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PhD and Postdoctoral positions at GRAPPA University of Amsterdam

We invite applications for one or more in general relativity, gravitational wave astrophysics, and dark matter phenomenology, funded by the ERC Advanced Grant “De Tenebris” (PI: Prof. Gianfranco Bertone) and hosted at GRAPPA, University of Amsterdam. Application deadline: December 1st, 2025.

PhD positions — Apply via AcademicJobsOnline (#30677):
https://academicjobsonline.org/ajo/jobs/30677

Postdoctoral positions — Apply via AcademicJobsOnline (#30676):
https://academicjobsonline.org/ajo/jobs/30676

GRAPPA is the center of excellence in gravitation and astroparticle physics at the University of Amsterdam, located at Amsterdam Science Park. We offer a vibrant research environment with strong ties to major experimental collaborations (including LIGO/Virgo/KAGRA, LISA, and Einstein Telescope).

The successful candidates will have the opportunity to collaborate with GRAPPA faculty (S. Ando, D. Baumann, G. Bertone, P. Decowski, B. Freivogel, A. Heijboer, S. Markoff, P. Moesta, S. Nissanke, J. Vink, A. Watts, C. Weniger), postdocs, and students, as well as with external partners in the broader gravitational waves and dark matter communities.

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

Postdoctoral Position on Extreme Mass Ratio Inspirals and QPEs in Leiden

Leiden Observatory invites applications for a postdoctoral position on theoretical and computational astrophysical studies of gravitational wave-related phenomena, with a strong preference for Extreme Mass Ratio Inspirals (EMRIs), and Quasi-Periodic Eruptions (QPEs). The postdoctoral position is within Prof. Elena M. Rossi’s group, which currently consists of five PhD students and one post-doc, who work on various galactic nuclei phenomena. It is funded by Rossi’s grant awarded within the National Roadmap for the Laser Interferometer Space Antenna (LISA). This consortium coordinates activities in the Netherlands in preparation for LISA data.

The position is for 2+2 years, and preferentially targets candidates straight out of their PhD.

Leiden Observatory, founded in 1633, is the oldest university astronomy department in the world. It is ranked the 7th best Space Science Department in the world, and the first outside the USA. With about 35 faculty, over 60 postdoctoral associates and about 80 PhD students, it is one of the largest and most international astronomy departments in the world. Leiden is a charming university town with an international flair. Most English is the common language at the Institute and in town.

Compensation and Benefits

The positions include all employees’ benefits, including but not limited to parental leave, holiday bonus, retirement benefits, etc

Application Details

Applicants are requested to send an email to emr(at)strw.leidenuniv.nl, attaching their CV, list of publications (link to a website is also ok), cover letter (important!) and a maximum of one page of research experience and plans. The email subject should be: “your surname_LISA_application. All files must contain in the title your surname (e.g., Rossi_CV, Rossi_cover_letter, etc..). Please, arrange to have three letters of reference to be emailed to emr@strw.leidenuniv.nl with the application deadline, with subject “your surname reference LISA position” (e.g., Rossi reference LISA position) and the pdf file of the letter should be named “your surname_surname-of-letter-writer” (e.g., “Rossi_UgoFoscolo”).

The successful candidate must have a PhD degree by the starting date. The starting date is 1st of September 2026, but an earlier start is possible.

Complete applications received by November 15, 2025, will receive full consideration.

Inquiries
Elena Maria Rossi emr(at)strw.leidenuniv.nl

Please find here details.

Postdoc Positions at the University of Chicago

Multiple postdoctoral positions in gravitational-wave science, as well as general relativity, astrophysics, and cosmology more broadly, are available at UChicago. 

Of particular interest to the LIGO/GW community may be the KICP, Fermi, Schmidt, SkAI, and Leinweber Fellowships. UChicago is a member of SkAI and the Simons Collaboration on Black Holes and Strong Gravity. Please contact Daniel Holz with questions.

Postdoctoral fellowships in gravitational physics and gravitational-wave astronomy at Johns Hopkins University

The William H. Miller III Department of Physics and Astronomy at Johns Hopkins University invites applications for postdoctoral fellowships in the general area of gravitational physics and gravitational-wave astronomy. These fellowships offer the opportunity for postdoctoral research that combines academic freedom with strong faculty mentorship in an intellectually vibrant, inclusive, and welcoming department. The Department has strong programs in condensed-matter physics, particle physics, astrophysics, and biological physics and is embarking upon a significant expansion, including growth into new areas of physics. The department also benefits from its close relationship with the Space Telescope Science Institute, located on the Johns Hopkins campus.

The candidates are expected to work in my research group (https://pages.jh.edu/eberti2/about/). The group currently includes 6 postdocs, 7 Ph.D. students, and various undergraduate students supported by grants from the National Science Foundation, NASA, the John Templeton Foundation, the Simons Foundation, and the Italian Ministry of Foreign Affairs and International Cooperation. The postdoctoral fellows will be provided with support for travel across the nodes of the recently established Simons Collaboration on Black holes and Strong Gravity (SimonsC-BHSG). The Department of Physics and Astronomy at Johns Hopkins University has a vibrant and interdisciplinary research environment, and the candidates are encouraged to collaborate with other faculty members, students and postdocs working in closely related research areas. More details about the department and its research can be found at https://physics-astronomy.jhu.edu

Consideration of applications will begin on 1 December 2025 and continue until all available positions are filled. Applicants should submit a curriculum vitae, a statement of research interests, and a list of publications, and arrange for at least three letters of reference on their behalf to be submitted to the application website:

https://academicjobsonline.org/ajo/jobs/30711

Postdoctoral and Assistant Professor Fellowships in Gravitational Physics at NBI Copenhagen

The Center of Gravity at the Niels Bohr Institute invites expressions of interest for Postdoctoral Fellowships in multiple fields related to Gravitational Physics and Gravitational Wave Astrophysics for a fixed period of up to four (3+1) years. Exceptional and highly motivated individuals will also be considered for 5-year Assistant Professorships. The preferred starting date is Fall 2026. Application deadline November 15th 2025.

Postdoctoral Fellows and Assistant Professors at the Center of Gravity at the Niels Bohr Institute have the opportunity to guide more junior fellows, teach courses at various levels, participate in outreach activities, and organize international meetings. Interested individuals are encouraged to upload all material before November 15th, 2025. The search will remain open until completed.

We seek international outstanding individuals eager to join an ambitious research program addressing the physics of black holes, gravitational motion using both advanced quantum field scattering and gravitational self-force techniques, black hole spectroscopy, quantum aspects of spacetime via string theory and holography, and the effect of environments in gravitational wave physics. It further includes the exploration of black holes as engines of discovery, including implications for dark matter physics and connections to particle physics. However, outstanding individuals in complementary fields are also warmly welcomed to upload their material.

This search is part of a vigorous expansion at the Niels Bohr Institute into the field of Gravitational Physics, bringing together several scientists from several areas of theoretical physics and astrophysics, and addressing some of the most burning questions related to gravity. More information can be found on the website: https://the-center-of-gravity.com/

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.

The University of Copenhagen wishes to reflect the diversity of society and welcomes all qualified individuals regardless of personal background. Postdoctoral Fellows 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. A favorable tax scheme is generally granted to international researchers.

Please find here full details.

Call of interest for postdocs at SISSA, Trieste

The gravitational-wave physics group at SISSA (Trieste, Italy) invites expressions of interest for several postdoctoral research positions on the following topics: numerical-relativity simulations; environmental effects for binary systems; gravitational-wave data analysis and machine learning; waveform modeling. The positions will start in the fall of 2026 and will be for two years, with possible extension conditional on satisfactory performance. These positions will be part of the GWSKy ERC synergy project.

Applications should consist of a cover letter, a CV, a publication list, a research statement and three reference letters, and should be received by December 19th to receive full consideration.

Application Materials Required:
Submit the following items online at this website to complete your application:

  • Cover letter
  • Curriculum Vitae
  • Research statement
  • Publication list
  • Three reference letters (to be submitted online by the reference writers on this site help popup)

And anything else requested in the position description.

Please find here details.

ETpathfinder Visiting Scientists Programme Open For Applications

The ETpathfinder Visiting Scientists Programme provides funding to welcome researchers and engineers to our ETpathfinder R&D facility in Maastricht, the Netherlands. This program is designed for senior scientists and engineers, postdoctoral researchers and experienced PhD students who wish to engage with cutting-edge interferometric technology while contributing their expertise to advance our experimental capabilities.

ETpathfinder serves as a R&D fieldlab facility for developing technologies that will enable future -generation gravitational wave detectors, such as Einstein Telescope. Our research focuses on high-precision interferometry with cryogenic silicon test masses, seismic isolation systems, optics, photonics, quantum noise reduction, controls and environmental monitoring as well as on engineering, systems engineering, integration and cleanliness aspects.

For any questions or enquiries, please contact us via etpf-visiting-scientist-prog(at)nikhef.nl

Applications can be submitted via this webpage.

Postdoctoral positions in Gravitational-Wave Physics and Astrophysics at the Max Planck Institute for Gravitational Physics in Potsdam

The "Astrophysical and Cosmological Relativity" (ACR) department at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute, AEI) in Potsdam announces the opening of several postdoctoral appointments, which will be available at different levels, depending on experience and seniority, and can last from 2 to 5 years. We also have openings as part of the ERC-Synergy Grant  “Making Sense of the Unexpected in the Gravitational-Wave Sky”, one opening as part of the Simons Collaboration on Black Holes and Strong Gravity, and one opening for a postdoctoral position as part of the Center of Gravity. For the latter, the successful candidate will spend the first two years at the AEI and the subsequent two years at the Niels Bohr Institute in Copenhagen. The ACR department also offers Max Planck Fellowships to non-German scientists. Information on those fellowships and explanations on how to apply are summarized here. We are particularly interested in hiring creative and highly motivated candidates who are at ease working both collaboratively and independently in a vibrant, interdisciplinary, and synergistic group.

The ACR department, led by Alessandra Buonanno, is composed of about 45 scientists, including three permanent research group leaders, Jonathan Gair, Harald Pfeiffer and Jan Steinhoff, and the five-year research group leader Miguel Zumalacarregui. The department also hosts several long and short-term visitors, and has ties with the Physics Department at the University of Maryland, the Humboldt University in Berlin, and the University of Potsdam.

The ACR department is interested in  many aspects of gravitational-wave astronomy, including (i) analytical modeling of gravitational dynamics and radiation (effective field theory, post-Newtonian and post-Minkowskian expansions, gravitational self-force approach, perturbation theory and effective-one-body formalism), (ii) numerical relativity, most notably simulations in vacuum of compact objects on bound and unbound orbits in general relativity and alternative gravity theories, (iii) observation (including searches and detector characterization) and interpretation of data from gravitational-wave detectors on the ground (LIGO, Virgo, KAGRA, Cosmic Explorer, Einstein Telescope) and in space (LISA), (iv)  techniques for the acceleration of gravitational-wave inference, including machine learning, (v) astrophysics of compact objects and bi-nary’s formation scenarios, (vi) cosmography with gravitational waves (including dark energy, dark matter, gravitational lensing), and (vii) tests of gravity in the strong-field and highly dynamical regimes.

The ACR department participates in many international collaborations: the Simulating extreme Spacetimes Collaboration (SXS), the LIGO Scientific Collaboration (LSC),  the Einstein Telescope (ET) Collaboration, the LISA Consortium, and the LISA Distributed Data Processing Centre (DDPC), where our department plays a leading role in waveform generation and the global fit deep analysis.

Currently, the ACR department operates a high-performance compute cluster, Urania, with ~6,050 cores, a high-throughput compute cluster, Hypatia, with ~12,000 cores, and two servers, Saraswati and Lakshmi, each with 8 A100 GPUs. Those clusters are in the process of being extended. They are used to run numerical-relativity simulations of gravitational-wave sources, and to carry out source modeling and data-analysis studies for current and future gravitational-wave detectors.

To apply, please submit your application via our job portal here.

You will be asked to upload a cover letter, curriculum vitae, list of publications and a statement of past and future research activities of not more than 3 pages (excluding references). Applicants will need to indicate the names of three referees for recommendation letters. Please register an account with our job portal and fill in the contact information for the referees well before the deadline, so that reference letters can be received in time. Referees will receive an email with instructions on how to upload their letters. In case of technical problems with the application form, please contact jobs @ aei.mpg.de.

Candidates are encouraged to apply as soon as possible. The deadline for full consideration is November 25, 2025, including reception of reference letters. The anticipated start date of the positions is Fall 2026. Applications will be considered until all positions are filled.

The salary and social benefits (e.g. health insurance) are based on the collective labor agreement “TVöD Bund” for the German public sector, usually at pay grade E13 (if the qualifications according to TVöD are met). A projection of the gross and net salary based on the TVöD regulations will be prepared in case an offer is made.

The Max Planck Institute for Gravitational Physics is an equal opportunity employer, and is committed to provide employment opportunities to all qualified applicants without regard to race, color, religion, age, gender identity, sexual orientation or national origin. The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and therefore encourages applications from such qualified individual. The AEI and the Max Planck Society welcome persons with diverse backgrounds, experiences, and ideas who embrace and value diversity and inclusion (Code of Conduct). The institute promotes a healthy work-life balance by offering all employees a family support service, cooperation with a nearby international kindergarten, as well as an in-house parent-child office and nursing room.

For further information please contact acr-jobs @ aei.mpg.de.

Please find here details.

Weinberg fellowships in gravitation, multi-messenger astrophysics and AI/ML

The Center for Gravitational Physics (CGP) within the Weinberg Institute at the University of Texas at Austin invites applicants for multiple Weinberg Institute Postdoctoral Fellowships. These are full-time postdoctoral positions starting in September 2026.

This position is open to candidates in gravitational-wave physics, astrophysics and data analysis, especially in (but not limited to) the areas of:

(1) Cosmological inference with gravitational-wave observations
(2) Applications of AI/ML techniques broadly to astrophysics, cosmology or gravitational wave data analysis
(3) Nuclear astrophysics with gravitational-wave observations
(4) Gravitational-wave multimessenger astrophysics
(5) Numerical simulations of compact binaries

Applicants must submit a cover letter (no more than 1 page), CV, list of publications, a short statement of research interests (no more than 3 pages in length) and arrange to have at least three letters of reference uploaded to AJO. Applications are due November 21, 2025. The completion of a PhD is required prior to the beginning of this appointment. The initial appointment is for two years, with the possibility of extension to a third year subject to available funding and research performance.

Inquiries may be sent to Profs. Hsin-Yu Chen (hsinyu(at)austin.utexas.edu) or Jay Wadekar (jay.wadekar(at)utexas.edu).

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. 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@cosmos.esa.int.

The next deadline for applications is Monday 10 November 2025, 23:59 UTC

Call for applications

Applications can be submitted at any time by sending email to arvp(at)cosmos.esa.int. The email should contain a single PDF document of at most three pages detailing:

  • description of the goals of the research project
  • public archival data on which help is sought
  • which type of expertise you expect to gain
  • proposed time and duration of the visit
  • expected publications
  • contact information

Please keep it short (max 3 pages) and follow the simple template provided here. Note that this is just a template, you can use the font type and size that you prefer (not smaller than 10), but please do not exceed three pages. You must indicate the (expected) year of your PhD.

To prevent unconscious biases, your name, email address, and other contact information (on the third page) will not be visible to reviewers. To help in the process, you must write your application in an “anonymous” way, i.e. do not identify yourself in the text. For instance, do not mention the name of your institute or collaborators in the scientific description of the project (page 1 and 2) and when you are referring to one of your papers, do not write “I have shown that … (Author Name, 2023, Journal, 954, 125)”, but rather write “It has been shown that … (Author Name, 2023, Journal, 954, 125)”. If you identify yourself, the application will not be considered.

We encourage you to contact us if you have any questions about the data that could support your research project. You will find the names of our experts in the various science areas in the table of expertise below. Or write to the programme coordinators for assistance at arvp(at)cosmos.esa.int.

Students

We welcome proposals by graduate students. The proposals can be submitted by the students themselves or in collaboration with their supervisors. If you are a student and would like to visit ESA to learn more about doing science with archival data, make sure that you coordinate and agree your research project with your supervisor. Mention this in the application, but omit the name of the supervisor, otherwise the application is not anonymous.

Deadlines

Applications can be submitted at any time and are reviewed twice a year, with deadlines usually on 30 April and 31 October. The results of the review will be communicated to applicants within about two months of the deadlines. Applicants are encouraged to contact the ESA scientists or the programme coordinators well ahead of the deadlines in order to discuss their research plans.

Applications received by 10 November 2025 (23:59 UTC) will be considered for visits in spring and summer 2026.

Please find here full details.