Techniques & Approaches Flashcards
(48 cards)
We need a strategy for detecting short-lived intermediates at room temperature - generating them at a high concentration & detect them
What are the various ways can we do this?
- Use photochemistry - initiate chemical reactions
a) cooling down to make intermediates very long-lived ≤ 77K - traps complex in solid glass (transparent) or matrix (noble gas)
b) cool down to make intermediates and reactive products long-lived - complex in inert solvent (noble gas)
c) Detect at room temperature using fast spectroscopy
What are two ways we can study intermediates
- Low temperature in a solid matrix
- Or a liquidifed noble gas to study intermediates
Describe the matrix isolation approach for intermediate monitoring?
- Uses inert gases (e.g. Ar) at ca. 12K or hydrocarbon glass (e.g. methyl cyclohexane) at 77K
- Using low temperatures and rigid matrix means that intermediates are long-lives and can be studied using conventional spectroscopy e.g. FTIT or UV/Vis
- UV or visble light are used to initiate reactions
How many IR spectrums might you take when analysing intermediates in a reaction using matrix isolation?
- Run the IR to get a starting spectrum of the products
- Run a second IR once the reaction has started to monitor the spectrum of photoproduction
- New band in the middle showing intermediate
For the following reaction:
Cr(CO)₆ + PPh₃ → Cr(CO)₅(PPh₃) + CO
The experiment of: trapping Cr(CO)₆ in Ar matrix at 12K and photolyse this, forming
How can this be measured?
- CO will produce a characteritic peak of its own the the IR
- The C4v product is predicted to have 3 IR bands
- The D3h product is predicted to have 2 IR bands
- e.g. on graph before photolysis shows 1 CO peak and after photolysis it shows 3 new CO peaks (C4V)
There is also large differences in the UV before and after photlysis for the following reaction:
Cr(CO)₆ + PPh₃ → Cr(CO)₅(PPh₃) + CO
What did it suggest
- Effect was not a generalised matrix effect
- suggested matrix coordination e.g. Cr(CO)₅…CH₄
A similar example of the following reaction undertaken in a matrix of isolation in Argon for:
What are two things you can comment on this reaction
- Solid Argon prevents reaction warming allowing diffusion
- Shows activation energy is around ~0°
Here is a similar reaction taken in a maxtrix isolation in Argon:
How can we characterise this reaction process?
Why is there no back reaction?
- Ni(CO)₃(N₂) - characterised by v(CO) and v(NN) IR bands
- N₂ only shows on IR once coordinated due to the formation of a dipole - sigma donation + pi backbonding
- There is no reverse reaction (30K) - Ea>0 (18e- compound) - importance of kinetic of reactivity not just intermediates
How can be study unstable species in solution?
- Using liquified noble gases - inert
- This is done at 20 atm pressure to increase the range they are liquid
Why are unstable species studied in noble gases?
- Need solvent to be transparent to IR
- IR absorbed by vibration of bond between atoms - Ar, Kr, and Xe only have one atom in the molecule
What is interesting about the following reaction
- The thermal back reaction can go by either Id or D pathway depending on the temperature (Id at low T)
- By using liquid Krypton, we can probe the mechanism, measuring its thermodynamic parameters and deduce what is happening
Intermediates are short-lived at room temperature
What is required to detect them?
- Rapid detect
- To characterise intermediates
- Allowing reaction kinetics to be obtained
If we have a slow reaction with the t½ (half-life) > single scan of the FT-IR; we can use FTIR to monitor the reaction
If we have a fast reaction with the t½ (half-life) < single scan of the FT-IR, we need a new approach of …
- UV/Visible Flash Photolysis
UV/Visible Flash Photolysis uses a pump-probe technique
What does this entail?
- Use pump (flash) to generate intermediates
- Use probe to monitor reaction
- Detection can be in UV/visible/IR region
- Original apparatus - use UV/Vis detection
UV/Vis Flash Photolysis uses a point-by-point appraching
What does this entail?
- Select on λ₁ (specific wavelength) and use pump to generate intermediate
- Measure change in absorbance at λ₁ with regards to time
- Select λ₂ and repeat
- Repeat for many λ
- Plot change in absorance vs λ for a certain Δt after flash
- We get kinetic (left) and spectra (right) information from this approach
What are some benefits of the UV/Visible Flash Photolysis
- Works well for nanoseconds/miliseconds/microseconds → due to having a continous wave (cw) probe and can use electronics to get the timings right
- (CW - light on probe on all the time)
- Obtain kinetics
- Can now use multichannel detectors to obtain all wavelengths at once
Lazers can be very fast but sometimes reactions occur on the picosecond/femtosecond scale - might need another approach to get the timng right
What is a way to get to get around this?
- Use pulsed pump and probe pulses
- Change time between pump and probe by making the probe beam travel further
What are some important features of he lazers in ns-IR flash photolysis?
- Uses IR laser - orginally IR diodines and now Quantum Cascade Lazers
- These give out tunable CW IR light
- Each lazer covers 150 cm⁻¹ - available to cover whole IR region
How do you do ns-IR Flash Photolysis
- Tune IR diode lazer to one IR frequency, λ₁
- Pulse UV lazer and measure cange in IR intensity at λ₁
- Tune IR lazer to λ₂ and repeat measurement
- Build up IR spectra “point-by-point”
List some advantages of UV/Vis for Detection methods for flash photolysis
- Good CW sources e.g. Xe lamp
- Sensitive detectors
- Very good kinetics
- Commercially available nanosecond and picosecond systems
List some advantages of IR detection methods for flash photolysis
- Narrow absorptions
- Very good specificity
- Obtain structural information especially good for metal carbonyls
- Moderate Kinetics
List some disadvantages of UV/Vis for detection methods for flash photolysis
- Broad absorptions
- Difficult to obtain kinetics in multi-component systems
- Little structural information for large molecules in solution
List some disadvantages for IR detection methods for flash photolysis
- Detectors much less sensitive than those in UV/Vis
- Powerful IR sources (lasers) only cover part of the IR range
The following two molecules are isomers of [CpFe(CO)₂]₂
How would the photochemistry (IR) of them differ?
- The cis- and trans-isomers in solution (mainly trans in non-polar solvent)
- Cis isomer = 3 IR v(CO) bands → 2 v(CO) terminal and 1 bridging
- Trans isomer = 2 IR v(CO) bands → 1 terminal and 1 bridging