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States/Phases of matter:
There are three common states of matter: solid, liquid, and gas. (Plasma is another state of matter but is beyond this discussion.)
Libretexts has this excellent material on it: https://chem.libretexts.org/Courses/Bellarmine_University/BU%3A_Chem_104_(Christianson)/Phase_1%3A_The_Phases_of_Matter
A solid will maintain its shape (ice, wax, steel), while a liquid will flow and take the shape of its container (water, mercury). A gas or vapor will fill all available volume (steam, air, mercury). There is a 4th state which is plasma, also known as ionized gas state. It's a gas state where atoms lose their electrons in presence of very high electromagnetic field, which causes these electrons to start conducting electricity, which isn't typical of gases. In nature, lightning is the most common example of plasma. It's the most common state in the universe, since all stars are in plasma state. However, in real life we don't encounter this state, so we don't discuss the plasma state.
States of matter are generally based on the form of the substance at room temperature and pressure. Things like air are gaseous at room temperature while water is a liquid. When heated, water become gaseous, but is referred to as a vapor. At atmospheric temperature (25C) and pressure (1.0 atm), most of the elements are found in solid state. Mercury (Hg) and Bromine (Br) are the only 2 elements found in liquid state. All noble gases and H, N, O, F and Cl are the only ones found in gaseous state.
For Pressure details, see "Force, work, energy" section under Physics.
GASES:
Maxwell-Boltzmann distribution (MBD): Maxwell-Boltzmann (MB) distribution gives the distribution of speed of gas particles. It's derived from MB statistics (MBS) which s the more general case. MBD is a special case of MBS. MBD was found first by Maxwell in 1860, and then proved formally in 1870 by Boltzmann.
Link for MB statistics (not distribution) => https://en.wikipedia.org/wiki/Maxwell%E2%80%93Boltzmann_statistics
MBS describes the distribution of classical material particles over various energy states in thermal equilibrium. It states that # of particles, Ni with energy εi is:
where total # of particles N = Σ Ni and
Basically what MBS is trying is getting the fraction of particles in a particular energy state (the numerator and denominator with T term in the exponents) and then multiplying by N to get total particles. Let's see if it makes sense. At 0K (absolute 0 temperature), the number of particles in any energy state is 0. This makes sense as at 0K, there are no energy states besides the ground energy state, and all particles are in that energy state. As Temp inc, the number of particles in higher energy states begin to inc.
MBD is a probability dist func of particles with a particular speed and applies to ideal gas. We can derive MBD from MBS by observing that εi is the kinetic energy of that particle = 1/2*m*v^2, and then doing some manipulation.
Therefore, the Maxwell–Boltzmann speed distribution (i.e MBD) is :
where m=mass of particle
The above eqn is of the form x*e-x. It starts from 0 at x-=0 and goes to 0 at x=infinity. It's not a gaussian distribution as it's not symmetric. It's a chi distribution.
If we find RMS velocity of all particles, it's V = √ (v1^2 + v2^2 + ...). We use func above to find # of gas particles having speed b/w v and dv. We then integrate it as v^2*f(v)*dv, which leads to
Vrms = √ (3*kb *T)/m = √ (3*R *T)/M = Where M is molecular mass and R = kb * Na (universal gas constant explained below)
Vrms of diatomic N2 gas at 300K = sq rt[ 3*1.38*10^-23*300/(1.67*(10^-27)*28)] = 515m/s. Total KE of each particle = 1/2*m*(Vrms)^2. = 3/2*kb *T. What this implies is that KE of any gas is the same for a given temp (doesn't depend on anything except Temp).
From above eqn, Vrms is higher for lighter gas, and lower for heavier gases. With pdf plotted on Y axis and rms velocity plotted on x axis, pdf curve's peak has to be at lower velocity for heavier gases. However total kinetic energy of any gas is dependent only on Temp. Since RMS velocity became lower for heavier gases, more particles will need to within the vicinity of the peak to keep energy same (i.e area under the curve can't change). This causes the curve to start shifting right for lighter gases (i.e curve starts flattening for lighter gases).
Total energy of 1 mole of gas = 1/2* (3*kb *T) * Na = 3/2*R*T. This is the most known eqn that KE of any gas at any Temp is 3/2*R*T (which is only dependent on Temperature and nothing else). This can also be seen from the observation that for a given thermodynamic system at temp T, the average thermal energy carried by each microscopic degree of freedom in the system is 1/2 kT (i.e., about 2.07×10−21 J, or 0.013 eV, at room temperature). Since particles in 3D have 3 degrees of freedom, each particle has 3/2 kT of energy. For 1 mole of particles, energy = 3/2kT*Na = 3/2RT = 3/2*8.3 J⋅K−1⋅mol−1 =* 300K * 1mole = 3735 J = 3.7KJ.
Internal Energy (U) and degrees of freedom: Internal energy of a gas includes not only translational energy due to motion of particles, but also rotational energy (molecules spinning) and vibrational energy (molecules vibrating). All of these energy contribute to KE. On top of KE, we may also have PE resulting from proximity of particles. Combing both of these (KE+PE), we get Internal Energy (U) of the particle. What all motion (translational, rotational or vibrational) any molecule has is determined by it's degree of freedom.
Degree of freedom is the number of variables required to describe the motion of a particle completely. For any molecule with n atoms, each molecule has 3 degrees of freedom as the molecule is free to move in any of 3 dimensions. For n atoms in the molecule and assuming each atom within the molecule can also move independently in 3 dimensions, it will have a total of 3*n degrees of freedom. For ex, He gas will have 3 degrees of freedom, while N2 gas will have 3*2=6 degrees of freedom.
However, all atoms within molecule are not free to move in any motion as these atoms are bonded together. So, all motions are not translational; some become rotational, some others vibration. For non-linear molecules, all rotational motions can be described in terms of rotations around 3 axes, the rotational degree of freedom is 3 and the remaining 3N-6 degrees of freedom constitute vibrational motion. For a linear molecule however, rotation around its own axis is no rotation because it leave the molecule unchanged. So there are only 2 rotational degrees of freedom for any linear molecule leaving 3N-5 degrees of freedom for vibration. And to complicate matters, the degrees of freedom changes with Temp too !!
This link has few videos to explain => https://openbooks.library.umass.edu/toggerson-131/chapter/energy-associated-with-motion-at-the-molecular-scale-temperature-and-thermal-energy/
Each degree of freedom has 1/2RT of energy. For monoatomic gas such as Helium, atoms have translational energy only. So, total energy is 3/2RT. For diatomic gases such as Nitrogen gas (N2) , on top of translational energy, we have rotational energy of RT due to 2 degrees of motion, while vibrational energy is almost zero. So, Total internal Energy U of N2 gas is 5/2RT. For other molecules, we have vibrational energy too, which may contribute to total energy.
U in solids, liquids and gases: In gases, calculating total energy was easy as gas molecules only had KE (no PE as molecules don't interact with each other due to large distances), and hence their energies can be calculated in isolation. Any molecule whether in solid, liquid or gas form has KE in all forms, it's just that contribution from translation, rotational and vibrational motion changes, which changes total KE too. Gas form has the highest U and is mostly from KE due to translational energy (as particles are far apart, no interaction b/w particles, so potential energy negligible). U is lower than gas as there's limited translational motion, but at same time PE is higher as particles are closer. Solids have the lowest U as particles are fixed in place, so only KE is from vibration of particles. However PE is highest as particles are closest together. At absolute 0K, KE of particles go down to 0, but still have some residual PE known as zero point energy.
Latent heat during phase change: As a liquid changes to gas form, it takes in latent heat at it's boiling point, which doesn't inc the temperature. All of this latent heat goes into the liquid in increasing PE as particle distance increases. ,
PE change: PE at infinity is taken as 0. If +ve particles come closer together, then we have to apply energy to bring them closer, so their PE has to inc (since our work done gets stored as PE). If -ve particles come closer together, then they release energy as they come closer closer, so their PE has to dec (since we have to do -ve work which gets stored as PE). PE decreases as neutral particles come closer, as there are attractive forces b/w neutral particles (They behave as opposite charged particles or have attractive forces due to Van der waals (see below) in solid, liquid states). However, beyond a certain proximity, when particles get too close, then repulsive forces start dominating and PE starts to inc rapidly. We are talking about distances in solids/liquids where these attractive forces exist, so we can treat different particles as having opposite charges.
This is the reason, why applying heat changes from solid to liquid to gas => The internal energy increases which changes the state. Specific heat of any material in the 3 states, gives us the amount of internal energy of any molecule.
Ex: Internal energy of Water calculated from specific heat:
- Solid water (Ice) => specific heat = 36J/mole-K. So, at 0C (273K), Internal energy of ice = 36*273 = 9.8 KJ/mole.
- Latent heat from ice to water => 6KJ/mole. 100X more than specific heat of ice.
- liquid water (water) => specific heat = 75J/mole-K. So, at 27C (300K), Internal energy of water = 75*300 = 22.6 KJ/mole.
- Latent heat from ice to water => 44KJ/mole. 500X more than specific heat of water.
- gas water (vapor) => specific heat = 34J/mole-K. So, at 100C (373K), Internal energy of vapor = 34*373 = 12.7 KJ/mole.
Ex: Thermal energy of Noble gas Helium, which doesn't form any bonds with any other atoms.
- Solid He => specific heat = 2J/mole-K. He becomes solid only at very high pressure and Temp of 1K. So, at 1K, Internal energy of solid He = 1*2 = 2 J/mole.
- liquid He => specific heat = 20J/mole-K. He becomes liquid at 4K (at atm pressure). So, at 4K, Internal energy of liquid He = 20*4 = 80 J/mole.
- gas He => specific heat = 20J/mole-K (or 20J/4g=5J/g-K). So, at 27C (300K), Internal energy of gas = 20*300 = 6 KJ/mole. From internal energy eqn, we get 3/2nRT = 4.7KJ/mole which is not too far.
Internal Energy vs atomic energy: This internal energy that we have been talking about is the thermal energy, This is energy for collection of atoms gaining energy due to heat. Other energy that we have within atome is in formation of atom itself => energy needed for formation of nucleus (nuclear energy) + energy needed for getting 2 electrons in it's orbit (Ionization energy or IE). IE for He is 7.6MJ (1000x more than U of He), while nuclear energy is 2.7BJ (1000x more than IE). These energies are also dependent on Temp? FIXME ?
Ideal gas law: This provides a relation between P, V, T of an ideal gas (ideal gas is one with no interaction among gas particles and assuming gas particles having zero size) with the number of gas molecules for an ideal gas. There were multiple laws discovered by various scientists, but they were all combined into one once "Ideal gas law" was found. Link: https://en.wikipedia.org/wiki/Ideal_gas_law
The law states that
P*V = n*R*T => where P,V,T are pressure (in pascal), Volume (in m^3), Temperature (in Kelvin) of gas and n=amount of gas particles (in moles), R= universal gas constant = (boltzmann constant) *
(Avagadro constant) = 1.380×10−23 J⋅K−1 * 6.022×1023 mol-1 = 8.3 J⋅K−1⋅mol−1 . Here R represents energy in 1 mole of gas particles per unit temp.
The equation above is written in many different forms. The one above is the molar form. Under STP (T=273K, P=atmospheric pressure = 1 bar = 101kPascal), 1 mole of gas occupies V=nRT/P = 8.3*273/(101*10^3) m^3 = 0.0224 m^3 = 22.4 L (since 1L=1000 cm^3 = 1/1000 m^3). So, 1 mole of any ideal gas is always 22.4L in volume under STP. What is very surprising is that no matter what gas it is, it always occupies the same volume under same conditions of P, T. Whether the gas is water or oxygen or complex compound, they all occupy 22.4L for 1 mole of gas under STP. This doesn't seem intuitive, as one might expect gases to have different forces, size, etc and hence occupy diff volumes.
Derivation: Ideal gas law is easy to derive. See wiki link above. Simple proof:
Consider a container of Volume V with N gas particles moving with rms velocity v. Assuming random movement is equally likely in all 3 directions, x,y and z, 1/3 of the particles move in x direction (1/6 th move in +X, while 1/6 th move in -X dirn), strike against the container wall of Area S, and bounce back with reverse velocity v. Momentum change = 2mv for each particle, Force due to each particle=Momentum change/t = 2mv/t. For "q" particles hitting in time t, F=2mv/t*q. In time t, volume of particles striking the wall are = v*t*S. If there are N particles in Volume V, then number of particles in Volume v*t*S = v*t*S*N/V. But only 1/6th are striking. So, number of particles striking wall in time t = v*t*S*N/V *1/6. This is "q". So, P=F/S = 2mv/t*q*1/S = 2mv/(tS)*1/6*v*t*S*N/V=1/3m*v^2*N/V. So, PV=1/3Nmv^2
Using Maxwell-Boltzmann distribution above, ,we found rms velocity (v^2) which comes out to 3k*T/m. So, PV=1/3N*m*3kT/m=NkT => PV=NkT. This is the molecular formula of ideal gas law. If we take n moles of gas, then PV=n*NA*kT => PV=nRT
Deviation from ideal gases: Real gases follow ideal gas laws only at low pressure and at high temperatures. This happens because at low pressure molecular volume of gases is still negligible compared to volume of container. Also, intermolecular forces are low amongst the particles. The same thing happens at high temp, where particles are able to break the intermolecular forces and don't interact with each other. Van der waals eqn which has experimentally determined constants a,b corrects the ideal gas law to incorporate it for real gases. Plots are shown in link above (section 1.7). When very high pressure or low temps are applied, gases change state to liquid, which is an extreme case, where intermolecular forces are very high, and KE is not enough to break them apart.
Dalton's Law o partial pressure: It states that total pressure of a mixture of ideal gases is equal to the sum of the partial pressures of the component gases. i.e if 2 gases are in their own containers with pressure P1 and P2, then, they are both put in the same size container, then total Pressure = P1+P2, as long as the gases don't react with each other. It seems counter intuitive, as we would expect presence of other gas to affect pressure of 1st gas compared to when it was by itself. Apparently that doesn't happen. Reason is that collisions are elastic, so presence of any amount of gas particles doesn't affect the energy of our gas particles (it's only dependent on Temperature), so energies of all gas particles can just be added up.
Phase changes: When a substance changes from one state of matter to another, it experiences a phase change. For instance, ice melting into water is a phase change from solid to liquid. Water changing into steam is a phase change from liquid to vapor. Energy in the form of heat is required to create a phase change. The elements in periodic table change state, as well as the compounds formed from them. Infact most matter made up of any number of compounds has to exist in all of the 3 states. It's just that at room temperature and pressure, it exists in one of the 3 states. But by changing temp and pressure, it can be converted to other states too.
Section 3 from above link (dedicated to phase changes only) => https://chem.libretexts.org/Courses/Bellarmine_University/BU%3A_Chem_104_(Christianson)/Phase_1%3A_The_Phases_of_Matter/3%3A_Phase_Changes
Intermolecular Bonds:
Intermolecular forces (IMF) are forces that exist between molecules. They are much weaker than intramolecular bonds which are atomic bonds (explained under atomic bonds). IMF are important because they determine the physical properties of molecules like their boiling point, melting point, density, and enthalpies of fusion and vaporization. IMF are called weak bonds, while atomic bonds are called strong bonds. The force within a molecule to break the bonds is lot higher at 430 KJ/mole, while IMF is lot lower at 17KJ/mole (for conversion from gas to liquid) for HCl. So, these IMF are lot easier to break, and hence change phases. The phase in which a substance exists depends on the relative extents of its intermolecular forces (IMFs) and the kinetic energies (KE) of its molecules.
Intermolecular forces: https://chem.libretexts.org/Bookshelves/General_Chemistry/Map%3A_Chemistry_-_The_Central_Science_(Brown_et_al.)/11%3A_Liquids_and_Intermolecular_Forces/11.02%3A_Intermolecular_Forces
All of these attractive IMF are also called "Van der Waals" forces, after the name of the scientist who found these. There are 3 kinds of van der waals forces.
- Dipole-Dipole attraction: Polar molecules such as HCl have +ve charge on one side and -ve charge on other side resulting in a dipole. An attractive force between HCl molecules results from the attraction between the positive end of one HCl molecule and the negative end of another. This attractive force is called a dipole-dipole attraction.
- Effect of dipole dipole attraction is apparent when we compare Fluroride gas with HCl. Both have same molecular mass, but polar nature of HCl causes the molecules to stick together, while F2 molecules being non polar don't have this attractive force. As a result, HCl becomes gas at 188K,, compared to F2 molecules which boil at much lower temp of 85K.
- London dispersion forces : These forces are present in all matter. London dispersion forces are weak attractions between molecules. They can occur between atoms or molecules of any kind, and they depend on temporary imbalances in electron distribution. This causes formation of temporary dipoles, resulting in electrostatic attraction b/w molecules. Being very weak, they become significant only when the molecules are very close. Larger and heavier atoms and molecules exhibit stronger dispersion forces than do smaller and lighter atoms and molecules. In a larger atom, the valence electrons are, on average, farther from the nuclei than in a smaller atom. Thus, they are less tightly held and can more easily form the temporary dipoles that produce the attraction. The shapes of molecules also affect the magnitudes of the dispersion forces between them. Compact shapes provide less surface area and hence less force, while elongated shapes provide a greater surface area available for contact between molecules, resulting in correspondingly stronger dispersion forces.
- Melting and boiling point trend in periodic table:
- Hydrogen Bond: This is a a bond that is usually b/w +ve charged H atom and another -ve charged atom. This bond forms due to EN diff b/w the 2 diff atoms that form the molecule. Water is one of the ex of H bond. Even though they are called, they are not real bonds.
- In general, these are the requirements for a H bond:
- A polar covalent bond needs to exist b/w H atom and a highly EN atom as N(2p3), O(2p4), and F(2p5), These are the only 3 that have large EN difference to form a highly polar bond.
- There should be at least one active lone pair of electrons available in highly EN atom. Lone pairs at the 2-level have electrons contained in a relatively small volume of space, resulting in a high negative charge density.
- Once these 2 conditions are satisfied, a bond starts forming b/w lone pair of electrons in 1 molecule which is highly EN with highly positive hydrogen atoms of another molecule. This bond has 1/10 the strength of an avg covalent bond, so it is strong enough to change properties of that molecule.
- NH3, H2O and HF are 3 examples of compounds which form strong enough H bonds that their boiling points are lot higher, compared to what is expected in the absence of H bond.
- Water is the perfect ex of how H bond causes higher boiling pt. There are 2 pair of lone electrons available on Oxygen to form 2 H bonds with neighboring Hydrogen atoms of another molecule. Even though H2O has covalent bonds and hydrogen and oxygen atoms share their electrons, they end up developing a polarity due to higher electronegativity of oxygen compared to hydrogen. Oxygen ends up getting a slightly negative charge, while hydrogen a slightly positive charge. This allows different molecules of H2O to form a lattice structure with -ve polarity of oxygen of 1 molecule forming polar bonds with +ve polarity of hydrogen atoms of another molecule. These bonds are called Hydrogen bonds (and NOT polar bonds). When temperature are low, the vibrational energy of each molecule is very low, and not enough to break these hydrogen bonds between hydrogen and oxygen of different molecules. This makes it a solid, where the molecules can't slide past each other. But as temperature rises, the vibrational energy of each molecule increases, causing these hydrogen bonds to get weaker to a point where the molecules can slide past each other. This forms a liquid. If we keep on increasing the temperature, these hydrogen bonds break completely free, and different molecules become independent of each other. This forms the vapor or gas state. This video from Khan Academy explains it => https://www.khanacademy.org/science/chemistry/states-of-matter-and-intermolecular-forces/states-of-matter/v/states-of-matter
- In general, these are the requirements for a H bond:
Liquid -> Gas (phase change): Just like we have distribution of gas particles with different speed/energy (as per Maxwell-Boltzmann distribution), the same law applies to liquid particles too. Some liquid particles will have higher kinetic energy than others. Ones which exceed the energy needed to break off the liquid surface (and near the surface traveling upward) will leave the liquid surface and become gas. This is called evaporation. If this gas is allowed to escape, then avg energy of liquid particles will drop (dropping the temp). This will force absorption of heat from surroundings, which will maintain the avg speed of molecules in liquid. Over time, all liquid will evaporate. However, if the liquid is kept in closed container, then evaporation will stop after some liquid has evaporated. This is due to the fact that vapors that form above the liquid start exerting a pressure, and will start getting recaptured at the surface (i.e condense into liquid state again). The 2 rates => rate of evaporation and rate of condensation balance each other out. The pressure of vapor at which this happens is called "vapor pressure" and is constant for a given liquid at a given temperature (irrespective of it's volume). Vapor pressure of water at 25C is 24mm Hg (3 kPa).
The magnitude of the vapor pressure of a liquid depends mainly on two factors: the strength of the forces holding the molecules together and the temperature. Lower the intermolecular forces, easier for molecules to escape as vapor, and hence higher the vapor pressure. Also, as Temp inc, more molecules have higher energy and can get to vapor state, and hence higher vapor pressure.
Boiling point: Boiling pt is related to the vapor pressure. We saw above that Vapor pressure of water at 25C is 24mm Hg (3 kPa). At this temp, water converts to gas only at surface (not thru out the liquid). This process is called evaporation and heat needed for this is called "latent heat of evaporation". If we keep increasing temp to increase the vapor preesure, then at some temp, the vapor pressure will exceed the atmospheric pressure. As soon as this happens, water will start forming bubbles even deep within the liquid, indicating the bonds have been broken inside the liquid too. These bubbles will come to surface and escape.
and those bubbles. Let's say we removed the walls of the closed container and replaced it with air pressure of 24mm Hg. Then the situation is still the same as that of a closed container. Now, we slightly decrease the air pressure. Then vapor molecules will start moving from high pressure to low pressure, creating a pressure lower than vapor pressure near the water surface. This will cause more water to evaporate as it needs to maintain the vapor pressure. This process will continue indefinitely, resulting in creation of bubbles in the liquid, which are actually vapors at vapor pressure. These will keep escaping, until all the liquid has escaped as vapor. This vigorous process is called boiling and the temperature at which it happens is called "boling point" at that air pressure. For our definition, we define "Boiling point" as temp at which vapor pressure equals atmospheric pressure. At 100C, vapor pressure of water is 1 atm, so that is our boiling pt for water (at atm pressure).
Vapor pressure Vs Temp graph shows non linear relation, but do show that as Temp inc, Vapor pressure inc. So, at lower atm pressure, vapor pressure equals atm pressure at lower temp, and so liquids boil at lower temp, when atm pressure is reduced.
Melting point: Just as boiling pt is defined, melting pt is defined as Temp where solid to liquid conversion happens.
Phase change graph: Pressure and Temp are the only 2 var affecting phases of any material. Graphs depicting these phases with P, T being on X,Y axis are called Phase change graphs.
Critical Temperature/Pressure: Once a gas is above its critical temperature and critical pressure (i.e critical point), it is impossible to get it to separate into a liquid layer below and a vapor layer above no matter how great a pressure is applied. Increasing the pressure only leads to the transition from gas to supercritical fluid.
Triple point: This is a particular temp and Pressure, where all 3 states exist simultaneously. For water, this point is at T=0.01C and P=0.006atm.