Structure, Bonding and Equilibria Flashcards
Electronegativity
The ability of an atom to attract an electron to itself.
Electronegative elements
F
O
Cl
Top right of periodic table
Electropositive elements
Cs
Ba
Rb
Bottom left of periodic table
Ionic bonding when…
Difference in electronegativity >2
Covalent bonding when …
0.5< difference in electronegtivity <2
Metallic bonding when…
Difference in electrnegativity <0.5
ΔH atomisation
X(standard) -> X(g)
always endothermic
1st ionisation enthalpy
X(g) -> X⁺(g) + e⁻
always endothermic
Electron gain enthalpy
X(g) + e⁻ -> X⁻(g)
usually exothermic (or close to it)
Lattice enthalpy
X⁺(g) + Y⁻(g) -> XY(s)
always exothermic (when defined in this way)
General trend in I.E. across a period.
Why?
Overall, ionisation energy increases across a period.
Increasing nuclear charge and reduced electron shielding ability increases effective nuclear charge.
Electrons experience greater attraction to nucleus, so more energy input required to remove them.
Zeff
Effective nuclear charge - the actual amount of positive charge experienced by an electron.
Zeff = Z (atomic number) - S (shielding constant)
Electron shielding
Partial neutralisaiton of nuclear charge by core electrons + electron-electron repulsion reduces Zeff felt by outer shell electrons.
Electron penetration
An electron’s relative electron density near the nucleus - i.e. proximity to which an electron can approach the nucleus.
Penetrating power depends on shell and subshell
1s>2s>2p>3s>3p>4s>3d etc
In the second period, why is there a dip in 1st I.E at B and O?
Boron - the outer 2p electron does not penetrate the 2s electrons effectively. Therefore easier to remove.
Nitrogen - repulsion between paired 2p electrons makes them easier to remove.