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PhD position in Numerical Relativity in Jena

Applications are invited for a PhD position in Numerical Relativity at the Theoretical Physics Institute (TPI) FSU Jena, Germany.

The successful applicant will join the team led by Prof. Sebastiano Bernuzzi and work on numerical relativity simulations of neutron star mergers. The position is part of a cross-border project between Jena and Prof. David Radice’s group at Penn State University (USA). The project is funded by the Deutsche Forschungsgemeinschaft (DFG) and the US National Science Foundation (NSF) under the DFG-NSF Physics initiative. Candidates with background in numerical relativity, relativistic astrophysics and/or multi-messenger astrophysics with neutron star mergers are encouraged to apply. Application deadline: November 2nd 2025.

The application should be sent by e-mail to ‘sebastiano.bernuzzi[AT]uni-jena.de’ by November 2nd, 2025.
Review of the applications shall start immediately after that date; short-listed candidates will be invited for interviews.

Please submit a single PDF file and use as e-mail subject: ‘Application for PhD position – SURNAME NAME’.
Candidates should submit the following documents:

  1. a copy of their MSc diploma or a binding statement of its date of completion together with exam results,
  2. a CV including the list of publications,
  3. a short statement of research achievements and interests (maximum 2 pages).

Applicants should arrange for letters of recommendation to be sent directly to the same e-mail address above.

PhD positions at the International Helmholtz-Weizmann Research School on Multimessenger Astronomy

The school aims at bringing highly qualified and motivated graduate students to the forefront of the field of Multimessenger astronomy through a world-class international training environment. PhD students will work with leading scientists in the field and benefit from their complementary expertise in theory and experiments involving the various messengers. Application deadline November 7th, 2025.

Please finde here full details and how to apply.

PhD Program in Astronomy and Astrophysics at Leiden University

Leiden Observatory invites applications for approximately 6-10 new PhD positions. The four-year PhD program consists mostly of research under the supervision of one or more faculty members. Positions are available in most of the research areas in which the Observatory is active. These include galaxy formation and evolution, stars and planetary systems, computational astrophysics, high energy astrophysics, and instrumentation. More information about research at Leiden Observatory can be found here. Application deadline: November 15th, 2025.

Leiden Observatory, founded in 1633, is the oldest university astronomy department in the world. With about 35 faculty, over 40 postdoctoral associates and about 65 PhD students it is the largest astronomy department in the Netherlands. Leiden is a charming university town with an international flair. Most Leiden researchers have an international background. English is the common language.

During their thesis, Leiden PhD students are paid as civil servants, which means that they earn competitive salaries (the current annual gross salary, including allowances, increases from about EUR 37,000 in year 1 to about EUR 47,000 in year 4) and are eligible for both social security and retirement benefits. PhD positions are funded for four years.

Application forms and instructions are available at https://local.strw.leidenuniv.nl/jobs/phd/. Applicants are requested to upload a curriculum vitae, a list of all university courses taken and transcripts of grades obtained, brief statements of research interests and experience, and the contact information for at least two referees.

The successful candidates must have a MSc degree (or equivalent) by the starting date. The starting dates are negotiable.

Please find here full details.

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.

PhD Fellowships 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 (in particular black-hole and gravitational-wave physics) for a fixed period of three years. The preferred starting date is April-September 2026. Interested individuals are encouraged to upload all material before December 1, 2025, by submitting a 2-page CV, transcripts, and a one-page letter of motivation. 

The search will remain open until completed.

We seek international outstanding individuals eager to join an ambitious research program at 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 details.

PhD Position in Gravitational Waves Physics at IFAE Barcelona

IFAE is an internationally recognized center for fundamental research in Particle Physics, Astroparticle Physics, and Cosmology. Its main mission is to advance these fields through theoretical, experimental, and technological research. IFAE offers an international, dynamic, and competitive environment for the training of young researchers. IFAE has been accredited three times with the “Severo Ochoa Centre of Excellence” distinction, most recently for the 2025-2029 period.

About the IFAE Gravitational Waves group
The detection of GWs from a black hole binary merger by LIGO in 2015 started a new era in the exploration of the universe. The addition of the Virgo antenna into the network led in 2017 to the detection of a neutron star binary merger that could be followed in electromagnetic signals, representing the beginning of multi-messenger astronomy. At the moment, LIGO and Virgo observation plans extend until 2030 with upgraded detectors. At the same time, work is beginning on the development of the third generation of detectors which will offer an order of magnitude increase in sensitivity.

The ET project, a third-generation experiment to be realized in Europe, has been included in the 2021 EU ESFRI roadmap and has recently entered into the preparatory phase. CE is the planned US contribution to the third-generation GW network, with significant funding from the US NSF and the UK’s STFC for design studies.

IFAE is a member institution of the LVK collaboration. A group of researchers from IFAE has taken significant responsibilities in the Virgo experiment related to the control of the stray light inside the experiment, which is considered a limiting factor for its sensitivity. The group plays an important role in the commissioning, operations and upgrade of the interferometer. For the latter, IFAE is leading the construction of new baffles instrumented with photo sensors around the test masses.

IFAE is actively participating in ET, coordinates the EU Horizon INFRA-DEV project for the ET preparatory phase, and has central responsibilities in the design of the stray light control systems. In addition, IFAE is deeply involved in the detector R&D and optical simulation activities of ET and CE. IFAE works with CERN in the design of the ET vacuum pipes.

The IFAE research program spans many topics in astrophysics and cosmology using LIGO-Virgo data. This includes searches for compact binary coalescence events and determining their mass/spin spectrum, for primordial black holes as candidates for dark matter, and for axion-like signals in continuous GW signals. We perform tests of exotic models for Gravity beyond General Relativity, and cosmological measurements using GWs such as Hubble constant and probes of inflation and phase transitions in the early universe. We are developing new data analysis methods like the use of deep learning and the use of robust statistics. This work is naturally extended to studying physics prospects for the next generation of detectors.

IFAE is supported by its own PIC computing center, a Tier1 LHC center fully integrated into the LIGO/Virgo distributed computing network. IFAE is in a privileged position to analyze the LIGO/Virgo/KAGRA data and, in collaboration with IFAE’s teams in CTA/MAGIC and Observational Cosmology, to fully profit from a multi-messenger approach.

As a PhD student in our group, you will get involved in one of the group’s detector-related activities including LV data characterization, optical simulation studies, or the active monitoring of the stray light inside the LV optical cavities with new photo sensors in an ultra-high vacuum environment. You will also be deeply involved in the physics analysis of the LIGO-Virgo data, in one or more of the subjects described above. In addition, and within the framework of IFAE’s GW research activities, you will be offered significant training and networking opportunities, including extended stays of research in top-level international research centres in Europe and USA.

Required skills and evaluation criteria

To be eligible for this position, candidates must meet the requirements for enrollment in the UAB doctoral program for the 2025/2026 academic year. Key requirements include:

  • Holding a Bachelor’s degree (or equivalent) in Physics or a related field.
  • Holding a Master’s degree in Physics, Astrophysics, or a related field, which must be completed by the contract start date.
  • Basic knowledge on Gravitation.
  • We are looking for candidates with a strong background in physics, a pro-active attitude and good communication skills. While not mandatory, previous experience in programming (especially Python or C++), data analysis. Previous experience in Gravitational Wave physics and related technologies will be appreciated.
  • Fluency in written and spoken English is required.

The process of evaluation and selection guarantees the principles of open competition, publicity and transparency, according to the following criteria:

  • University Records: 50 points
  • Computing Skills: 20 points
  • Experience on physics analysis: 20 points
  • Communication skills in English: 10 points

A Selection Committee will evaluate the received applications. Shortlisted candidates may be invited to give a brief online presentation, followed by a Q&A with the committee.

Offered contract

  • Full-time contract (40 h/week)
  • Predoctoral contract; 4 years
  • The position will correspond to a PhD student.
  • Salary will be proportional to experience and qualifications within the corresponding category range.
  • Work with interesting experimental science. Opportunity to gain first-hand learning experience.
  • Personal growth, innovation and learning every day.
  • The selected candidate is expected to join the IFAE as soon as possible.

Application and Selection process

Applicants should have a Master Degree in Physics and provide a motivation letter, a CV and full University Records (transcripts of Bachelor’s and Master’s studies), and arrange for one or two letters of reference, sent to alundgren(at)ifae.es , mmp(at)ifae.es and rrhh(at)ifae.es and including in the subject “IFAE2025/33_GW_SO_PhDStudent”.

All applications received within one month of the opening date will receive full consideration. Sending CVs to the above addresses implies consent to the IFAE’s legal warning on data privacy. For further information please contact: Prof. Andrew Lundgren (alundgren(at)ifae.es ) Prof. Mario Martínez (mmp(at)ifae.es )

Please find here full details.

One PhD position in Relativistic Astrophysics and Gravitational-Wave Physics at the University of Valencia

The Relativistic Astrophysics Group at the University of Valencia (Spain) invites applications for one 4-year PhD position in the Topic of gravitational-wave physics in theories beyond general relativity. This position is linked to the research project “Computational relativistic astrophysics and data analysis in the era of gravitational-wave astronomy” (PID2024-159689NB-C21) of the Spanish Research Agency. The position entails research work on modelling of astrophysical sources of gravitational waves, numerical relativity, and data analysis. Application deadline: October 15th 2025.

We are seeking a highly motivated candidate interested in strong field modifications of general relativity and their test through astrophysical observations of compact objects. The candidate will conduct gravitational-wave source modelling in such theories, with these three main goals: (1) Find new qualitative features in gravitational-wave signals and electromagnetic signals from binary black hole and binary neutron star mergers in modified gravity. (2)
Explore the core-collapse supernova gravitational-wave signature for a rotating progenitor in modified theories of gravity. (3) Model isolated rotating black holes and neutron stars beyond General relativity, studying their observational properties and stability.

The Relativistic Astrophysics Group at the University of Valencia comprises faculty members Pablo Cerdá-Durán, José Antonio Font, Samuel Santos, and Alejandro Torres-Forné, non-tenured faculty Daniela Doneva, Milton Ruiz and Nicolás Sanchis-Gual, and over ten PhD students. The group is part of the LIGO-Virgo-KAGRA Collaboration, the Einstein Telescope Collaboration and of the LISA Consortium.

The successful candidate will be supervised by Daniela Doneva.

Applicants should prepare a CV, a brief statement of research interests, the academic transcripts, and the names (address, e-mail) of two potential referees. This documentation has to be sent by email before Oct 15th, 2025 to Toni Font (j.antonio.font(at)uv.es) and Daniela Doneva (daniela.doneva(at)uv.es). The start dates are flexible, but we aim to fill the position as soon as possible.

The University of Valencia is an equal opportunity employer that is committed to diversity and inclusion encouraging applications from women and/or other underrepresented groups.

PhD position in gravitational-wave astronomy and massive binary evolution at Radboud University

Join a pioneering PhD project exploring how massive stars evolve into gravitational-wave sources. Combine stellar physics, simulations and cutting-edge data to uncover the origins of black holes and neutron stars, linking theory with the latest discoveries in this rapidly growing field. Application deadline October 31st 2025.

It has been just over a decade since the first detection of gravitational waves, marking the birth of a new field in astronomy. Since then, the number of detections has grown rapidly: from one, to a few, to hundreds, revealing entire populations of gravitational-wave sources. These signals are produced by black holes and neutron stars, the compact remnants of massive stars.

Many questions on how these populations form remain. To solve this puzzle, we must understand how massive stars are born, interact in binary systems, and how they end their lives as black holes or neutron stars. This will be the topic of this PhD thesis.

As a PhD candidate, you will conduct fundamental research on the evolution of massive binary stars, with a special focus on the systems that give rise to gravitational-wave sources.

This theoretical project will be at the intersection of stellar physics, computational astronomy and an unprecedented amount of data driven by observation. You will learn to run simulations on high-performance computing clusters, ranging from broad parameter studies with rapid binary-population synthesis codes to detailed stellar evolution calculations with 1D stellar evolution codes. The models you develop will be directly linked to new and upcoming observations, including the just-released 4th gravitational-wave observations (O4, released in August 2025) and the Gaia DR4 dataset (expected mid-2026).

Your duties as a teaching assistant cover about 10 percent of your work time, spread over the course of the appointment.

Would you like to learn more about what it’s like to pursue a PhD at Radboud University? Visit the page about working as a PhD candidate.
Does this sound like you?

You hold a Master's degree in astronomy/physics or a related field, or you expect to obtain your Master’s degree around the starting date of the appointment.
You bring curiosity and enthusiasm, enjoy thinking critically, communicate openly, and take initiative.
You are able to work in a team as well as independently.
You have excellent writing and verbal communication skills in English.

What we offer you

We will give you a temporary employment contract (1.0 FTE) of 1.5 years, after which your performance will be evaluated. If the evaluation is positive, your contract will be extended by 2.5 years (4-year contract).     
You will receive a starting salary of €3,059 gross per month based on a 38-hour working week, which will increase to €3,881 in the fourth year (salary scale P).
You will receive an 8% holiday allowance and an 8,3% end-of-year bonus.
We offer Dual Career Coaching. The Dual Career Coaching assists your partner via support, tools, and resources to improve their chances of independently finding employment in the Netherlands. 
You will receive extra days off. With full-time employment, you can choose between 30 or 41 days of annual leave instead of the statutory 20. 

Additional employment conditions

Work and science require good employment practices. Radboud University’s primary and secondary employment conditions reflect this. You can make arrangements for the best possible work-life balance with flexible working hours, various leave arrangements and working from home. You are also able to compose part of your employment conditions yourself. For example, exchange income for extra leave days and receive a reimbursement for your sports membership. In addition, you receive a 34% discount on the sports and cultural activities at Radboud University as an employee. And, of course, we offer a good pension plan. We also give you plenty of room and responsibility to develop your talents and realise your ambitions. Therefore, we provide various training and development schemes.
Where you will be working

Your PhD project will be supervised by Dr. Lieke van Son (Radboud University) and will be carried out in a highly international setting. Collaboration with international research groups across the globe is expected.

This PhD position is embedded in the Astrophysics Department at the Institute for Mathematics, Astrophysics and Particle Physics (IMAPP) at Radboud University (Nijmegen, Netherlands). We are a very tight-knit and socially active department, currently home to 18 faculty members (junior and senior) and about 65 postdoctoral researchers and PhD candidates. Research at the department covers a broad range of topics, including stellar physics, black hole and accretion physics, gravitational waves, cosmic rays, and instrumentation.

Faculty of Science
The Faculty of Science (FNWI), part of Radboud University, engages in groundbreaking research and excellent education. In doing so, we push the boundaries of scientific knowledge and pass that knowledge on to the next generation.

We seek solutions to major societal challenges, such as cybercrime and climate change and work on major scientific challenges, such as those in the quantum world. At the same time, we prepare our students for careers both within and outside the scientific field.

Currently, more than 1,300 colleagues contribute to research and education, some as researchers and lecturers, others as technical and administrative support officers. The faculty has a strong international character with staff from more than 70 countries. Together, we work in an informal, accessible and welcoming environment, with attention and space for personal and professional development for all.

Please find here full details.

PhD student fellowship position at Center for Theoretical Physics Polish Academy of Sciences Warsaw

The Director of the Center for Theoretical Physics PAS announces a competition for oneScholar-PhD Student position at the CTP PAS, within the research Project Weave-UNISONO „Lensing of electromagnetic and gravitational waves”, financed by the National Science Center (GA no. UMO-2024/06/Y/ST2/00190), and within the Geoplanet doctoral school. The project’s leader is dr hab. Mikołaj Korzyński. The research will be conducted in collaboration with the group of Dr. Marius Oancea from the University of Vienna. Application deadline October 15th 2025.

The aims of the project are:

Optical drift effects close to caustics: investigating the effects of lens, observer and source transverse motion in strong gravitational lensing, for objects near caustics, Lensing of gravitational waves by strong gravitational fields: computing lensed gravitational waveforms originating from sources in strong-gravity environments, Computing the effects of propagation of waves in curved spacetimes beyond geometric optics using the Wigner function approach.

The scope of work of the successful Candidates will be pursuing their PhD project at CTP PAS and within the Geoplanet doctoral school. The scope of the project involves:

  • Developing software for raytracing of gravitational waves in strong gravitational fields,
  • Computing the waveforms from binary black hole systems,
  • Theoretical research on wave propagation in curved spacetimes.

Where to apply
E-mail rekrutacja(at)cft.edu.pl

Requirements

  • Research Field Astronomy » Astrophysics
  • Education Level Master Degree or equivalent
  • Research Field Physics » Other
  • Education Level Master Degree or equivalent

Skills/Qualifications

We expect the Candidates to have:

  • MSc in physics, astronomy or compatible,
  • Good programming skills and experience in numerical methods,
  • Independence and creativity in problem solving.

Knowledge of general relativity would be welcome.

Languages ENGLISH
Level Excellent

Please find here full details.

PhD position in gravitational-wave astronomy and massive binary evolution at Radboud University

Join a pioneering PhD project exploring how massive stars evolve into gravitational-wave sources. Combine stellar physics, simulations and cutting-edge data to uncover the origins of black holes and neutron stars, linking theory with the latest discoveries in this rapidly growing field. Application deadline October 31st 2025.

It has been just over a decade since the first detection of gravitational waves, marking the birth of a new field in astronomy. Since then, the number of detections has grown rapidly: from one, to a few, to hundreds, revealing entire populations of gravitational-wave sources. These signals are produced by black holes and neutron stars, the compact remnants of massive stars.

Many questions on how these populations form remain. To solve this puzzle, we must understand how massive stars are born, interact in binary systems, and how they end their lives as black holes or neutron stars. This will be the topic of this PhD thesis.

As a PhD candidate, you will conduct fundamental research on the evolution of massive binary stars, with a special focus on the systems that give rise to gravitational-wave sources.

This theoretical project will be at the intersection of stellar physics, computational astronomy and an unprecedented amount of data driven by observation. You will learn to run simulations on high-performance computing clusters, ranging from broad parameter studies with rapid binary-population synthesis codes to detailed stellar evolution calculations with 1D stellar evolution codes. The models you develop will be directly linked to new and upcoming observations, including the just-released 4th gravitational-wave observations (O4, released in August 2025) and the Gaia DR4 dataset (expected mid-2026).

Your duties as a teaching assistant cover about 10 percent of your work time, spread over the course of the appointment.

Would you like to learn more about what it’s like to pursue a PhD at Radboud University? Visit the page about working as a PhD candidate.
Does this sound like you?

  • You hold a Master’s degree in astronomy/physics or a related field, or you expect to obtain your Master’s degree around the starting date of the appointment.
  • You bring curiosity and enthusiasm, enjoy thinking critically, communicate openly, and take initiative.
  • You are able to work in a team as well as independently.
  • You have excellent writing and verbal communication skills in English.

What we offer you

  • We will give you a temporary employment contract (1.0 FTE) of 1.5 years, after which your performance will be evaluated. If the evaluation is positive, your contract will be extended by 2.5 years (4-year contract).
  • You will receive a starting salary of €3,059 gross per month based on a 38-hour working week, which will increase to €3,881 in the fourth year (salary scale P).
  • You will receive an 8% holiday allowance and an 8,3% end-of-year bonus.
  • We offer Dual Career Coaching. The Dual Career Coaching assists your partner via support, tools, and resources to improve their chances of independently finding employment in the Netherlands.
  • You will receive extra days off. With full-time employment, you can choose between 30 or 41 days of annual leave instead of the statutory 20.

Additional employment conditions

Work and science require good employment practices. Radboud University’s primary and secondary employment conditions reflect this. You can make arrangements for the best possible work-life balance with flexible working hours, various leave arrangements and working from home. You are also able to compose part of your employment conditions yourself. For example, exchange income for extra leave days and receive a reimbursement for your sports membership. In addition, you receive a 34% discount on the sports and cultural activities at Radboud University as an employee. And, of course, we offer a good pension plan. We also give you plenty of room and responsibility to develop your talents and realise your ambitions. Therefore, we provide various training and development schemes.
Where you will be working

Your PhD project will be supervised by Dr. Lieke van Son

(Radboud University) and will be carried out in a highly international setting. Collaboration with international research groups across the globe is expected.

This PhD position is embedded in the Astrophysics Department at the Institute for Mathematics, Astrophysics and Particle Physics (IMAPP) at Radboud University (Nijmegen, Netherlands). We are a very tight-knit and socially active department, currently home to 18 faculty members (junior and senior) and about 65 postdoctoral researchers and PhD candidates. Research at the department covers a broad range of topics, including stellar physics, black hole and accretion physics, gravitational waves, cosmic rays, and instrumentation.

Faculty of Science
The Faculty of Science (FNWI), part of Radboud University, engages in groundbreaking research and excellent education. In doing so, we push the boundaries of scientific knowledge and pass that knowledge on to the next generation.

We seek solutions to major societal challenges, such as cybercrime and climate change and work on major scientific challenges, such as those in the quantum world. At the same time, we prepare our students for careers both within and outside the scientific field.

Currently, more than 1,300 colleagues contribute to research and education, some as researchers and lecturers, others as technical and administrative support officers. The faculty has a strong international character with staff from more than 70 countries. Together, we work in an informal, accessible and welcoming environment, with attention and space for personal and professional development for all.

Please find here full details.