and other relationships

A

REFER TO IMAGE -> isochoric, isobabaric, isothermal, adiabatic and free expansion

48
Q

Why is a quasi-static process reversable

A

An important feature of a quasi-static processes is that it is reversible: if a system starts in a state i and is taken through a quasi-static processes to a state f, we can easily reverse the process and take the system back from f to i. The reason that all quasi-static processes can be reversed is due to the fact that they are carried out by making small incremental steps, all of which are reversible.

The direction in which a thermodynamic process will spontaneously occur is determined by a quantity called entropy

49
Q

What happens when an irreversible process occurs within an isolated system?

A

If an irreversible process occurs within an isolated system, the entropy S of the system increases.

50
Q

What is the formula for entropy change?

A

∆S = Sf − Si = f∫i (dQ / T)

51
Q

What is the formula for infinitesimal entropy change?

A

dS = dQ/T

52
Q

Second Law of Thermodynamics and Entropy

A

The second law of thermodynamics: In an isolated system, the entropy cannot decrease. More specifically, if a process occurs in an isolated system, the entropy change of the system will be zero if the process is reversible, and will be greater than zero if irreversible.

In equation form the second law of thermodynamics states: for an isolated system undergoing some process the entropy change ∆S of the system is ∆S ≥ 0. Here the greater-than sign applies if the process is irreversible and the equal sign applies if the process is reversible.

Entropy may decrease for a system provided it is not isolated.

53
Q

Define Entropy

A

Entropy can be understood in a number of different ways which are closely related to one another: it can be thought of as a measure of the disorder of a system; or as a measure of how likely it is that a system will be in its current state; or as how much useful work a
system has to offer. The greater the entropy a system has, the more disordered the system is and the more probable its current state is.