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Postdoctoral position in Quantum Gravity, Cosmology, and AI for Science in Annecy

The Laboratoire d’Annecy de Physique Théorique (LAPTh, CNRS/Univ. Savoie Mont Blanc) invites applications for one postdoctoral position in theoretical physics, with research opportunities in quantum gravity, cosmology, and AI for Science, and additional connections to the Physics of Learning.

The main project investigates connections between fundamental theory and cosmology, with particular interest in accelerated expansion and the origin of dark energy within string theory and M-theory. It combines analytical approaches with the application and development of Machine Learning methods for solving the equations of motion governing compactifications.

There will also be opportunities to work on the Physics of Learning, whether to understand and improve learning algorithms in their own right or to feed back into the physics applications, using methods from physics to study, for example, the dynamics of optimization and sampling, the theory of neural networks, and neural scaling laws. The successful candidate will be encouraged to develop their own independent research program alongside collaborative work within the project.

Qualifications: Applicants must hold, or expect to obtain by the starting date, a PhD in theoretical physics or a closely related field. We welcome candidates with a strong theoretical physics background and research interests relevant to one or more of the project’s directions. Experience with AI and machine learning is welcome but not required. Knowledge of French is not required.

Research Environment: The successful candidate will join the Mathematical Physics group at LAPTh and work with Dr. G. Bruno De Luca. A PhD student will be recruited at the same time, offering the opportunity to contribute to their supervision and help develop a growing research team.

The project is funded by the Multidisciplinary Institute for Artificial Intelligence (MIAI Cluster), offering interactions with researchers in fundamental physics, mathematics and AI. Existing contacts with researchers in the Simons Collaboration on the Physics of Learning provide further opportunities for scientific exchange. The position provides dedicated computing resources and support for conferences and research visits. The laboratory is located in Annecy, in the French Alps, about 45 km from Geneva, with proximity to CERN offering further opportunities for exchange and collaboration.

Terms of Employment: The appointment is for three years, with an anticipated start date in September 2027 and some flexibility possible. Salary will follow the USMB scale and be commensurate with experience. The appointment includes the usual social benefits.

Application Procedure: Interested candidates are invited to apply in English via AcademicJobsOnline, including:

(i) a cover letter;
(ii) a CV with a list of publications;
(iii) a research statement describing past work and future research interests;
(iv) at least three recommendation letters submitted directly by the referees.

Applications, including recommendation letters, received by 18 December 2026 will receive full consideration. The position will remain open until filled. Shortlisted candidates will be invited to a remote interview.

Please find here details.

Particle Physics Beyond the Standard Model at Colliders and in Gravitational-Wave Observations at NICPB Tallinn

The Laboratory of High Energy and Computational Physics (HEPC) at NICPB, Tallinn, invites applications for a fully funded PhD position in theoretical particle physics. The doctoral degree will be awarded by Tallinn University of Technology (TalTech). The position has just become available, so we aim to fill it as soon as possible. Applications will be reviewed on arrival, and an early start is strongly preferred. The position offers a competitive salary for the full duration of four academic years. Application deadline: November 30th 2026.

The project focuses on BSM model building and phenomenology, addressing the flavour puzzle, neutrino masses and dark matter. This work will link new physics testable at colliders to phase-transition gravitational-wave signals at LISA and ET. The ideal candidate has a strong background in quantum field theory and an interest in BSM phenomenology.

The PhD will be supervised by Dr. Carlo Marzo, with co-supervision by Dr. Ville Vaskonen. HEPC has more than 20 members and is part of the CMS collaboration, the ET collaboration and the LISA consortium. Its research spans collider physics, dark matter, cosmology and gravitational-wave phenomenology. Funding is available for participation in international schools and conferences.

Requirements: A Master’s degree in Physics and fluency in English. Applicants should submit a CV, academic transcripts and at least one reference letter.

Contact
Letters of Reference should be sent to: carlo.marzo(at)taltech.ee

Please find here details.

PhD Positions in GW Astrophysics & Dark Matter at GRAPPA (UvA)

GRAPPA invites applications for one or more PhD positions to work at the interface of general relativity, gravitational wave astrophysics, and dark matter phenomenology within the ERC Advanced Grant “De Tenebris,” led by Prof. G. Bertone.

The PhD candidate will develop and apply theoretical and computational models for compact binaries in astrophysical/dark matter environments and contribute to the interpretation of current and future gravitational wave observations (LISA and next-generation ground-based detectors). The position is embedded in a collaborative team with strong ties to the international gravitational wave and dark matter communities.

We are looking for candidates who: – will have completed an MSc in Physics, Astronomy, or a closely related field by the start date; – have a solid grounding in general relativity and/or gravitational wave astrophysics; – have experience in scientific programming (e.g., Python or C++); – can communicate clearly in English and enjoy working in a collaborative research environment. It is a plus—not a requirement—if you are familiar with cosmological or N-body simulations, gravitational wave data analysis, or dark matter phenomenology.

GRAPPA is the center of excellence in gravitation, astroparticle physics, and cosmology at the University of Amsterdam, located at Amsterdam Science Park, with a lively seminar culture and close connections to the LIGO/Virgo/KAGRA, LISA, and Einstein Telescope collaborations.

The University of Amsterdam is an equal-opportunity employer. We are committed to building a diverse, inclusive community and welcome applications from all qualified candidates.

How to apply

Applications should be submitted via AcademicJobsOnline. Please include:

  • a cover letter;
  • your CV, including a list of publications (if any);
  • a brief statement of research interests;
  • two letters of recommendation.

The expected start date is between Spring and Fall 2027. Application Deadline: 1 December 2026.

Please find here details.

The Center of Gravity: Exchange of researchers working on gravitational physics

Grants for short term scientific missions (STSMs) are available to visit and work on research projects within the Center of Gravity (CoG), a DNRF Center of Excellence at the Niels Bohr Institute and at the AEI Astrophysical and Cosmological Relativity Department (ACR), a partner of CoG.

We are inviting you to submit proposals for STMSs starting after April, 2027 and ending before October 1, 2027 (applications outside this timeframe will be discarded). We are looking for exciting and challenging research proposals to be developed jointly with our members. We value high risk/high gain proposals at the boundary between different research directions within CoG.

STSMs are a great opportunity for all scientists within the community to exchange visits, nurture collaborations, or develop new ones.

This call starts on October 1 and closes November 30, 2026. All proposals will be reviewed and the results will be announced by January 1, 2027. The selection committee will take into account the matching of funds by the Home Institution, gender diversity, the scientific proposal and the experience of the applicant (preference is given to Early Career Investigators).

A STSM application should include

  1. Name and contact of applicant and name of CoG or ACR member with whom the visit was discussed
  2. A single pdf with:
  • proposal title
  • brief CV of the applicant (2 pages)
  • short description of the proposed project work (1 page max) 
  • motivation letter (1 page max)
  • Estimate and breakup of the financial request (specify if the Home Institution will provide matching funds). Typical STSMs lasts between 1- 6 weeks.
  • A support letter from the Home Institution

Applications should be made following this link: https://the-center-of-gravity.com/join-us/

We encourage all applicants to apply for funding or co-funding to visit the CoG and /or the ACR department with either their home institute, the Simons Collaborative Grant on Black Holes and Strong Gravity, or one of the following COST Actions CA23130, CA23115, CA22113, CA22113, CA21136.

For the successful applicants, The Center of Gravity (and the AEI Astrophysical and Cosmological Relativity Department, if the visit is at the AEI) will cover economy-class flights, train, or bus tickets and provide hotel accommodation near the Institutes during part or for the full stay.  Details will be provided upon acceptance. After the STSM, the grantee is required to submit a short scientific report (one page max). The report should contain the purpose of the STSM, a description of the work carried out during the STSM, a description of the main results and other comments (if any).

Contact: Nils Siemonsen, nils.siemonsen(at)nbi.ku.dk

STSM recipients should acknowledge the Center of Gravity, through the statement “The authors would like to acknowledge networking support by the Center of Gravity, a Center of Excellence funded by the Danish National Research Foundation under grant No. DNRF184.”

The Center of Gravity is now a partner of the AEI Astrophysical and Cosmological Relativity Department. We accept STMSs for either institute, and value science proposals that involve scientists in both.

Please find here details.

PhD positions at the Center of Gravity, Copenhagen

The Center of Gravity at the Niels Bohr Institute (NBI) invites expressions of interest for a PhD fellowship in gravitational-wave theory and solutions to the relativistic 2-body problem under the supervision of Maarten van de Meent. The preferred starting date is Fall 2027. To receive full consideration, interested candidates should upload the material requested below before December 15th, 2026. The search will remain open until the optimal candidates are found.

Successful candidates will join the GWSKy project, funded by an ERC Synergy Grant. We are particularly interested in hiring creative and highly motivated candidates who can work collaboratively in a vibrant, welcoming, and synergistic group. The ERC-funded project called “Making sense of the unexpected in the gravitational-wave sky (GWSky)” is led by PIs Maarten van de Meent (NBI, Copenhagen, Denmark), Enrico Barausse (SISSA, Trieste, Italy), Zvi Bern (University of California, Los Angeles, US), and Alessandra Buonanno (Albert Einstein Institute, Potsdam). Given the synergistic aspect of the GWSky project, we anticipate the possibility of PhD students having a co-supervisor at one of the other nodes, and for them having the opportunity to have extended visits there.

The aim of the GWSky project is to use gravitational-wave measurements by existing and future observatories on the Earth and in space as precision laboratories for fundamental physics, cosmology, and astrophysics. This includes the current LIGO-Virgo-KAGRA detectors, as well as the future ground-based observatories Cosmic Explorer and Einstein Telescope, and the space-based detector LISA. By leveraging the PIs and their team’s expertise, the GWSky project aims to develop a groundbreaking framework capable of solving the highly nonlinear equations of Einstein’s General theory of Relativity, creating waveform models with unprecedented accuracy, and translating these results into practical tools for interpreting the data.

More information can be found on the website: https://gwsky.org/

Possible topics include: development of gravitational self-force methods at second order in the mass-ratio; incorporation of environmental and/or beyond GR effects in the self-force formalism; and utilization of self-force data to enhance effective-one-body waveform models.

The Center of Gravity (CoG) is a center for new ideas about the foundations of physics. We bring together cutting-edge research in observations of black holes and in the formal theory of relativistic and quantum aspects of gravity, completing the visions of Bohr and Einstein for the gravitational interaction. Our research endeavor spans from data analysis to theoretical disciplines within astrophysics and high-energy physics, and we aim to drive gravitational-wave physics to an exciting future. We have our physical home in the beautiful and legendary building at Blegdamsvej 17, established by Niels Bohr. This is the place where quantum theory was born and where many exciting new developments in gravity are now taking place. Today, the Niels Bohr Institute carries an important legacy in physics and is one of the leading institutes in theoretical and experimental physics. At the Center of Gravity, we hope to carry on the pioneering spirit that has defined our predecessors at the Niels Bohr Institute through trailblazing and fundamental research. More information can be found on the website: https://the-center-of-gravity.com/ The University of Copenhagen wishes to reflect the diversity of society and welcomes expressions of interest from all qualified candidates regardless of personal background. PhD students at the University of Copenhagen receive a competitive salary (including pension) and funds for travel and computing. Generous parental leave, state-subsidized childcare, vacation, and full medical care are provided to employees in Denmark.

For any inquiries, kindly send an email to Maarten.Meent(at)nbi.ku.dk, with email subject “PhD Fellowship in Gravitational Self-Force”

Please find here full details and how to apply.

PhD Position: Search for quantization of space-time with photon counting interferometry in Cardiff

The Gravity Exploration Institute at Cardiff University has an open PhD position in gravitational-wave and fundamental physics instrumentation. The post will initially be focused on developing of a new optical readout scheme for laser interferometry, that uses photon counting instead of continuous-wave photodetection. The work will be developed in context with our world-leading table-top experiment, and is being funded by an ERC advanced grant.

Please talk to Prof. Hartmut Grote if you have further questions. Closing date for the application is 30 October 2026.

Please find here details.

PhD Fellowship in Gravitational Physics at NBI Copenhagen

The Center of Gravity at the Niels Bohr Institute invites expressions of interest for PhD Fellowships in Gravitational Physics for a fixed period of three years. The preferred starting date is April-September 2027. Interested individuals are encouraged to upload all material before December 1, 2026, by submitting a 2-page CV, transcripts, and a one-page letter of motivation. In addition, we are requesting (at least) two letters of recommendation. The search will remain open until completed.

We seek international outstanding individuals eager to join Center of Gravity, a center bringing together cutting-edge research on formal and phenomenological aspects of black holes and gravitational waves, as well as related fundamental research areas.

This call is seeking specifically outstanding candidates for an ambitious research program on quantum aspects of black holes and spacetime via string theory and holography. The research program is an integral part of the Center of Gravity, a new DNRF Center of Excellence initiative which is composed of the young and vibrant team consisting of Vitor Cardoso, Emil Bjerrum-Bohr, Jose Ezquiaga, Troels Harmark, Niels Obers, Marta Orselli, Alessia Platania, Johan Samsing, Maarten van de Meent, Ziqi Yan, focused on addressing the physics of black holes, quantum aspects of spacetime via string theory and holography, the problem of motion in General Relativity using advanced quantum field scattering and gravitational self-force techniques, and gravitational-wave physics. An ample travel budget for the Center is available.

Brief interviews will be conducted with team members after an initial shortlist is formed. This search is part of a vigorous expansion at the Niels Bohr Institute into the field of Gravitational Physics, bringing together scientists from various areas of theoretical physics and astrophysics to address some of the most pressing questions related to gravity. The Center of Gravity is hosted by the Niels Bohr Institute. It functions as a primary center for fundamental research, including gravitational physics, theoretical and computational astrophysics, cosmology, and high-energy physics. The Center hosts several international programs, including visitor programs, workshops, and Ph.D. schools. The University of Copenhagen wishes to reflect the diversity of society and welcomes all qualified individuals regardless of personal background.

Please find here full details.

PhD positions at the International Max Planck Research School for Astronomy & Astrophysics, Bonn & Cologne

The International Max Planck Research School (IMPRS) for Astronomy & Astrophysics is a joint structured Ph.D. program of the Max Planck Institute for Radioastronomy (MPIfR, Bonn) and the Universities of Bonn and Cologne. At one of the most vibrant astronomy centers in Europe, several PhD positions are available for talented students nearing the end of their Master's degree (or equivalent) in physics or astrophysics. The teaching language is English. The application deadline is October 30th, 2026.

Program Details:

Appointments are for 3 years, starting at any time in 2027.

Starting annual gross salary: ~40617 Euro; with attractive benefits.

The IMPRS for A&A has 70+ Ph.D. students from 20+ countries.

Supervision by world-leading experts at the MPIfR and the Universities of Bonn and Cologne.

Research on a wide range of cutting-edge topics in observational and theoretical astrophysics.

Access to world-class observing facilities at a wide range of wavelengths. Career development workshops, advanced lecture courses, soft skill seminars. Funding for travel and research.

Remuneration is based on the German collective agreement for the public sector (TVöD-Bund or TVL), level 13, 65%, which includes comprehensive health care and other social benefits such as contributions to a pension fund, accident insurance, sick leave and 30 days of vacation per year. In addition, our school has special agreements with daycare providers and counselors, and offers German classes.

The Max Planck Society is committed to increasing diversity in its workforce and encourages applications from individuals with disabilities. The society also seeks to increase female representation in underrepresented areas and strongly encourages women to apply.

For more information visit: https://www.mpifr-bonn.mpg.de/en/imprs

Link to Online Application: https://imprs.mpifr-bonn.mpg.de

Publication Start Date: 2026 Sep 15

Application Deadline: 2026 Oct 30

Inquiries: IMPRS A&A Office, Email: imprs(at)mpifr-bonn.mpg.de

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25 PhD Positions in Astronomy and Astrophysics in Munich

The International Max Planck Research School (IMPRS) on Astrophysics at Ludwig Maximilian University (LMU) Munich invites applications for its international PhD program.

Located in the vibrant Munich–Garching science campus in southern Germany, the IMPRS offers a unique research environment through the close collaboration of four world-renowned institutions: MPI for Extraterrestrial Physics (MPE), University Observatory Munich, LMU (USM, MPI for Astrophysics (MPA), European Southern Observatory (ESO).

The IMPRS provides a highly competitive doctoral program that combines advanced lecture courses, seminars, and an independent research project leading to a PhD degree under the supervision of leading scientists at one of the participating institutions. The language of instruction is English.

The students have access to some of the world’s most powerful ground- and space-based observatories, state-of-the-art scientific instrumentation, and high-performance computing facilities for advanced numerical simulations and theoretical research. Applications are welcome from outstanding students of all nationalities. Application deadline: November 1st 2026.

Successful applicants receive either a fully funded employment contract or a fellowship providing financial support sufficient to cover living expenses in Munich. We also offer comprehensive assistance with visa procedures, relocation, accommodation, and all administrative matters to ensure a smooth start.

Please find here details and how to apply.

ESA – Archival Research Visitor Programme

To increase the scientific return from its space science missions, ESA welcomes applications from scientists interested in pursuing research based on publicly available data in the ESA Space Science Archives. The Archives host data from all current and past ESA space science missions in astronomy, planetary science, and heliophysics.

The ESA Archival Research Visitor Programme is open to scientists at all career levels who are affiliated with institutes in ESA Member States and Cooperating States (note that all visits must comply with the ESA Security Directives, which may necessitate additional checks). Early-career scientists are particularly encouraged to apply, including PhD students (see below). We encourage applications from women and minorities. The peer-review evaluation process is anonymised to ensure equal opportunities for all applicants.

Residence lasts typically between one and three months, also distributed over multiple visits, depending on the complexity of the research project. The research projects can be carried out at ESAC (Madrid, Spain) and at ESTEC (Noordwijk, Netherlands). To offset the expenses incurred by visitors, ESA covers travel costs from and to the home institution and provides support for lodging expenses and meals.

During their stay, visiting scientists have the opportunity to interact with archive and mission specialists for questions on the retrieval, calibration, and analysis of archival data. In principle, all areas of space research covered by ESA science missions can be supported (the data must be publicly available in the archives). To ensure that technical expertise in the specific area of interest is available at ESAC or ESTEC, applicants should consult the table of expertise and contact the relevant scientists in their field of interest (this is very important). In case of doubts, write to the programme coordinators for assistance at arvp(at)cosmos.esa.int.

The next deadline for applications is Saturday 31 October 2026, 23:59 UTC

Please find here full details.