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Definition of Physical Properties
Properties which can be studied without changing the identity of a substance
Examples of physical properties
Boiling of water, melting of ice, color, odour, density, and sublimation
Definition of Chemical Properties
Properties which cannot be studied without changing the identity of a substance
Examples of chemical properties
Neutralization reactions, decomposition reactions, and rusting
Definition of Non-Matter
That which is not matter; examples include love, emotions, feelings, thoughts, energy, sound, light, anger, and time
Relationship between Kelvin (K) and Celsius (C)
K = C + 273
Relationship between Fahrenheit (F) and Celsius (C)
C/5 = (F - 32)/9
Specific Charge
Ratio of charge to mass (Charge of particle / Mass of particle)
Specific charge of a proton
Approx 9.9 x 10^7 C/kg
Specific charge of a neutron
0
Mass number (A)
Number of neutrons + Number of protons
Identity of number of protons (p) and electrons (e) in a neutral atom
No. of p = No. of e = Z (Atomic number)
Formula for number of neutrons (n)
A - Z
Minimum real charge on any particle
1.6 x 10^-19 Coulomb
Mass of a proton in terms of mass of an electron
Mass of proton = 1837 x (Mass of electron)
Definition of a Molecule
Smallest particles of an element or compound which must have independent existence
Protons in a molecule
Sum of [(Z value of atom) x (Total no. of atoms)]
Electrons in a molecule
Sum of [(Z value of atom) x (Total no. of atoms)]
Neutrons in a molecule
Sum of [(A - Z value of atom) x (Total no. of atoms)]
Electrons in an ion
No. of protons - (Total positive charge) + (Total negative charge)
Percentage of more neutrons than electrons in an ion
[(n - e) / e] x 100%
Definition of Valency
Combining capacity of any atom
Solid state condition regarding forces
Attractive Force >> Thermal Energy
Liquid state condition regarding forces
Attractive Force < Thermal Energy
Gaseous state condition regarding forces
Attractive Force << Thermal Energy
Correct order of Thermal Energy
Gas > Liquid > Solid
Correct order of Intermolecular force
Solid > Liquid > Gas
Standard form of Scientific Notation
N x 10^n (where 1 <= N < 10)
Scientific notation decimal move towards Left
Power becomes positive
Scientific notation decimal move towards Right
Power becomes negative
Significant figure rule for non-zero digits
All non-zero digits are considered significant
Significant figure rule for leading zeros
Zeros placed to the left of non-zero digits are not considered significant
Significant figure rule for trapped zeros
Zeros placed between non-zero digits are considered significant
Significant figure rule for trailing zeros
Without decimal, they are insignificant; with a decimal point, they are significant
Significant figure rule for counting physical quantities
Considered to be infinite
Rule for addition/subtraction of Significant Figures
The result cannot have more significant figures to the right of the decimal point than any of the numbers being added or subtracted
Rule for multiplication/division of Significant Figures
The result cannot have more significant figures than the number having the minimum significant numbers in the calculation
Rule if rightmost digit is > 5
Preceding digit is increased by one (+1)
Rule if rightmost digit is < 5
Preceding digit remains the same
Rule if rightmost digit is 5 and preceding digit is Odd
Preceding digit is increased by one (+1)
Rule if rightmost digit is 5 and preceding digit is Even
Preceding digit remains the same
Definition of Isotopes
Same elements (same Z value) having different mass numbers (different A value)
Definition of Isobars
Different elements (different Z value) having the same mass number (same A value)
Definition of Isotones
Different elements having the same number of neutrons or same (A - Z) value
Definition of Isodiaphers
Different elements (different atomic number) having the same (n - p) value or (A - 2Z) value
Definition of Isoelectronic species
Different atoms, ions, or molecules having the same number of electrons
Definition of Isosters
Different molecules having the same number of total electrons and the same number of atoms
Relationship between number of alpha particles deflected (N) and thickness of foil (T)
N proportional to T
Relationship between number of alpha particles deflected (N) and Kinetic Energy (KE)
N proportional to 1 / (KE^2)
Relationship between number of alpha particles deflected (N) and Atomic Number (Z)
N proportional to Z^2
Relationship between number of alpha particles deflected (N) and Angle of Deviation (theta)
N proportional to 1 / [sin(theta/2)]^4
Formula for Centrifugal Force (Fc)
Fc = (m * v^2) / r
Force of Attraction (Fa) in orbit derivation
Fa = (K * Z * e^2) / r^2
Orbital Kinetic Energy (KE)
KE = 1/2 * m * v^2 = (Z * e^2 * K) / 2r
Orbital Potential Energy (PE)
PE = -(Z * e^2 * K) / r
Orbital Total Energy (TE)
TE = -(Z * e^2 * K) / 2r
Energy Relationship between PE and KE
PE = -2 * KE
Energy Relationship between TE and KE
TE = -KE
Ratio of PE to KE
-2
Radius of Nucleus (R)
R = [1.33 x A^(1/3)] x 10^-13 cm (where A is mass number)
Distance of Closest Approach (r)
r = (4 * Z * e^2 * K) / (malpha * valpha^2)
Density of a nucleus
A constant quantity and very large
Definition of Wave Number (v-bar)
Reciprocal of Wavelength (1/lambda)
Speed of light/radiation (C)
C = frequency * wavelength
Definition of Quantum/Photon
Discrete and indivisible packets of energy
Energy of a single photon (Eph)
Eph = h * frequency = (h * c) / wavelength
Total Energy of N quanta (ETotal)
ETotal = N * h * frequency OR N * (h * c / wavelength)
Planck constant (h) value
6.626 x 10^-34 Js
Avogadro number (NA)
6.022 x 10^23
Conversion of 1 eV to Joules
1.6 x 10^-19 J
Shortcut formula for Energy in eV
E(eV) = 1240 / wavelength(nm)
Additive properties of wavelength when energy is conserved
1/lambda = 1/lambda1 + 1/lambda2
Definition of Power
Power = Energy / Time
Definition of Stationary State
A fixed orbit where an electron revolves and its energy remains constant
Bohr Postulate for Quantization of Angular Momentum (L)
L = mvr = nh / 2pi
General formula for Radius of nth orbit
r = (n^2 * h^2) / (4 * pi^2 * m * Z * e^2 * K)
Numerical formula for Radius (r)
r = (0.529 Angstrom) * (n^2 / Z)
Numerical formula for Velocity of electron (V)
V = 2.18 x 10^6 * (Z / n) m/s
Velocity acquired by electron accelerated from rest
v = sqrt(2eV / m)
Relationship between Time period (T) and n, Z
T proportional to n^3 / Z^2
Relationship between Frequency (f) and n, Z
f proportional to Z^2 / n^3
Energy of an electron in nth orbit (TE in eV)
TE = -13.6 * (Z^2 / n^2) eV
Definition of Ground State
The state of electron where its energy is minimum (n=1)
Definition of nth Excited State
Orbit No. = n + 1
Ionization Energy (IE) of Uni-electronic system
IE = +13.6 * (Z^2 / 1^2) eV
Definition of Separation Energy (SE)
Energy required to send an electron from its excited state to infinite energy state; SEnth = -E(n+1)
Rydberg Equation for Wavelength
1/lambda = RH * Z^2 * (1/n1^2 - 1/n2^2)
Rydberg Constant (RH)
109677 cm^-1 or 10967700 m^-1
Rydberg Calculation trick for wavelength
1/R = 912 Angstrom
Rydberg Equation for Energy Change (delta E)
delta E = R-primeH * Z^2 * (1/n1^2 - 1/n2^2) where R-primeH approx 2.18 x 10^-18 J
Total number of spectral lines for transition from n to 1
n(n-1)/2
Total number of spectral lines for transition from n2 to n1
(n2 - n1)(n2 - n1 + 1) / 2
Einstein Photoelectric Equation
Energy of photon (Eph) = Work-function (phi) + KE_max
Definition of Work-function (phi)
Minimum energy needed to overcome in order to take an electron out of a metal surface
Formula for Work-function (phi)
phi = h * frequency0 = (h * c) / wavelength0
Conditions for Photoelectric Effect
Eph >= phi, frequency >= frequency0, and wavelength
De-Broglie Wavelength Equation
lambda = h / p = h / (m * v)
De-Broglie relationship between wavelength and Kinetic Energy (KE)
lambda = h / sqrt(2 * m * KE)
De-Broglie relationship between wavelength and Voltage (V)
lambda = h / sqrt(2 * m * q * V)
Shortcut formula for electron wavelength (lambda_e)
lambda_e = sqrt(150 / V) Angstrom or 12.3 / sqrt(V) Angstrom