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Chemical Reactions José R. Valverde CNB/CSIC jrvalverde@cnb.csic.es
CC-BY-NC-SA
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Index Goals FMO theory Transition State calculations
Reaction Coordinate calculations Derived properties Limits
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Goal Predict compound reactivity Predict reaction mechanism
Compute reaction path and energies Calculate derived properties for experimental validation Compare properties between mutants/ligands
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Some terms e- donor: nucleophile, base, reductor
must be an occupied orbital e- acceptor: electrophile, acid, oxidizer must be an unoccupied orbital
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Frontier Molecular Orbitals
Reactions wih small energy barriers are favored The smaller the difference in energy among orbitals, the more favorable the reaction Orbitals normally have increasing energy as they distance from the nucleus The HOMO has the highest energy among occupied orbitals The LUMO has the lowest energy among unoccupied orbitals
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Simple FMO Theory HOMO + LUMO -> bonding MO
HOMO + HOMO -> antibonding MO LUMO + LUMO -> null (no e-) SOMO + SOMO -> bonding MO
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Cycloaddition
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Photochemical reactivity
Under thermal conditions Under photo-excitation
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8-oxo-GTP GTP HOMO LUMO Computed with ErgoSCF at the
6-31G** level from PDBechem entries 8GT and GTP LUMO
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Reactivity GTP 8-O-GTP
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Dynamic changes mov/QM/gtp-bnd-lumo.avi
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Dynamic changes mov/QM/8ogtp-bound-lumo-wire.avi
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Dynamical changes
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SN2 reaction A nucleophile (e- donor) attacks an electrophile
breaking a bond and releases a leaving (L) group.
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Active site effect
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Accurate modeling Explore conformational space to find lowest energy path Beware of tunneling effects Transition State Search Reaction Coordinate Path Quantum Dynamics
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Transition state Can be computed from reactants and products
A good intuition of the reaction path helps From TS, activation energy can be computed.
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Saddle calculations Optimize reactant Optimize product
Optimize product using reactant as reference Optimize reactant using closer product as reference Using the intermediate geometries, run a SADDLE calculation Use the result for a Transtion State calculation
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Reaction coordinate The reaction is modelled from reactants
The two atoms reacting and their relative path must be specified Some methods allow for specification of the atoms only and explore the space.
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Dynamic reaction models
mov/react/triton.mpeg
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ΔG‡-1 ΔG‡ DG
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Derived properties
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Balanced reactions reactants <--> products
DEreaction = SEproducts - SEreactants DE < 0 => exothermic, favorable DE > 0 => endothermic, unfavorable
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Isomer stability isomer1 <--> isomer2
DEisomer = Eisomer2 - Eisomer1 DE < 0 => isomer2 is more stable
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Activation energy DE‡ = ETS - Ereactants TS = Transition State
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Free Energy DGrxn = DHrxn - T DSrxn
DHrxn = enthalpy of rxn ≈ DErxn = SDEprod - SDEreac T = Temperature DSrxn = entropy of rxn = SDSprod - SDSreac In most reactions DS can be neglected DGrxn ≈ DHrxn ≈ DErxn
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Equilibrium constant Keq = e ( - DG / RT ) DGreaction = - R · T · ln Keq Keq = equilibrium constant DGreaction = Free energy of the reaction R = Gas constant T = Temperature in ºK Keq = e ( · DGreaction) in a. u. at 300K: Keq ≈ e ( · DEreaction) in Kcal/mol at 300K: Keq ≈ e( · DEreaction)
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Reaction rate Krxn is related to DG. If entropy is neglected
Krxn = (Keq T h) · e ( -DE‡ / R T) Keq = Boltzmann's constant h = Planck's constant DE‡ = Activation energy In a.u. at 300K: Krxn = 6.2 · 1012 · e ( DE‡)
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Half life (t½) Amount of time taken for the reactant concentration to drop to 1/2 the original value. For a first-order rate reaction rate = - Krxn [reactant] t½ = ln 2 / Krxn = 0.69 / Krxn
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Thanks To all of you For coming... and not falling asleep
To the organizers For this wonderful opportunity To CNB/CSIC, EU-COST, CYTED For funding
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