Research of Physics and Astronomy

Main research fields of the Department are material physics, quantum mechanics, and astronomy and space research.

Main research areas of Department of Physics and Astronomy

Solar energetic particle analysis platform for the inner heliosphere (SERPENTINE)

The University of Turku -led EU/H2020 project SERPENTINE investigates the origin of solar energetic particle events and provides an advanced platform for the analysis and visualization of high-level datasets to benefit the wider heliophysics community. The key data comes from the most recent European and US missions, i.e., Solar Orbiter, Parker Solar Probe and BepiColombo, which have opened completely new avenues to investigate solar eruptions.

European heliospheric forecasting information asset (EUHFORIA 2.0)

The EU/H2020 project EUHFORIA 2.0 addresses geoeffectiveness, impacts and mitigation related to solar eruptions, solar wind streams and solar energetic particles. In Turku, the research group focuses on the modelling of acceleration of particles to high energies in the corona.


Turku Centre for Quantum Physics

The Centre (TCQP) was founded in September 2009 and currently it consists of five research groups at the Department of Physics and Astronomy. It coordinates the shared activities of the participating groups and provides a unified background for teaching of quantum mechanics. TCQP is a joint activity between Laboratory of Quantum Optics, Laboratory of Theoretical Physics and Wihuri Physical Laboratory.

Centre of Excellence in Quantum Technology

This Academy of Finland centre of excellence ( aims to introduce novel approaches for control of quantum systems in order to develop technologies within quantum sensing, simulation, communication and computation. Quantum Technologies group, led by Prof. Sabrina Maniscalco, provides its theoretical expertise and collaborates with research groups from Aalto University and VTT.

Non-Markovian processes and complex systems

Theory of open quantum systems is an important and active area of modern quantum physics. Adjunct professor Jyrki Piilo with this group is studying how decoherence - the loss of quantum properties and information within small physical systems - happens when open system interacts with their environments. We are interested in how to characterize different dynamical features, e.g. non-Markovian memory effects,  and how to control and exploit these in fundamental tests of quantum physics and in applications to quantum technologies. Going from quantum optical to complex systems, we are interest in the realization of complex quantum networks, how quantum dynamics occurs within these networks, and how they can be used in the open system context. Having a more cross-disciplinary nature, we also work on developing statistical tools for the general field of network theory and use these methods and concepts in a data driven research on complex socio-economic systems. 

Dynamic response of organic molecules

In the research project of the Academy of Finland, led by Prof. Edwin Kukk, we follow, in the femto and picosecond timescales, the dynamic response of organic molecules to the x-ray or UV radiation. The purpose is to understand the nature of these omnipresent processes at a fundamental level, and at the same time to obtain insight into their practical consequences, such as the deterioration of materials under the influence of radiation (light).

Molecular mechanisms of radiosensitizers used in cancer therapy

In Prof. Edwin Kukk's project we study what kind of molecular-level mechanisms are at play when the so-called radiosensitizer-molecules are used in cancer therapy. One of the goals here is to find new, more efficient molecular compounds.


Studies on surfaces of semiconductor crystals

Docent Pekka Laukkanen studies and modifies surfaces of solids such as semiconductor crystals experimentally in order to decrease surface-related losses in the material applications.

Quantum mechanical simulations of matter

Professor Kalevi Kokko studies properties of matter using quantum mechanical simulations. The result is, for example, computational models that can be used to tune the properties of materials to fit better to the extreme conditions.

The Finnish Centre of Excellence in Research of Sustainable Space, FORESAIL (2018-2025)

FORESAIL is a consortium of four research groups led by the University of Helsinki, which concentrates on the research of space radiation and its effects on technology, and develops novel de-orbiting technologies suitable for small satellites to counter the ever increasing amount of space debris in near-Earth space. Professor Rami Vainio acts as the vice-director of FORESAIL and leads the Instruments team of the unit.

Space Radiation Expert Service Centre

Space Radiation Expert Service Centre is a project under the Space Situational Awareness programme of the European Space Agency, where we develop empirical data-driven models for predicting space radiation conditions. The project is led in Turku by Prof. Rami Vainio.

Towards Electron-scale Modelling of space Plasmas

We develop numerical models for particle acceleration and transport processes in the FORESAIL Centre of Excellence and in the Academy project "Towards Electron-scale Modelling of space Plasmas". The models are applied especially in investigations of solar eruptions and near-Earth space environment. The projects are led by professor Rami Vainio and senior researcher Alexandr Afanasiev.

Astrophysical transients

The main research interests of the group focus on observational work on extragalactic astrophysical transients. Supernovae are among the most energetic phenomena in the Universe marking the end-point in the evolution of certain stars, producing neutron stars and in more exceptional cases stellar mass black holes. These explosions play a vital role in our understanding of stellar evolution, the synthesis of heavy elements, and through feedback processes also in galaxy evolution. Furthermore, they can also be used as probes of the cosmic star formation history which is one of the most fundamental observables in astrophysical cosmology. While thousands of supernovae are discovered each year, luminous transients occurring within the nuclei of galaxies have been largely missed or overlooked by the surveys. Such events may arise when a star passing too close to a supermassive black hole at the center of a galaxy is disrupted by tidal forces caused by the gravity of the black hole. Tidal disruption events provide a means of probing central black holes in galaxies and testing scenarios of accretion onto supermassive black holes important for our understanding of galaxy evolution.

Quantum properties of Atomic Hydrogen

Docent Sergey Vasiliev pursues studies of quantum properties of atomic hydrogen in a gas phase at lowest possible temperatures and atomic velocities. Other research directions of the group include quantum behavior of atomic hydrogen in solid molecular crystals of hydrogen and its isotopes, and magnetic resonance of shallow donors in semiconductors. Further details can be found in the group's web site.

Flux pinning in high temperature superconductors

The group of prof. Petriina Paturi studies magnetic flux pinning in high temperature superconductor thin films. The research is done both experimentally and by computational modelling of the systems. The main aim is to enable design-based pinning structures for applications of superconductivity. More information can be found from the group web page.

Memristors from low bandwidth manganites

Memristors are seen to enable neuromorphic computing, which mimic the brain in their working. In the group lead by prof Petriina Paturi, we develop and model memristors made from low band width manganites such as Gd_1-xCa_xMnO_3. More information can be found from the group web page.

High Energy Astrophysics

The high-energy astrophysics group works on accreting black holes and neutron stars. The group uses both ground-based ESO VLT and the Nordic Optical Telescope (NOT) as well as space telescopes (XMM-Newton, Chandra, RXTE, INTEGRAL, Fermi, Swift, NuSTAR, SRG). We are also involved in preparation for the new X-ray missions being science group members of the NASA’s Imaging X-ray Polarimeter Explorer (IXPE) and of the Chinese enhanced X-ray Timing and Polarimetry (eXTP) missions. We are also doing optical polarimetric studies with the in-house built high-precision DIPol-2 and DIPol-Ultra Fast (UF) polarimeters.  On the theory side, we develop atmosphere models for rapidly rotating neutron stars with the aim to determine the equation of state (EoS) of cold dense matter of neutron stars and to understand the physics of accretion in these objects. We work on hydrodynamical models of boundary/spreading layers on weakly magnetized neutron stars to understand the nature of kHz quasi-periodic oscillations. We also study X-ray pulsars and ultra-luminous X-ray pulsars, both observationally and theoretically. We construct models for the accretion column and for the accretion disc around magnetized neutron stars as well as monitor the sources to study the transition to the propeller regime to measure the neutron stars magnetic field. We model broadband spectra and timing properties of accreting black holes both in the optical/infrared and the X-rays. See more in the link


Space Research Laboratory

The laboratory focuses on space physics at high energies. We investigate the generation of energetic particle radiation in particle acceleration processes at the Sun as well as its effects on spacecraft and satellites in orbit. We employ both computational and experimental methods in our studies, developing spacecraft instruments for detecting energetic particles and numerical models for simulating their acceleration and transport. The laboratory belongs to the Finnish Centre of Excellence in Research of Sustainable Space funded by the Academy of Finland (2018-2025) and to the Space Radiation Expert Service Centre of the Space Situational Awareness programme of the European Space Agency.

Laboratory of Quantum Optics

Main research topics of the laboratory are physics of laser cooled atoms and Bose-Einstein condensate, and quantum information, open quantum systems and complex networks. Research is mainly theoretical but it is closely related to experimental work on this field.

Materials Research Laboratory

In the Materials Research Lab, we use the latest spectroscopic and imaging methods for investigating the key properties, behaviour and suitability for practical purposes of a large variety of materials.  We study single molecules, clusters, nanoparticles, surfaces and multilayers and we perform experiments at the home laboratory as well as at large international accelerator facilities – synchrotrons and free electron lasers. We also offer materials characterization services to  companies, helping them in troubleshooting and in developing better materials.

There are two research groups in our laboratory:
In Femto group we focus on the behaviour of small quantum systems and on their interaction with radiation.
At Prof. Kalevi Kokko’s group, we conduct international materials research with cutting-edge methods. Interesting new material's phenomena found help us to aim to safer environment and better future.


Laboratory of Industrial Physics

The research of the laboratory is focused on porous nanostructured materials, electrostatics and pharmaceutical physics. The laboratory has also over 30-years history of collaboration with national and international companies. We have studied all kind of things from fishing lure to novel pharmaceutical formulations.

Laboratory of Theoretical Physics

The Laboratory of Theoretical Physics tackles fundamental questions within the fields of quantum technologies, quantum foundations, quantum field theory and cosmology. It is part of the Turku Centre for Quantum Physics.


Tuorla Observatory

The research at the Tuorla Observatory is carried out using ground-based telescopes of the European Southern Observary (ESO), the Nordic Optical Telescope (NOT) and space telescopes of ESA and NASA, and includes theoretical astrophysics and numerical methods. The largest groups at the Tuorla Observatory are the High-Energy Astrophysics group ( and Astrophysical Transients group ( In addition, research is done on active galaxies, solar system, astrobiology and simulations of large scale structures in the Universe. Research on solar physics is done in collaboration with the Space Research Laboratory (SRL) and on astronomical instrumentation in collaboration with the Finnish Centre for Astronomy with ESO (FINCA).

Wihuri Physical Laboratory

The Wihuri Physical Laboratory has two research groups: Superconductivity and magnetism and Atomic Hydrogen. Common theme on all research is working at low temperature, which continues the over 60 year old traditions of the laboratory.

The superconductivity and magnetism group concentrates in high temperature superconductors and magnetic perovskites and their applications. It is lead by prof. Petriina Paturi.

The atomic hydrogen group studies physics of hydrogen atoms at very low temperatures. It is lead by docent Sergey Vasiliev.

Latest publications

First Detection of Polarization in X-Rays for PSR B0540-69 and Its Nebula (2024)

Astrophysical Journal
Xie Fei, Wong Josephine, La Monaca Fabio, Romani Roger W., Heyl Jeremy, Kaaret Philip, Di Marco Alessandro, Bucciantini Niccolò, Liu Kuan, Ng Chi-Yung, Di Lalla Niccolò, Weisskopf Martin C., Costa Enrico, Soffitta Paolo, Muleri Fabio, Bachetti Matteo, Pilia Maura, Rankin John, Fabiani Sergio, Agudo Iván, Antonelli Lucio A., Baldini Luca, Baumgartner Wayne H., Bellazzini Ronaldo, Bianchi Stefano, Bongiorno Stephen D., Bonino Raffaella, Brez Alessandro, Capitanio Fiamma, Castellano Simone, Cavazzuti Elisabetta, Chen Chien-Ting, Ciprini Stefano, De Rosa Alessandra, Del Monte Ettore, Di Gesu Laura, Donnarumma Immacolata, Doroshenko Victor, Dovčiak Michal, Ehlert Steven R., Enoto Teruaki, Evangelista Yuri, Ferrazzoli Riccardo, Garcia Javier A., Gunji Shuichi, Hayashida Kiyoshi, Iwakiri Wataru, Jorstad Svetlana G., Karas Vladimir, Kislat Fabian, Kitaguchi Takao, Kolodziejczak Jeffery J., Krawczynski Henric, Latronico Luca, Liodakis Ioannis, Maldera Simone, Manfreda Alberto, Marin Frédéric, Marinucci Andrea, Marscher Alan P., Marshall Herman L., Massaro Francesco, Matt Giorgio, Mitsuishi Ikuyuki, Mizuno Tsunefumi, Negro Michela, O’Dell Stephen L., Omodei Nicola, Oppedisano Chiara, Papitto Alessandro, Pavlov George G., Peirson Abel L., Perri Matteo, Pesce-Rollins Melissa, Petrucci Pierre-Olivier, Possenti Andrea, Poutanen Juri, Puccetti Simonetta, Ramsey Brian D., Ratheesh Ajay, Roberts Oliver J., Sgrò Carmelo, Slane Patrick, Spandre Gloria, Swartz Douglas A., Tamagawa Toru, Tavecchio Fabrizio, Taverna Roberto, Tawara Yuzuru, Tennant Allyn F., Thomas Nicholas E., Tombesi Francesco, Trois Alessio, Tsygankov Sergey S., Turolla Roberto, Vink Jacco, Wu Kinwah, Zane Silvia, (IXPE Collaboration), Wadiasingh Zorawar, Ho Wynn C. G., Harding Alice K., Gendreau Keith C., Arzoumanian Zaven
(Refereed journal article or data article (A1))

The metamorphosis of the Type Ib SN 2019yvr: late-time interaction (2024)

Monthly Notices of the Royal Astronomical Society: Letters
Ferrari Lucía, Folatelli Gastón, Kuncarayakti Hanindyo, Stritzinger Maximilian, Maeda Keiichi, Bersten Melina, Román Aguilar Lili M, Sáez M Manuela, Dessart Luc, Lundqvist Peter, Mazzali Paolo, Nagao Takashi, Ashall Chris, Bose Subhash, Brennan Seán J, Cai Yongzhi, Handberg Rasmus, Holmbo Simon, Karamehmetoglu Emir, Pastorello Andrea, Reguitti Andrea, Anderson Joseph, Chen Ting-Wan, Galbany Lluís, Gromadzki Mariusz, Gutiérrez Claudia P, Inserra Cosimo, Kankare Erkki, Müller Bravo Tomás E, Mattila Seppo, Nicholl Matt, Pignata Giuliano, Sollerman Jesper, Srivastav Shubham, Young David R
(Refereed journal article or data article (A1))

First Sagittarius A* Event Horizon Telescope Results. VII. Polarization of the Ring (2024)

Astrophysical Journal Letters
Akiyama K, Alberdi A, Alef W, Algaba JC, Anantua R, Asada K, Azulay R, Bach U, Baczko A, Ball D, Balokovic M, Bandyopadhyay B, Barrett J, Bauböck M, Benson BA, Bintley D, Blackburn L, Blundell R, Bouman KL, Bower GC, Boyce H, Bremer M, Brinkerink CD, Brissenden R, Britzen S, Broderick AE, Broguiere D, Bronzwaer T, Bustamante S, Byun D, Carlstrom JE, Ceccobello C, Chael A, Chan C, Chang DO, Chatterjee K, Chatterjee S, Chen M, Chen Y, Cheng X, Cho I, Christian P, Conroy NS, Conway JE, Cordes JM, Crawford TM, Crew GB, Cruz-Osorio A, Cui Y, Dahale R, Davelaar J, Laurentis MD, Deane R, Dempsey J, Desvignes G, Dexter J, Dhruv V, Dihingia IK, Doeleman SS, Dougal ST, Dzib SA, Eatough RP, Emami R, Falcke H, Farah J, Fish VL, Fomalont E, Ford HA, Foschi M, Fraga-Encinas R, Freeman WT, Friberg P, Fromm CM, Fuentes A, Galison P, Gammie CF, García R, Gentaz O, Georgiev B, Goddi C, Gold R, Gómez-Ruiz AI, Gómez JL, Gu M, Gurwell M, Hada K, Haggard D, Haworth K, Hecht MH, Hesper R, Heumann D, Ho LC, Ho P, Honma M, Huang CL, Huang L, Hughes DH, Ikeda S, Impellizzeri CMV, Inoue M, Issaoun S, James DJ, Jannuzi BT, Janssen M, Jeter B, Jiang W, Jiménez-Rosales A, Johnson MD, Jorstad S, Joshi AV, Jung T, Karami M, Karuppusamy R, Kawashima T, Keating GK, Kettenis M, Kim D, Kim J, Kim J, Kim J, Kino M, Koay JY, Kocherlakota P, Kofuji Y, Koch PM, Koyama S, Kramer C, Kramer JA, Kramer M, Krichbaum TP, Kuo C, Bella NL, Lauer TR, Lee D, Lee S, Leung PK, Levis A, Li Z, Lico R, Lindahl G, Lindqvist M, Lisakov M, Liu J, Liu K, Liuzzo E, Lo W, Lobanov AP, Loinard L, Lonsdale CJ, Lowitz AE, Lu R, MacDonald NR, Mao J, Marchili N, Markoff S, Marrone DP, Marscher AP, Martí-Vidal I, Matsushita S, Matthews LD, Medeiros L, Menten KM, Michalik D, Mizuno I, Mizuno Y, Moran JM, Moriyama K, Moscibrodzka M, Mulaudzi W, Müller C, Müller H, Mus A, Musoke G, Myserlis I, Nadolski A, Nagai H, Nagar NM, Nakamura M, Narayanan G, Natarajan I, Nathanail A, Fuentes SN, Neilsen J, Neri R, Ni C, Noutsos A, Nowak MA, Oh J, Okino H, Olivares H, Ortiz-León GN, Oyama T, Özel F, Palumbo DCM, Paraschos GF, Park J, Parsons H, Patel N, Pen U, Pesce DW, Piétu V, Plambeck R, PopStefanija A, Porth O, Pötzl FM, Prather B, Preciado-López JA, Psaltis D, Pu H, Ramakrishnan V, Rao R, Rawlings MG, Raymond AW, Rezzolla L, Ricarte A, Ripperda B, Roelofs F, Rogers A, Romero-Cañizales C, Ros E, Roshanineshat A, Rottmann H, Roy AL, Ruiz I, Ruszczyk C, Rygl KLJ, Sánchez S, Sánchez-Argüelles D, Sánchez-Portal M, Sasada M, Satapathy K, Savolainen T, Schloerb FP, Schonfeld J, Schuster K, Shao L, Shen Z, Small D, Sohn BW, SooHoo J, Salas LDS, Souccar K, Stanway JS, Sun H, Tazaki F, Tetarenko AJ, Tiede P, Tilanus RPJ, Titus M, Torne P, Toscano T, Traianou E, Trent T, Trippe S, Turk M, Bemmel I, Langevelde HJ, Rossum DR, Vos J, Wagner J, Ward-Thompson D, Wardle J, Washington JE, Weintroub J, Wharton R, Wielgus M, Wiik K, Witzel G, Wondrak MF, Wong GN, Wu Q, Yadlapalli N, Yamaguchi P, Yfantis A, Yoon D, Young A, Young K, Younsi Z, Yu W, Yuan F, Yuan Y, Zensus JA, Zhang S, Zhao G, Zhao S; Event Horizon Telescope Collaboration
(Refereed journal article or data article (A1))

Intermediate-luminosity Type IIP SN 2021gmj : a low-energy explosion with signatures of circumstellar material (2024)

Monthly Notices of the Royal Astronomical Society
Murai Yuta, Tanaka Masaomi, Kawabata Miho, Taguchi Kenta, Teja Rishabh Singh, Nakaoka Tatsuya, Maeda Keiichi, Kawabata Koji S, Nagao Takashi, Moriya Takashi J, Sahu D K, Anupama G C, Tominaga Nozomu, Morokuma Tomoki, Imazawa Ryo, Inutsuka Satoko, Isogai Keisuke, Kasuga Toshihiro, Kobayashi Naoto, Kondo Sohei, Maehara Hiroyuki, Mori Yuki, Niino Yuu, Ogawa Mao, Ohsawa Ryou, Okumura Shin-ichiro, Saito Sei, Sako Shigeyuki, Takahashi Hidenori, Uno Kohki, Yamanaka Masayuki
(Refereed journal article or data article (A1))