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International LILA Meeting (2025 Lunar Gravitational-Wave Workshop), November 13-14 2025 at APL, Laurel, Maryland

The Johns Hopkins Applied Physics Laboratory (APL) and the Vanderbilt Lunar Labs Initiative cordially invite the scientific community to the International LILA Meeting (2025 Lunar Gravitational-Wave Workshop), to be held 13–14 November 2025 at APL, Laurel, Maryland, USA. This is the fifth annual meeting in the Lunar GW Workshop series, following Belle-Île-en-Mer (2024), Nashville (2023), Bern (2022) and Cascina (2021). The 2025 Lunar GW workshop will take place in Building 200 on APL’s South Campus.

This meeting continues community discussions on the Laser Interferometer Lunar Antenna (LILA) project – a proposed detector on the lunar surface to measure gravitational waves in the mid-band between ground-based detectors LIGO–Virgo–KAGRA and the future space mission LISA. The primary foci of this workshop will be on defining the science goals, instrument implementation, deployment timeline, and establishing the formal consortium structure for LILA. Sessions will include multi-messenger astrophysics, lunar geoscience, instrumentation, and technology development.

Scientific Organizing Committees

  • Karan Jani, Vanderbilt University (co-chair)
  • Jim Kinnison, Applied Physics Laboratory (co-chair)
  • James Trippe, Vanderbilt University (co-chair)
  • John Conklin, University of Florida
  • Stephen Eikenberry, University of Central Florida
  • Kris Izquierdo, Applied Physics Laboratory
  • Philippe Lognonné, Institut de Physique du Globe de Paris
  • Mark Panning, Jet Propulsion Laboratory
  • Volker Quetschke, University of Texas Rio-Grande Valley
  • Robert Reed, Vanderbilt University
  • Brett Shapiro, Applied Physics Laboratory
  • Joseph Silk, Johns Hopkins University

Workshop Website

LIGO Scientific Collaboration Postdoctoral Position in the CGCA at UWM

The Leonard E. Parker Center for Gravitation, Cosmology, and Astrophysics (CGCA) at the University of Wisconsin-Milwaukee (UWM) invites applications for a postdoctoral position working with Prof. Brady and Prof. Creighton on research in gravitational wave physics and astronomy within the LIGO Scientific Collaboration.

The initial appointment is for one year, with renewal for a second (and, in most cases, a third) year contingent on continued funding and satisfactory performance. This position includes competitive salary and excellent fringe benefits. Applicants should have a PhD in physics, astrophysics, or a related field.
The CGCA at UWM has active research efforts in astronomy, astrophysics, gravity, and cosmology, with membership in the LIGO Scientific Collaboration, NANOGrav, the Event Horizon Telescope, and more. The core group is comprised of 8 faculty (Brady, Chang, Creighton, Erb, Kaplan, Medeiros, Vigeland and Wiseman), plus a number of scientists, postdocs, and graduate students.

Applicants should send a C.V., publication list, and a brief statement of their research interests by email to cgca-postdoc-applications(at)uwm.edu. Please include “LIGO” in the subject line of your email. Applicants should also arrange to have three letters of recommendation sent by e-mail to the above address. Review of applications will begin on 23 January 2026. Questions should also be sent to the above address, with “LIGO” included in the subject.

The University of Wisconsin – Milwaukee is an Equal Opportunity, Affirmative Action Employer.

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In Pursuit of Gravitational Waves: Solving the Two-Body Problem in General Relativity, Potsdam, October 20-22, 2025

The year 2025 offers a fitting moment to reflect on the development of one of the most profound problems in general relativity: the relativistic two-body problem. Just over fifty years ago, the discovery of the Hulse–Taylor pulsar provided the first observational evidence for gravitational radiation from binary systems. Since then, key contributions have marked decisive steps forward, leading to the first detection of gravitational waves in 2015 by the LIGO-VIRGO collaboration. As we commemorate ten years since that historic achievement, this progression of achievements not only traces a remarkable trajectory of scientific progress but also underscores the crucial interplay between analytical, numerical, and experimental communities in advancing our understanding of the two-body problem and its foundational role in gravitational-wave astronomy.

Against this backdrop, the Balzan Workshop In Pursuit of Gravitational Waves: Solving the Two-Body Problem in General Relativity, to be held from October 20 to 22, 2025, will bring together a select group of researchers who have played a central role in this history, alongside historians and philosophers of physics. The workshop offers an opportunity not only to revisit landmark developments, but also to reflect on the evolving methods, collaborations, and conceptual challenges that have shaped this remarkable scientific journey.

Hosted by the “Astrophysical and Cosmological Relativity” division at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute) in Potsdam, Germany, the Workshop is part of the Balzan Prize Project. This project investigates the historical and philosophical dimensions of solving the two-body problem in general relativity, with particular emphasis on the development of both analytical and numerical approaches, as well as the synergy—and at times, the dissonance—between these methods. The event will feature twelve talks that are historical, philosophical, and forward-looking in scope, along with three panel discussions centered on key themes:

• Why Did Progress in Analytical Relativity Differ in Europe Compared to the US, and More Generally Among Countries?
• Why Did the Progress in Numerical Relativity Differ in Europe Compared to the US, and More Generally Among Countries?
• Appreciation, Competition, and Synergism Between Analytical and Numerical Relativity Approaches

Contributions from experimentalists are also included, highlighting how theoretical modeling has both informed and responded to observational work.

The workshop is by invitation only. Each talk will be complemented by ample time for discussion, encouraging open and engaging exchanges across disciplinary boundaries.

Scientific organizing committee
Alexander Blum, Alessandra Buonanno, Félix-Louis Julié, Dennis Lehmkuhl, Jean-Philippe Martinez, Harald Pfeiffer, Christian Röken, and Jan Steinhoff.

Local organizing committee
Alessandra Buonanno, Félix-Louis Julié, Jean-Philippe Martinez, Harald Pfeiffer, and Jan Steinhoff.

Illustration and design
Ana Carvalho

Web development
Marco Gajardo

Administrative support
Brit Holland, Elke Müller

Workshop Website

Two postdoc positions at Syracuse University

Syracuse University is seeking two gravitational-wave experimentalist postdocs. The positions begin on or around January 1, 2026.

Postdoc in High Power Laser Applications under Professor Craig Cahillane, who is working on building a ultra-high power photoneutralization cavity for applications in nuclear fusion and gravitational wave detectors. Read more

Postdoc in Quantum Optics under Professor Georgia Mansell, who is working on understanding the interactions of squeezed light with complex interferometers, as well as building an electrostatic violin mode damper for Advanced LIGO. Read more

Both are involved in the optical design of Cosmic Explorer, the United States’ third generation gravitational wave observatory.Open until filled.

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(at)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.

PhD school in Stavanger, November 24- December 5

The University of Stavanger is glad to announce the 2025 NPACT school (Stavanger, Nov. 24th - Dec. 5th).

This school is part of the activities of the Norwegian Particle, Astroparticle and Cosmology Theory (NPACT) network and is open to Ph.D. students and early-career scientists worldwide who wish to broaden their understanding of topics within the NPACT scope.

Lectures and speakers:

  • Dark matter — T. Bringman (U. of Oslo)
  • Thermal history of the universe — H. Kolesova (U. of Stavanger)
  • Cosmological phase transitions and thermal particle production — M. Laine (U. of Bern)
  • Physics of neutron stars — A. Kurkela (U. of Stavanger)
  • Mapping the theory space: Bayesian and frequentist global fit — A. Kvellestad (U. of Oslo)
  • Gravitational waves and data analysis — A. Nielsen (U. of Stavanger)
  • Effective field theories and applications in particle physics — A. E. Thomsen (U. of Bern)

Practical information:

No attendance fee is required.
The school provides free accommodation to a limited number of participants requesting financial support by Oct. 14th. Under similar circumstances, priority will be given to early applicants.

Participants enrolled in a Norwegian Ph.D. program can earn 5 or 10 ECTS credits. For non-Norwegian programs, the official ECTS accreditation must be assessed on a case-by-case basis.

For details and registration, see the school webpage

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.

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.