Exam 2 Flashcards

(69 cards)

1
Q

4 postulates of Kinetic theory of gases

A
  1. Gas consists of a large number of identical molecules separated by distances that are great compared to their size
  2. Gas molecules are constantly moving in random directions with a distribution of speeds
  3. Molecules can collide with each other (bounce off each other with no loss of kinetic energy) but exert no forces on one another between collisions
  4. The collisions of molecules with the walls of the container are also elastic (no loss of kinetic energy)
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1
Q

Kinetic theory of gases

A

a model for molecular motion that predicts the properties of gases, particularly the relationship between temperature and the distribution of molecular speeds

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2
Q

Maxwell-Boltzmann plot (with constant molecule mass but varying temperature)

A

-Low temperature will have higher peak, more condensed shape, and lower average speed (closer to 0)
-Higher temperature will have lower peak, more spread out shape, and higher average speed (farther from 0)

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3
Q

Maxwell-Boltzmann plot (with constant temperature but varying molecule mass)

A

-Higher molecular mass will have higher peak, more condensed shape, and lower average speed (closer to 0)
-Lower molecular mass will have lower peak, more spread out shape, and higher average speed (farther from 0)

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4
Q

<V> (mean speed
</V>

A

-<V> = √8kBT/πm or √8RT/πm
-Will always be greater than most probable speed, as area under the curve to the right is somewhat larger than the area under the curve to the left
-<v> = (1.128)(Vmp)</v></V>

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5
Q

mean square speed

A

-<v^2> = √3kBT/m
-Directly related to KE (½mv^2)

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6
Q

Vmp (most probable speed)

A

-Vmp = √2kBT/m or √2RT/m
-Found at the peak of the graph
-will always be less than <v></v>

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7
Q

Area under Maxwell-Boltzmann plot

A

-Total area always equals 1 (100% of molecules)
-To find fraction of molecules under graph with given range of speeds, find number of molecules at max of range and min of range and take max - min
-Act like the max of graph=1 and add max y to min y value then times by percentage of graph x values take up

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8
Q

Total kinetic energy (monatomic gas)

A

-KE(total translational) = 3/2nRT
-KE total also equals = N<KE>
-Total kinetic energy increases linearly with temperature, depends on both temperature and number of molecules in sample</KE>

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9
Q

Average translational kinetic energy (for a single gas molecule)

A

-<KE> = 3/2 kT
-Average kinetic energy is the same for all molecules at a given temperature (depends only on temperature)
-increases linearly with temperature</KE>

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10
Q

Thermodynamics

A

-concerned with macroscopic properties of systems and changes in these properties during processes
-Study of the interconversion, transfer, and dispersal of energy among its various forms

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11
Q

Thermodynamic system

A

-a real or imagined portion of the universe that is confined by boundaries or mathematical constraints

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12
Q

Open system

A

both matter and energy may be freely exchanged with the surroundings

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13
Q

Closed system

A

does not gain or lose matter during a process because it is surrounded by impermeable walls

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14
Q

Isolated system

A

system which is surrounded by walls that prevent it from exchanging energy or matter with its surroundings

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15
Q

State function

A

-a property of a system that is uniquely determined by the present state of a system and not at all by its history
-Volume temperature, pressure, and internal energy (U) are examples of state functions
-the value of ΔU (or ΔV or ΔT) depends only on the initial and final states of the system, not the path by which the process got the system from initial to final

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16
Q

Path function

A

-a property of a system that is uniquely determined by the specific path taken to transition from initial to final states, rather than just the state itself
-Work and heat are path functions
-Path-dependent, values vary depending on how the process occurs not just the initial and final states

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17
Q

First law of thermodynamics

A

-in any process, energy can be changed from one form to another (eg potential to kinetic) and energy can be transferred from one object to another (as heat or work), but energy is never created or destroyed
-Law of conservation of Energy
-If energy change is caused by mechanical contact of system with its surroundings, work is done
-If energy change is caused by thermal contact, heat is transferred

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18
Q

Internal energy (U)

A

-the sum of internal kinetic energy and potential energies of the particles composing a system
-Any mechanical or electrical work done on a system can change its internal energy (unless heat is transferred out of system to compensate)
-For idea monatomic gases, U = KE (3/2nRT)
-ΔU = 3/2nRΔT
-ΔU = q + w

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19
Q

Work (w)

A

-the product of the external force F acting on a body and its displacement d
-W > 0, work is done on system by the surroundings
-W < 0, work is done by system onto surroundings

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20
Q

Pressure-Volume work

A

-results when system is compressed or expanded under influence of outside pressure
-w = -PextΔV
-For expansion, ΔV > 0 , and work is being done by system
-For compression, ΔV < 0, and work is being done by surroundings
-Can be reversible or irreversible

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21
Q

Isothermal reversible gas expansion/compression

A

-internal pressure is nearly equal to the external pressure and expansion/compression is slow
-w(rev exp) = -nRTln(V2/V1)
-w(rev comp) = -nRTln(V1/V2)
-Most efficient, maximum work is done

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22
Q

Irreversible process

A

-a process that does not proceed through a series of equilibrium states and cannot be reversed by an infinitesimal change in an external force
-Rapid and uncontrolled
-Cannot be represented by path
-Pext is constant and often lower/higher than internal (depending on if expansion/compression)

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23
Q

Reversible process

A

-a process that proceeds through a series of equilibrium states, and can be reversed by an infinitesimal change in external force
-Pint and Pext are nearly equal
-maximum possible work is done by gas
-Follows well-defined path

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24
Heat (q)
-energy is transferred from a hot body to a colder body when the two are placed in thermal contact with one another -Means of increasing the internal energy of a system without mechanical interaction -q at constant volume, (qv) = ΔU (ΔV = 0, w=0) -q at constant pressure, (qp) = ΔU - w -(or qv - w)
25
Bomb calorimetry
-methods for measuring quantitatively the amount of heat transferred into or out of a thermodynamic system in a process -ΔU = qv -Heat of reaction under constant volume -Surroundings consists of insulated walls, water, thermometer, and sparker (initiates reaction) -System consists of chemical reaction (combustion due to O2) -Heat capacity of calorimeter, C, is the amount of heat required to raise the temperature of the calorimeter by 1 C/K
26
Adiabatic process
-no heat is allowed to flow in/out of system due to insulated walls -q = 0 -ΔU = w
27
Heat capacity (C)
-the quantity of heat required to raise its temperature by 1 K (or C) -Depends on the quantity of the substance that is being heated (extensive property) -If mass increases, heat capacity increases -C = q/ΔT
28
Specific heat capacity (Cs)
-quantity of heat required to raise one gram of a substance by 1 K -Intensive property, does not depend on mass -Specific heat capacity is same for two samples of same compound regardless of difference in mass -Specific heat capacity of water is 4.184 J/gK -Metals get hot/cool really easily (Cs), while water requires a lot of thermal energy to change temp (high Cs) -Cs = q/mΔT or q = mCsΔT
29
Molar heat capacity (Cm)
-the quantity of heat required to raise the temperature of one mole of substance by 1 K -q = nCmΔT or Cm = q/nΔT
30
Molar heat capacity at constant volume (Cv)
-amount of heat required to increase the temperature of 1 mol of substance by 1 K at constant volume -qv = nCvΔT -Cv = 3/2R -qv = ΔU, ΔU = nCvΔT -For polyatomic gases, Cv is greater than 3/2R because energy is stored in different kinetic energy (rotational/vibrational)
31
Molar heat capacity at constant pressure (Cp)
-amount of heat required to increase the temperature of 1 mol of substance by 1 K at constant pressure -qp = nCpΔT -Cp = 5/2R -Cp = Cv + R (always greater than Cv) -ΔH = qp, ΔH = nCpΔT -qp = ΔU - w; qp = qv - w
32
Enthalpy (H)
-a function of state, defined as H = U + PV, for changes carried out at constant internal pressure, the enthalpy change of the system is equal to the heat absorbed -H = U + PV -Heat of reaction under constant pressure -Helps determine how much useful energy is contained in any chemical compound -Absolute enthalpy, H, cannot be measured, only changes in enthalpy, ΔH -Extensive property, dependent on the amount of substance present in the sample
33
Change in enthalpy (ΔH)
-ΔH = ΔU + ΔPV or ΔH = ΔU + nRΔT -ΔH=qp -Change in enthalpy is equal to heat gained/lost by system -When reaction takes place, enthalpy changes and heat is transferred into or out of system
34
Standard enthalpy of reaction (ΔH°rx)
-enthalpy change for a chemical reaction in which all reactants/products are in their standard states (1 atm, 1 M, 298 K) -ΔH°rx= ΣnpH°f(prod) - ΣnrH°f(react) -Measures heat absorbed/released in a reaction
35
Exothermic
-a reaction in which heat if given off -ΔH < 0 (negative) -ΔS > 0 (positive), -ΔG < 0 (negative)
36
Endothermic
-a reaction in which heat is taken up -ΔH > 0 (positive) -ΔS < 0 (negative), -ΔG > 0 (positive)
37
Standard enthalpy of formation (ΔH°f)
-the enthalpy change for the reaction that produces one mole of a compound in its standard states from its element, also in their standard state -Enthalpy change when 1 mole of a compound is formed from its elements in their standard states -Elements in their most stable form at 298 K have ΔH°f = 0 (O2, N2, C) -Usually given, measures stability of a compound -Used to calculate ΔH°rx
38
Hess’s law
-if two or more chemical equations are combined by addition or subtraction to give another equation, then adding or subtracting changes in enthalpies for these equations in the same way gives the enthalpy change associated with the resultant equation -Derives from the fact that enthalpy is a state function (only depends on initial and final states)
39
Standard Molar Bond Enthalpy (ΔH°b)
-the average molar enthalpy change in accompanying the dissociation (breaking) of a given kind of bond in the gas phase -For gas-phase reactions: -ΔH°rx = ΣΔH°b(reactants) - ΣΔH°b(products)
40
Standard Molar Atomization Enthalpy (ΔH°a)
-the enthalpy change associated with atomizing an element from its most stable form to a mole of gaseous atoms -For any gas-phase compound (atomizing element): -ΔH°f = ΣΔH°a(elements) - ΣΔH°b(compound)
41
Kirchhoff’s law
-describes how enthalpy change of a reaction (ΔH°rx) varies with temperature -ΔH°(T2) = ΔH°(T1) + ΔCp(T2 - T1) --ΔCp = ΣnpCp(prod) - ΣnrCp(react) --H° = nCpΔT, ΔH° = nΔCpΔT
42
Enthalpy of fusion
-the heat required to convert a substance from a solid to a liquid at its melting point -On heating curve, it is area where slope=0
43
Enthalpy of vaporization
the heart required to convert a substance from a liquid to a gas at its boiling point
44
Enthalpy of sublimation
the heat required to convert a substance directly from a solid to a gas
45
Second law of thermodynamics
-in any spontaneous process, there is always an increase in the entropy (disorder) of the universe
46
Entropy (S)
-measure of molecular randomness -thermodynamic state function that describe the total number of “microstates” that are available to a system -Processes that tend to increase entropy have a much higher probability of happening -Helps us predict how much useful work can be extracted from a reaction -Related to heat flow (flow of heat between systems increases entropy, when two objects are different temps, it is orderly arrangement. Transfer of heat causes disorder and higher entropy)
47
Microstate
-all the possible ways in which atoms can be placed into different energy levels -The more microstates there are for a given state, the greater probability for that state existing -Nature spontaneously proceeds towards the state with the highest probability (the most microstates/the highest increase in entropy) -States in which gas atoms are evenly distributed has the greatest number of microstates and the greatest probability -Number of microstates = volume ratio ^ number of particles
48
Boltzmann’s equation
-S = KblnΩ --Where Ω is number of microstates and Kb is boltzmann’s number (R/Na)
49
ΔS for an expanded gas (isothermal expansion)
-ΔS= nRln(V2/V1) -Or qrev/T (where qrev = -wrev = nRTln(V2/V1) -Gas expansion is reversible if Pint = Pext at every point -Change in volume leads to a greater disorder in arrangement of gas molecules (no change in temp)
50
ΔS for a heated gas
-ΔS= nCpln(T2/T1) -Where Cp = 5/2R -Temperature increase causes greater disorder
51
ΔS for constant volume
-ΔS= nCvln(T2/T1) --Where Cv = 3/2R -No change means no work is done by gas -Temperature change leads to increase in entropy (increase in temp leads to positive ΔS (greater entropy), while decrease in temp leads to negative ΔS (lesser entropy)
52
ΔS for constant pressure (isobaric process)
-ΔS= nCpln(T2/T1) -Work is done either by gas or by surroundings -Gas is heated/cooled at constant pressure, meaning volume changes. -Change in temperature lead to entropy change (volume changes in response to temperature change but still somewhat contributes)
53
ΔS for phase change
ΔS = ΔH(fus/vap) / T
54
Third law of thermodynamics
-the entropy of any pure substance (element/compound) in its perfectly ordered crystalline state at absolute zero is 0 -Perfect ordering is caused by distribution of charge (polar) throughout molecule, resulting in symmetrical alignment and no entropy -When absolute zero is reached, all energy associated with atomic motion has left crystal and atoms are perfectly still (O K) -When molecules lack distribution of polarity, it leads to lack of symmetrical alignment and no perfect crystal lattice (residual entropy)
55
residual entropy
when cooled to absolute zero, compound does not have 0 entropy
56
Standard molar entropy (S°
-the entropy of one mole of a substance in its standard state at 298 K and 1 atm -Molar entropy at different temperatures: -ΔS°(T2) = ΔS°(T1) + ΔCpln(T2 - T1) --ΔCp = ΣnpCp(prod) - ΣnrCp(react)
57
Standard molar entropy of reaction (ΔS°rx)
-change in entropy when reactants are converted to products under standard conditions (298 K, 1 atm) -ΔS°rx = ΣnpS°(prod) - ΣnrS°(react)
58
Entropy of the universe
-ΔS(univ) = ΔS(sys) + ΔS(surr) -ΔS(surr) = q(rev) / T -q(rev) = -w(rev) -If ΔS(univ) > 0, then forward process is spontaneous -If ΔS(univ) < 0, then backward process is spontaneous -If ΔS(univ) = 0, the system is at equilibrium
59
ΔS(univ) for a isothermal gas expansion
-S(sys) = nRln(V2/V1) -S(surr) = q(rev)/T -S(univ) = S(sys) + S(surr)
60
ΔS(univ) for cooling of hot body
-S(sys) = nCpln(T2/T1) -S(surr) = q(surr)/T -q(surr) = nCp(T2-T1) -S(surr) = q(surr)/T = -ΔH(sys)/T
61
Gibbs free energy (G)
-allows us to determine direction of spontaneous process (under constant T and P) without explicitly calculating ΔS(univ) -If ΔG < 0, then forward process is spontaneous -If ΔG > 0, then backward process is spontaneous -If ΔG = 0, the system is at equilibrium
62
H(sys)
-ΔH(Sys) = q(sys) (under constant P) q(surr) = -q(sys) = - ΔH(Sys) -ΔS(univ) = ΔS(sys) + ΔS(surr) = ΔS(sys) - -ΔH(sys)/T
63
Change in free energy (ΔG)
-indicates the spontaneity of a process or reaction -ΔG = ΔH - TΔS
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Spontaneous process
not requiring an outside source of energy to proceed
65
Standard free energy of formation, ΔG°f
-change in free energy when one mole of a compound is formed from its elements in their most stable form at standard conditions (298 K, 1 atm) -ΔG°f = ΔH°f - TΔS°f
66
Standard free energy of formation, ΔG°rx
-the free energy change for the reaction that produces one mole of its compounds in their most stable forms under standard state conditions (298 K, 1 atm) -ΔG°rx = ΣnpΔG°f(prod) - ΣnrΔG°f(react)
67
Calculating ΔG°rx with ΔH°’s and ΔS°’s
-ΔG°rx = ΔH°rx - TΔS°rx -Calculate individual ΔH°rx and ΔS°rx
68
When all products/reactants are in standard state
-Q=1 -T(eq) = ΔH°/ΔS°