- Value: This project is open to self-funded students and is eligible for funding in an open competition across the School of Chemistry, see funding schemes for details.
- Number of awards: 1
- Deadline: Applications accepted all year round
- Key benefits: The PhD will provide a broad spectrum of training in the use of high power lasers, vacuum systems, optics, computer controlled data acquisition systems and numerical calculations. You will work in a well equipped laboratory and be part of the active, thriving and well-funded Atmospheric and Planetary Chemistry group within the School of Chemistry. You will be supported to attend both national and international conferences, and will receive a wide range of training, for example in communication skills and other technical aspects.
Contact Professor Dwayne Heard to discuss this project further informally.
Neutral – neutral reactions are important in low temperature environments such as the interstellar medium (ISM), dense molecular clouds of star forming regions and planetary atmospheres, for example Titan, which is considered as an analogue of the primeval atmosphere of Earth. However, the chemical databases used to model such environments contain a relatively small number of this class of reaction and the low-temperature chemistry is poorly understood.
We have recently shown [1-4] that despite the presence of an energy barrier, the reaction between the OH radical and ketones, alcohols and ethers can proceed to products rapidly at very low temperatures, which we interpret via a mechanism involving the formation of a weak hydrogen bonded association adduct, and quantum mechanical tunnelling. These two features are present in many reactions involving hydrogen atom transfer and we propose that this behaviour may be widespread under the low temperature conditions found in space. Recently our data were included in an astrochemical model .
In this project you will measure rate constants and product branching ratios at very low temperatures using laser flash-photolysis combined with a variety of laser-based spectroscopic detection methods. You will use a pulsed Laval nozzle apparatus [1-6] to study the kinetics of reactions between ~40 and 150 K representative of the atmospheres of other planets and moons, for example Titan, as well as in star-forming regions, stellar outflows and the interstellar medium. [1-5]. Large molecular clouds of acetone, methanol and ethanol have been observed in space, and the large rate constants can be rationalised by the formation of a hydrogen-bonded complex, which can either be stabilised or undergo quantum mechanical tunnelling through the activation barrier to form products (Figure 1). For the OH-methanol reaction we observed the CH3O radical product, which was recently observed in space by astronomers [1, 5]. We have also studied the kinetics of singlet methylene, 1CH2, which is a metastable radical, and which is implicated in the formation of benzene and hazes on Titan. There are two competing paths for 1CH2, collisional quenching to the ground-state 3CH2, or reaction to form products.
You will interpret the laboratory measurements using theoretical methods, making use of ab initio potential energy surfaces and master equation calculations (using the MESMER program , developed in Leeds) to calculate rate constants as a function of temperature and pressure. These experiments use laser flash-photolysis combined with laser-induced fluorescence (LIF) spectroscopy, will be extended to study further reactions of OH, 1CH2 and other radicals, and will monitor both reactants and products, using LIF.
The PhD will provide a broad spectrum of training in the use of high power lasers, vacuum systems, optics, computer controlled data acquisition systems and numerical calculations. You will work in a well equipped laboratory and be part of the active, thriving and well-funded Atmospheric and Planetary Chemistry group within the School of Chemistry. You will be supported to attend both national and international conferences, and will receive a wide range of training, for example in communication skills and other technical aspects.
Read more about this project (pdf).
References 1. R. J. Shannon, M. A. Blitz, A. Goddard and D. E. Heard, Nature Chemistry, 5, 745-749, 2013. 2. R. J. Shannon, S. Taylor, A. Goddard, M. A. Blitz and D. E. Heard, Phys. Chem. Chem. Phys., 2010, 12, 13511–13514. 3. R.J. Shannon, R. L. Caravan, M.A. Blitz and D.E. Heard, Phys. Chem. Chem. Phys., 16, 3466, 2014. 4. R.L. Caravan, R. J. Shannon, T. Lewis, M. A. Blitz and D. E. Heard, J. Phys. Chem., DOI: 10.1021/jp505790m, 2014. 5. K. Acharyya, E. Herbst, R.L. Caravan, R.J. Shannon, M.A. Blitz & D.E. Heard, Mol. Phys., 113, 2243-2254, 2015. 6. S. E. Taylor, A. Goddard, M. A. Blitz, P. A. Cleary and D. E. Heard, Phys Chem Chem Phys, 2008, 10, 422-437. 7. D. R. Glowacki, C.-H. Liang, C. Morley, M. J. Pilling and S. H. Robertson, J Phys Chem A, 116, 9545-9560, 2012.
Applications are invited from candidates with or expecting a minimum of a UK upper second class honours degree (2:1), and/ or a Master's degree in a relevant science subject (but not limited to) chemistry or chemical engineering.
If English is not your first language, you must provide evidence that you meet the University's minimum English language requirements.
How to apply
Formal applications for research degree study should be made online through the university's website. Please state clearly in the research information section that the PhD you wish to be considered for is 'The kinetics of astrochemical and planetary reactions studied at very low temperatures' as well as Professor Dwayne Heard as your proposed supervisor.
We welcome scholarship applications from all suitably-qualified candidates, but UK black and minority ethnic (BME) researchers are currently under-represented in our Postgraduate Research community, and we would therefore particularly encourage applications from UK BME candidates. All scholarships will be awarded on the basis of merit.
If you require any further information please contact the Graduate School Office e: email@example.com