Skip to content

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.

Please find here details.

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

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

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.

GW-EM-Nu-2025: Multi-Messenger Science With Indian Facilities-Now and in the Next Decade, December 1-3 2025 at Tata Institute of Fundamental Research

This year marks the 10-years of discovery of Gravitational Waves, which has opened a new window for multi-messenger science. The era of multi-messenger science using signals from astrophysical sources observed in different cosmic messengers such as Cosmic Rays (CRs), Electromagnetic Waves (EW), Gravitational Waves (GW), and Neutrinos opens a new paradigm in understanding the physics governing the Universe over different length scales from the size of a nucleus to the size of the observable Universe. The success of this research frontier relies on the coordinated observation between different existing telescopes/observatories which are observing in different messengers and also on building the next generation telescopes/observatories that can jointly observe signals using different cosmic messengers in the coming years in the frequency range (or energy band) which are of scientific interests based on our theoretical understanding of these astrophysical sources. 

This conference plans to bring researchers from India working in different areas–instrumentation and theory on the same platform to discuss (i) the requirements and challenges in coordinated observations with existing Indian facilities between different messengers, (ii) key areas of development of telescope facilities and theoretical predictions for enhancing the scientific outcome, (iii) the roadmap for joint observations using multiple telescopes, and (iv) plan for strategically important future telescopes/observatories which will enhance multi-messenger science from India.

Conference Website

The School on Gravity: from motion to commotion, June 22-26 2026 at NBI Copenhagen

Understanding the gravitational interaction is one of the great scientific endeavors of the 21st century. The Nobel Prize-winning discovery of gravitational waves in 2015, and subsequent detections by the LIGO-Virgo-KAGRA Collaboration, have marked a revolutionary step forward in physics and astrophysics by opening an entirely new window for exploring the Universe. Future upgrades to these detectors, along with upcoming facilities such as LISA and the Einstein Telescope, promise even more breakthrough discoveries that the next generation of scientists will need to interpret.

The School on Gravity (22–26 June 2026, Copenhagen) will introduce junior scientists—graduate students and advanced undergraduates with a background in general relativity—to a wide range of foundational topics in the exciting new field of gravitational wave physics. Topics will span from the theory of motion, to new challenges introduced by quantum physics, to the astrophysics of black holes and source modeling for gravitational-wave detectors.

The School on Gravity will take place in the legendary Auditorium A of the Niels Bohr Institute, inviting students and lecturers to challenge current paradigms in gravitational physics in the spirit of the quantum revolution that unfolded in this very room.

The members of the Scientific Organizing Committee for the School of Gravity are Vitor Cardoso (Director of CoG), Emil Bjerrum-Bohr, Jose Ezquiaga, Troels Harmark, Niels Obers, Marta Orselli, Alessia Platania, Johan Samsing, Maarten van de Meent, Ziqi Yan.

The local organizing committee is composed of Vitor Cardoso and Jose Ezquiaga.

School Website

School on Gravity, Niels Bohr Institute, June 22-26 2026

Understanding the gravitational interaction is one of the great scientific endeavors of the 21st century. The Nobel Prize-winning discovery of gravitational waves in 2015, and subsequent detections by the LIGO-Virgo-KAGRA Collaboration, have marked a revolutionary step forward in physics and astrophysics by opening an entirely new window for exploring the Universe. Future upgrades to these detectors, along with upcoming facilities such as LISA and the Einstein Telescope, promise even more breakthrough discoveries that the next generation of scientists will need to interpret.

The School on Gravity (22–26 June 2026, Copenhagen) will introduce junior scientists—graduate students and advanced undergraduates with a background in general relativity—to a wide range of foundational topics in the exciting new field of gravitational wave physics. Topics will span from the theory of motion, to new challenges introduced by quantum physics, to the astrophysics of black holes and source modeling for gravitational-wave detectors.

The program is as follows:

Lectures on Black Holes and Neutron Stars (how, when and where they are born, how they spin, how many, when do they merge, how many merge).
Lecturer: Lieke van Son (Radboud University)

Lectures on Motion (the two body problem in General Relativity).
Lecturer: Julio Parra Martinez (IHES)

Lectures on Completing Einstein (why does General Relativity need completion, what type of effects should we be on look out for, where would they manifest themselves).
Lecturer: Gustavo Turiaci (U. Washington, Seattle)

Lectures on Environments (which type of environments, how do they affect strong field gravity, how do we model them, impact on gravitational wave signals).
Lecturer: Laura Sberna (Nottingham University)

Please apply at: https://the-center-of-gravity.com/events/the-school-on-gravity-from-motion-to-commotion-2026/

We require submission of a single pdf file containing a two-page CV, up to half a page motivation letter, and a signed support letter from an advisor on letterhead.

Deadline: February 01, 2026.

The number of seats is limited, so we encourage you to apply as soon as possible.

The School on Gravity will take place in the legendary Auditorium A of the Niels Bohr Institute, inviting students and lecturers to challenge current paradigms in gravitational physics in the spirit of the quantum revolution that unfolded in this very room. This is the first of a series of annual school organized by the Center of Gravity (CoG).

The members of the Scientific Organizing Committee for the School of Gravity are Vitor Cardoso (Director of CoG), Emil Bjerrum-Bohr, Jose Ezquiaga, Troels Harmark, Niels Obers, Marta Orselli, Alessia Platania, Johan Samsing, Maarten van de Meent, Ziqi Yan.

Local Organizing Committee: Vitor Cardoso and Jose Ezquiaga

Contact: sog(at)the-center-of-gravity.com

Save the Date: Black Holes Inside and Out 2027 (BHIO27): August 23-27 2027

The conference Black Holes Inside and Out 2027 (BHIO27) will take place at Sapienza University of Rome from August 23 to August 27, 2027.

This event follows the highly successful 2024 edition [https://strong-gr.com/black-holes-inside-and-out/], which brought together leading experts in black hole physics, including astrophysics and observational astronomy, cosmology, data analysis, mathematical and numerical relativity, perturbation theory, and quantum gravity, to discuss the state of the field and its future directions.

Preparations for the 2027 edition are underway, so please save the date! A webpage with all relevant information is under development and will be announced in early 2026.

We would greatly value your input regarding potential topics and speakers for this edition. To contribute suggestions, please fill out the following form: https://forms.gle/po4h8ifWm3LhvyTs7.

We particularly encourage suggestions outside your main areas of expertise, especially if motivated by an interest in learning more about developments in other branches of black hole physics.

Further information about the conference will be shared in the coming months.

The BHIO27 Scientific Organizing Committee

Luca Buoninfante, Raúl Carballo-Rubio, Vitor Cardoso, Francesco Di Filippo, Astrid Eichhorn, Paolo Pani