Doctoral studies in the Institute of Physics are regulated by the university Regulations for Doctoral Studies.
More information about the doctoral studies can be found in the Doctoral center page of Faculty of Science and Technology together with the information about organisation, planning and completing doctoral studies.
An overview of the steps you need to take if you are planning to apply for doctoral studies at the University of Tartu can be found in the web-page Admission to doctoral studies.
Important information for doctoral students is available on the web page of Doctoral Center of Faculty of Science and Technology. There is also specific section for the 1st year students including the to-do list for the first semester.
Information regarding the submission and defense of the doctoral thesis collected in a Guidance to reach PhD. The opponents can use a similar Guidelines for opponents.
Our institute is participating in the curriculum of Physics, the curriculum of Materials Science and the curriculum of Environmental Technology.
Since the year 2022/2023, we are participating in the following new doctoral programmes:
The programme includes three specialities with responsible institutes shown in parenthesis:
1. Physics (Institute of Physics)
2. Chemistry (Institute of Chemistry)
3. Space research and technology (Tartu Observatory)
The programme includes five specialities with responsible institutes shown in parenthesis:
1. Computer Engineering (Institute of Technology)
2. Sustainable Energetics (Institute of Chemistry)
3. Environmental Technology (Institute of Ecology and Earth Sciences)
4. Materials Science (Institute of Physics)
5. Molecular Biotechnology (Institute of Technology)
Progress review of doctoral students follows the procedure of Faculty of Science and Technology:
During the progress review, the progress of doctoral students in doctoral programmes opened from 2022/2023 is evaluated based on outcomes (not in credit points).
II.5. Progress review
II.5.3. Documents required for progress review
At the end of the first semester of the first year of study, the doctoral student:
At the end of the first year of study, the doctoral student:
At the end of the second year of study, the doctoral student:
At the end of the third year of study, the doctoral student:
At the end of the fourth year of study, the doctoral studies are assessed positively if the doctoral thesis manuscript has been completed in line with the requirements of the regulations and the compulsory activities of the modules of the doctoral programme have been completed.
In the progress review, it is necessary to submit the progress review report and period plan for the next year which can be obtained from the Doctoral center web-page.
The progress review report along with the activity plan for the next period, certified by the student’s and supervisors' digital signatures, must be loaded to CIS and sent to the head of the progress review committee. The first year students must also submit the individual plan for the end of first semester.
The estimated time for the review per one student is 15 min, including a short (up to 5 min) report with few slides, followed by answers to the questions from the members of the committee.
The attestation committee allows the doctoral student and the supervisors to give feedback on the cooperation without the presence of the other party. If you wish, please inform the chairman of the attestation committee before the attestation, in this case the committee will reserve time to give feedback.
The successful PhD research projects for the year 2026 are listed below. There are 4 projects in the specialty of Physics and 1 project in the specialty of Materials Science.
The admission period is 1-15 May: https://reaalteadused.ut.ee/en/node/111725
This project focuses on developing nanostructured photocatalytic materials that are active under visible light to create antimicrobial surface coatings for reducing microbial transmission on frequently touched surfaces in healthcare facilities and public spaces. Photocatalytic antimicrobial action is driven by the generation of reactive oxygen species (ROS), which oxidize and decompose organic contaminants and microbial cell components. Current commercial photocatalytic coatings, predominantly based on TiO₂, require UVA illumination, limiting their usefulness indoors where visible light dominates. A key challenge in the field is producing visible‑light‑active photocatalysts that generate ROS as efficiently as UVA‑activated materials.
To address this gap, during this project several promising visible-light responsive photocatalysts with known antimicrobial properties will be synthesized and evaluated: WO₃, ZnIn₂S₄, ZnIn₂S₄/g‑C₃N₄, and ZnIn₂S₄/WO₃. These compounds will serve as the active components in coating formulations. Another important challenge is ensuring strong, durable adhesion of the coatings to different surfaces. Commercial acrylic paints and ethyl‑methacrylate polymer will be explored as matrix materials and to achieving uniform distribution of the synthesized photocatalysts within these matrices remains one of the central tasks of this project.
Overall, this project aims to close the technological gap that currently limits photocatalytic coatings to UVA‑dependent systems. By integrating material synthesis, surface engineering, and antimicrobial testing, it will establish a robust basis for practical, indoor‑applicable antimicrobial surfaces.
Please contact prof. Vambola Kisand ([email protected]). Co-supervisors are dr. Alexander Vanetsev, prof. Angela Ivask and prof. Wei Cao (University of Oulu). The study will be carried out in the Laboratory of X-Ray spectroscopy.
Engineering and Technology (Materials Science).
Optical cavities, particularly planar Fabry–Perot (metal–dielectric–mirror) resonators, are key platforms in molecular strong coupling, polaritonics, and quantum optics. By enabling hybridization of light with excitonic, plasmonic, and vibrational excitations, these systems provide access to the strong-coupling regime, where optical and energetic properties can be profoundly modified. Such cavity-mediated effects underpin emerging applications in polaritonic light sources, cavity-controlled energy transfer, and polaritonic chemistry, including reaction-rate engineering.
This project builds on our group’s established expertise in cavity optics, polariton physics, strong light–matter coupling, and DNA origami–based nanosystems. We will further develop a grayscale UV-lithography technique for the rapid, parallel fabrication of Fabry–Perot microresonators. The method enables high-throughput production of dye-doped cavities, increasing fabrication yield from a few devices per day to thousands, thereby substantially accelerating experimental studies.
The work will focus on improving fabrication accuracy and defect control, optimizing photoresist–emitter combinations (including quantum dots, molecular dyes, photosynthetic proteins, and DNA origami FRET systems), and extending the approach to hollow, variable-thickness cavities for liquid-phase measurements. Advanced Fourier-plane spectroscopy will be employed to characterize the resonators and evaluate their performance in optical and vibrational strong-coupling experiments, with emphasis on spectral modification and cavity-controlled energy-transfer processes. As a result of this doctoral project, at least three scientific publications are planned. The present doctoral project is associated with two PRG projects that commenced in 2026.
Please contact dr. Siim Pikker ([email protected]). Co-supervisors are dr. Veikko Linko and Arvi Freiberg. The study will be carried out in the Laboratory of Physics of Nanostructures.
Chemical and Physical Sciences (Physics).
Do anthropogenic aerosols affect Earth’s climate by acting as ice-seeding particles? Our recent work revealed that certain industrial aerosols seed ice, suggesting that an overlooked climate-forcing mechanism may exist. This project develops the first-ever global database of anthropogenic aerosol sources seeding ice and calculates the associated impact on Earth’s climate. For this, the work combines long-term satellite records, atmospheric dispersion modelling, and laboratory experiments. Aerosol dispersion modelling will allow to automatically identify ice‑seeding at 30 thousand industrial facilities.
The ice seeding at isolated localised industrial sites will be compared with ice seeding around megacities and larger industrial regions at climate-relevant scales: over multiple decades at spatial scales spanning hundreds-by-hundreds of kilometres. To quantify the climate impact by ice-seeding aerosols, we calculate it relative to the climate impact by aerosols serving as seeds for liquid clouds. By this, we address a major open question in climate science: are current climate predictions missing an important anthropogenic climate-forcing mechanism?
Please contact prof. Velle Toll ([email protected]). The study will be carried out in the Centre for Climate Research.
Chemical and Physical Sciences (Physics).
Quantum computation is a novel paradigm of computing which is capable of solving problems that remain intractable for conventional computing. In particular, quantum computers are able to efficiently simulate large quantum systems, a task beyond the reach of conventional computers, regardless of their scale. This is of great interest for quantum chemistry and materials science, which underlie chemical and pharmaceutical industries and development of new materials and technologies. While fault tolerant quantum computing is predicted to arrive earliest in a decade, near term quantum devices which involve a few hundred qubits are becoming a reality presently. The project focuses on simulation of quantum systems that are of interest in quantum chemistry and solid state physics using the paradigm of variational quantum algorithms, as well as fault tolerant quantum computation. Analysis, benchmarking, testing and development of the range of methods that are used for simulation and computation of electronic structure and energy surfaces need to be carried out in order to make progress in quantum simulation on near term quantum devices.
Please contact dr. Veiko Palge ([email protected]). Co-supervisor is dr. Juhan Matthias Kahk. The study will be carried out in the Laboratory of Theoretical Physics and Laboratory of X-Ray spectroscopy.
Chemical and Physical Sciences (Physics).
The first direct image of a supermassive black hole in 2019 has been one of the most impressive scientific achievements not only for the gravitational research community but also for the general public, appearing in newspapers and on TV news. Understanding the physics behind this image is crucial to gathering more information about our universe and the theories governing it.
The equations of gravity describe how matter curves spacetime and how particles move within it. When these equations fail to explain observations fully, we can question either our assumptions about matter or the theory of gravity. The absence of direct evidence for dark matter and energy in explaining cosmic dynamics, for example, motivates exploring theories beyond Einstein’s general relativity. These lead to different equations and, therefore, also different black hole solutions, which leave distinct imprints on accretion dynamics and photon trajectories. In this way, black holes serve as natural laboratories for testing gravitational theories through their observable images. However, using toy models to reduce the complexity of the problem may introduce degeneracies between the effects of spacetime geometry and accretion disk physics, potentially leading to misinterpretation of the results.
Establishing a solid foundation for rigorously testing general relativity and theories beyond that against the current and future black hole observations requires a deep understanding of how gravity influences all physical processes encoded in the image. The objective of this PhD project is to make systematic steps to assess the impact of theories beyond general relativity on (1) the geometry of spacetime as manifested in the “shadow” of the image, (2) the matter dynamics and the feasibility to develop semi-analytic models of the accretion disk, and (3) the potential signatures in the polarisation patterns of the observational data.
Please contact dr. Laur Järv (laur.jä[email protected]). Co-supervisor is dr. Mercè Guerrero Román. The study will be carried out in the Laboratory of Theoretical Physics.
Chemical and Physical Sciences (Physics).