physical chemistry

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334 Terms

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atomic number

the number of protons in the nucleus

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mass number

the total number of protons and neutrons in the nucleus

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isotope

atoms of the same element with the same number of protons and electrons but a different number of neutrons

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relative atomic mass

the average mass of an atom compared to 1/12 of a carbon-12 atom

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relative formula mass

the sun of the relative atomic masses of atoms in a molecule

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relative molecular mass

the average mass of a molecule of an element or compound relative to 1/12 of a carbon-12 atom

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avogadro’s number

6.022×10²³

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stages of mass spectrometry

vaporisation, ionisation, acceleration, ion drift, detection

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electron impact

bombarded with high energy electrons, forms M^+ ions

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electrospray ionisation

sprayed through a hypodermic needle with large voltage, forms MH^+ ions

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acceleration stage of tof

all ions are accelerated such that they have the same kinetic energy. ions are accelerated by a negatively charged acceleration plate. all have same kinetic energy

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ion drift

lighter ions travel faster and meet the detector first. heavier ions travel slower

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detection stage of tof

ions hit the detector and gain an electron. the more abundant a particular ion, the greater the current generated

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avogadros number meaning

the number of ions present in a sample with a mass equal to its relative formula mass

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mass of one ion equation

mass = relative isotopic mass x 10^-3 / 6.022×10²³

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kinetic energy equation

KE = ½mv²

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velocity equation simple

v= d/t

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velocity equation combing kinetic energy

v = √m/2KE

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tof comparing different isotopes equations

mv = mv

m/t² = m/t²

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calculation for max number of electrons in energy level

2n² where n is the energy level

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number of orbitals in the s subshell

1

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shape of s orbital

spherical

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number of orbitals in p subshell

3

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shape of p orbital

dumbbell shaped

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number of orbitals in d subshell

5

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number of orbitals in f subshell

7

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the Aufbau principle

electrons always fill up the lowest energy subshell first

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hund’s rule

electrons will always go into empty orbitals before pairing because they repel each other

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the Pauli exclusion principle

there is a maximum of two electrons with opposite spin in one orbital

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electronic configuration of copper

[Ar] 4s^1 3d^10

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electronic configuration of chromium

[Ar] 4s^1 3d^5

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isoelectronic

atoms or ions of different elements that have the same electronic configuration

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are 4s or 3d electrons lost first?

4s because it is a higher energy level

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enthalpy change of 1st ionisation energy

when 1 mole of gaseous atoms lose 1 mole of electrons to form 1 mole of gaseous 1+ ions

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factors that affect ionisation energy

  1. atomic radius - greater distance - less attraction

  2. nuclear charge - greater charge - greater attraction

  3. electron shielding - greater shielding - less attraction

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trend in ionisation energy down the group

  1. greater radius - loses electrons more easily

  2. greater charge - more attraction

  3. more shielding - less attraction

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trend in ionisation energy across a period

  1. smaller radius - greater attraction

  2. greater charge - more attraction

  3. same shielding - neutral effect

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number of moles equation

n = mass / Mr

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empirical formula

simplest whole number ratio of atoms in a compound

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percentage yield

how much product was produced compared to the expected amount

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reasons for percentage yield of less than 100%

  • impure reactants

  • reversible reaction

  • side reactions

  • loss of mass during transfer

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percentage yield calculation

(actual yield / theoretical yield) x 100

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atom economy

the measure of the amount of useful products in relation to the reactants

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atom economy calcualtation

(total mass of useful products / total mass of reactants) x 100

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number of moles calculation with liquids

n = cv

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ideal gas equation

PV = nRT

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assumptions made for ideal gas equation to work

  • all the particles are perfect spheres

  • there are no attractive forces between the particles

  • all collisions between particles are elastic so kinetic energy stays the same

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ionic bonding

the electrostatic force of attraction between oppositely charged ions

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factors that determine strength of an ionic bond

  1. ionic radius - smaller radius - stronger

  2. ionic charge - greater charge - stronger

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covalent bond

the electrostatic force of attraction between a pair of shared electrons and a positive nucleus

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factor that determines the strength of a covalent bond

bond length - larger atoms - longer bonds- weaker

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dative covalent bond

one atom supplies both electrons to form a covalent bond

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conditions for a dative covalent bond to form

  1. one atom must have a vacant orbital

  2. another atom must have a lone pair of electrons

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dimer

when two of the same small molecule join together to form a larger molecule via dative covalent bonding

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metallic bonding

the electrostatic force of attraction between positive metal ions and a sea of delocalised electrons

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factors that affect the strength of metallic bonds

  1. ionic radius

  2. ionic charge

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valence shell electron pair repulsion theory

  • bonding pairs repel other bonding pairs equally and as much as possible

  • lone pairs repel other lone pairs equally and as much as possible

  • lone pairs repel more than bonding pairs

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way to find base shape of molecule

valence electrons of central atom + number of bonds formed all divided by 2

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bond angles with lone pairs

take 2.5 degrees away for every lone pair

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polar bonds

ionic character of covalent bonds

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electronegativity

the ability of an atom to withdraw electron density towards itself in a covalent bond

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factors affecting electronegativity

  1. nuclear charge

  2. atomic radius

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trend in electronegativity across a period

  • nuclear charge increases

  • atomic radius decreases

    —> greater electronegativity

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trend in electronegativity down a group

  • atomic radius increases

  • nuclear charge increases

    —> lower electronegativity

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most electronegative atom

fluorine

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requirement for ionic bonds with covalent character

  1. a polarising cation - small highly charged cations which distort the shape of the anion

  2. a polarisable anion - large anions

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van der waal’s forces

electron movement in first molecule induces a dipole in another, resulting to a temporary attraction between d+ on one molecule and d- on another

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factors that determine the strength of van der Waal’s forces

  1. size of the molecule - greater size - greater imf

  2. shape of the molecule - branched chains don’t pack as closely together - lower imf

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factors that determine the presence of dipole-dipole interactions

  1. presence of electronegative atoms resulting in polar bonds

  2. shape of the molecule - the distribution of charge must be asymmetric

    the molecule must have an overall dipole moment

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order of increasing strength of intermolecular forces

  1. van der Waal’s forces

  2. dipole-dipole interactions

  3. hydrogen bonds

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factors for hydrogen bonds to occur

  1. a hydrogen atom must be directly bonded to one of the most electronegative elements eg. F, N, or O

  2. the electronegative element must have a lone pair of electrons

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way to draw hydrogen bonds

  1. show all lone pairs of electrons

  2. show all partial charges

  3. linear arrangement of covalent bond and hydrogen bond

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periodicity

the study of trends shown by the elements which repeat themselves in each period of the periodic table

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oxidation

loss of electrons

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reduction

gain of electrons

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reducing agent

(itself is oxidised) loses electrons

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oxidising agent

(itself is reduced) gains electrons / oxidises another atom or ion

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neutral compound oxidation state

equals 0

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<p>name and bond angle of this shape </p>

name and bond angle of this shape

name: linear

bond angle: 180

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<p>name and bond angle of the shape</p>

name and bond angle of the shape

name: trigonal planar

bond angle: 120

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<p>name and bond angle of this shape</p>

name and bond angle of this shape

name: bent

bond angle: 117.5

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<p>name and bond angle of this shape</p>

name and bond angle of this shape

name: tetrahedral

bond angles: 109.5

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<p>name and bond angle of this shape</p>

name and bond angle of this shape

name: trigonal pyramidal

bond angle: 107

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<p>name and bond angle of this shape</p>

name and bond angle of this shape

name: bent

bond angle: 104.5

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: trigonal bipyramidal

bond angle: 90,120

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: sawhorse or seesaw

bond angles: 87.5, 117.5

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: T shaped

bond angles: 90

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: linear

bond angle: 180

89
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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: octahedral

bond angles: 90

90
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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: square pyramidal

bond angles: 87.5

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: square planar

bond angles: 90

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: T shape

bond angle: 87.5

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<p>name and bond angles of this shape</p>

name and bond angles of this shape

name: linear

bond angle: 180

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Exothermic reaction

Releases energy to the surroundings

  • energy of the products is less than the reactants

  • Characterised by an increase in temperature

  • Bond formation is exothermic

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Endothermic reaction

Absorbs energy from the surroundings

  • energy of the products is greater than the reactants

  • Characterised by a decrease in temperature

  • Bond breaking is endothermic

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Enthalpy change (delta H)

Heat change at constant pressure

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Standard conditions (°)

298K, 100kPa, 1.00 moldm-3

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Standard enthalpy change of formation

Enthalpy change when 1 mole of a substance is formed from its constituent elements with all reactants and products in standard states under standard conditions

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Standard enthalpy change of combustion

Enthalpy change when 1 mole of a substance is completely burned in oxygen with all reactants and products in standard states under standard conditions

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Mean bond enthalpy

The enthalpy change required to break 1 mole of a covalent bond in gas phase, averaged over a range of compounds