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Research associate in GW instrumentation at ULiege

Open position for: Research associate (“logisticien.ne de Recherche”) (Gravitational waves instrumentation) University of Liège for a permanent contract (full time) starting ideally start on the 1st of September 2026. Application deadline: May 30th, 2026.

Context and missions
The Einstein Telescope (ET) will be Europe’s most advanced observatory for gravitational waves. It will allow researchers to hear black holes mergers and learn about the early universe.

The department of aerospace and mechanical engineering of University of Liège hosts the ET-CRISTAL facilities. ET-CRISTAL is an R&D facility for demonstrating crucial aspects of ET-Low Frequency. It uses innovative approaches for seismic isolation, i.e. an inverted pendulum stage on top of active seismic isolation platform and contact-free radiative cryogenic cooling of a large-scale cryogenic mirror. ET-CRISTAL is a Center of Excellence for the sub-system comprising the mirror, its suspension system, the vibration Isolation system, and cryogenic cooling of the mirror.

The Precision Mechatronics Laboratory within the Department of Aerospace and Mechanics (A&M) and from the School of Engineering at the University of Liège invites applications for an open position as a research associate in gravitational wave instrumentation at ET-CRISTAL. The facilities are installed at the Space Center (CSL) of the University of Liège and the main research offices of the Precision Mechatronics Laboratory are located within the Department.

As a Research Associate, you will have as missions to:

  • Lead the management of ET-CRISTAL facilities together with the Scientific Director (Prof. C. Collette), including research logistics, participation and tutoring of Master and PhD students as well as fellow researchers.
  • Develop and support research activities in fields relevant to ET-CRISTAL
  • Contribute to securing new funding and develop new collaborations

Application requirements

  • To hold a PhD in engineering, or an equivalent experience.
  • To have proven experience in one or several of these fields:
    • cryogenic inertial sensors
    • low frequency seismic isolation
    • radiative cooling
    • thermal noise modeling
    • Newtonian noise

You must also have strong project management skills, as well as excellent written and oral communication skills in English and, if possible, in French. You should be able to take the initiative and be skilled in negotiation and consensus-building.

We offer

  • A pleasant and dynamic work environment with a wide variety of assignments
  • Significant freedom in how you organize your work and a degree of autonomy in decision-making
  • Salary based on established pay scales and pre-determined pay Progression plans
  • The opportunity to support fundamental and applied research related to a Major Big Science instrument in an international Environment

Additional information
Prof. Dr. Ir. christophe.collette(at)uliege.be

ET-CRISTAL: https://www.etest-emr.eu
Precision Mechatronics Laboratory: https://www.pml.uliege.be
Liège Space Center: https://www.csl.uliege.be/cms/c_10241774/en/csl?id=c_10241774
University of Liège: https://www.uliege.be/cms/c_8699436/en/uliege

Application modalities
Applications should include a complete curriculum vitae, a personal motivation letter, and the name of three references in a single PDF file which should be sent by email to Prof. Christophe Collette (christophe.collette(at)uliege.be ) by the 30th of May 2026.

Please find here full details.

PhD position in GW instrumentation at ULiege

PhD position in GW instrumentation at University of Liège Precision Mechatronics Laboratory (PML) invites applications for a PhD position in gravitational wave instrumentation at University of Liège. PML is an active member of the LIGO Scientific Collaboration, and of the Einstein Telescope Collaboration. The group is coordinating ET-CRISTAL, a full-scale prototype of large cryogenic mirror, demonstrating sub-Hertz seismic isolation, and cryogenic cooling using purely radiative technology.
Application deadline May 30th, 2026.

The prototype is installed at the Space Center (CSL) of the University of Liège. University of Liège is a Belgian public university located at the heart of Europe in the cross-border region between the Netherlands and Germany, counting 11 faculties and nearly 30 000 students.

Capitalizing on this unique facility, the objective of this PhD is to develop an interferometric gradiometer that will be validated as a probe of Newtonian noise in the prototype. The project will be realized in close collaboration with the EPFL in Switzerland.

Applicants should hold a Master degree in engineering, physics or equivalent. The position is fully funded for a duration of four years and should ideally start on the 1st of September 2026. Applications should include a curriculum vitae, a personal motivation letter, and the name of three references. Applications should be sent by email to Prof. Christophe Collette (christophe.collette(at)uliege.be ) by the 30th of May 2026.

For more information:
ET-CRISTAL: https://www.etest-emr.eu
Precision Mechatronics Laboratory: https://www.pml.uliege.be
Liège Space Center: https://www.csl.uliege.be/cms/c_10241774/en/csl?id=c_102417
University of Liège https://www.uliege.be/cms/c_8699436/en/uliege

Please find here full details.

APS Division of Particles and Fields (DPF), July 20-24, 2026 at Fermilab

The 2026 edition of the APS Division of Particles and Fields (DPF) meeting will be held at Fermilab on July 20-24, 2026.

Registration is now open. Please note May 20 registration deadline for non-US citizens.

Abstract submission for parallel talks and posters is now open at https://indico.fnal.gov/event/72820/abstracts/

The Fermilab Users and Affiliates Meeting will be held on the overlapping Friday, July 24, 2026 https://indico.fnal.gov/event/73552/

Please note that low-cost housing ($50/night) will be available in dormitories at nearby Benedictine University.

A limited number of student travel awards will be available: https://indico.fnal.gov/event/72820/page/4422-student-travel-awards

Important deadlines:

  • Abstract submission deadline: May 11, 2026
  • In‑Person Registration (Non‑U.S. Citizens): May 20, 2026 at 5:00 PM CST
  • In‑Person Registration (U.S. Citizens): June 20, 2026 at 5:00 PM CST
  • Virtual Registration: July 1, 2026 at 5:00 PM CST

Meeting Website

The RING project in Germany: 1 Postdoc and 14 PhD positions in Physics, Geophysics, Geodesy

we would like to draw your attention to the 4-year RING project recently funded by the German Research Foundation (extendable to 8 years). The project has strong overlap with gravitational wave detection research on instrumentation.

The project aims at pushing the sensitivity and stability limits of rotational motion sensing with ring laser technology into new realms using approaches from quantum optics and metrology. The ultimate goal is to enable ring laser observations as a complement to classic space-geodetic methods towards more precise, high-rate estimation of Earth Orientation Parameters (EOP). Furthermore, we plan to develop (trans-) portable ring lasers fit for weak, broadband 6 degree-of-freedom ground motion observations towards better understanding of atmosphere-solid Earth coupling (also relevant for seismic decoupling of gravitational wave detection facilities).

The project offers postdoctoral and PhD topics in laser physics, geodesy, geophysics, hydrology, and seismology. The successful candidates will be part of a multi-disciplinary research team at various institutions in Germany with excellent training and experimental facilities.

More information, links to the individual research projects and open positions can be found here:
https://www.ringlaser.de


Prof. Dr. Katharina Isleif
https://www.hsu-hh.de/karriere/wp-content/uploads/sites/658/2026/04/Reference-Number-MB-0926.pdf

Prof. Dr. Oliver Gerberding
https://www.physik.uni-hamburg.de/en/iexp/gruppe-gerberding/offene-stellen.html

Ringdown in Lisbon, October 19-21 2026

Ringdown-focussed workshops have been held in New York in February 2022 and in Copenhagen in August 2024. For the growing community of people working on this topic, we plan to have the next meeting in 2026.

In the last year, the realm of black hole quasi-normal modes have been more vibrant than ever. The large number of updates is recognisable in the rise of a vibrant, young and motivated community that is pushing the boundaries of where we can test the nature of black holes with gravitational waves observations. The aim of this workshop is to give a space to this community for relaxed discussion session and fostering the birth of collaborations.

If you want to participate to the workshop, please fill in the registration form. Please be aware that the maximum number of partecipants is 100 and priority is given to invited participants. You will need manual confirmation from the organisers to finalise the registration.

Local Organising Commitee

Nicola Franchini, David Hilditch, Rita Sousa

Scientific Organising Commitee

Emanuele Berti, Vitor Cardoso, Gregorio Carullo, Nicola Franchini, David Hilditch

Speakers and Chairs

Marina de Amicis (Perimeter Institute)
Macarena Lagos (Universidad Andres Bello)
Mark H. Y. Cheung (Princeton Univerity) [TBC]Neev Khera (Guelph University)
Lorena Magaña Zertuche (Niels Bohr Institute)
Costantino Pacilio (Università “La Sapienza” of Rome)
Paolo Arnaudo (Southampton University)
Adrien Kuntz (Instituto Superior Técnico)
Marina David (Leuven University)
Jutta Kunz (Oldenburg University)
Joao Cavalcante (ABC Federal University)
Hayato Motohashi (Tokyo Metropolitan University)
Joachim Pomper (Università di Pisa)
Ling Sun (Australian National University)
Chantal Pitte (SISSA)
Alessandra Buonanno (Max Planck Institute – Potsdam)

Workshop Website

Gravitational Waves at the Fin del Mundo, January 11-22 2027, Universidad Central La Serena

Since the historic first detection in September 2015, gravitational wave observations have become routine, with the LIGO-Virgo-KAGRA network now detecting approximately one black hole merger every three days and having captured around 300 events to date. The future promises even more: next-generation detectors like the Einstein Telescope and Cosmic Explorer are expected to detect hundreds of thousands to millions of compact binary coalescences per year. These observations enable tests of fundamental physics in strong-gravity regimes, insights into the nature of compact objects and the evolution of stars, probes of cosmological evolution, and opens the possibility of multi-messenger astrophysics.

Join us for the 4th Gravitational Wave School in Chile (January 11-15), continuing a proud tradition of training a new generation of latin-american scientists in this growing and exciting research field. This time, the event will be followed by the international conference Gravitational Waves at the Fin del Mundo (January 18-22), inviting world-leading experts in strong-field gravitational physics and astrophysics.

These events will be held at Universidad Central in La Serena, Chile. La Serena is a charming seaside, in a region renowned for its pisco production and tropical papayas. Most importantly, La Serena serves as the gateway to some of the world’s most important astronomical facilities, including Vera C. Rubin Observatory, Cerro Tololo, Gemini, Las Campanas, and La Silla—making it the perfect location to explore the future of gravitational wave astrophysics.

4th Gravitational Wave School: Lecturers

Thomas Sotiriou (University of Nottingham)
Katerina Chatzioannou (Caltech)
Alessandra Corsi (Johns Hopkins University)
Pablo Marchant (Ghent University)

Gravitational Waves at the Fin del Mundo: Invited Speakers

Max Bañados (Catholic University of Chile)
*Clécio R. Bom (Brazilian Center for Physics Research)
Vitor Cardoso (Niels Bohr Institute)
Cecilia Chirenti (University of Maryland)
Katy Clough (Queen Mary University of London)
Anuradha Gupta (University of Mississippi)
Natalia Korsakova (Université Côte d’Azur)
Luis Lehner (Perimeter Institute)
Caio Macedo (Federal University of Pará)
*Rafaella Margutti (University of California, Berkeley)
Nicolás Yunes (University of Illinois Urbana-Champaign)

*To be confirmed

School Website

Postdoctoral Position at Indian Institute of Astrophysics in Bangalore

The Indian Institute of Astrophysics, Bangalore, India, invites applications for a postdoctoral (Research Associate–I) position in theoretical gravitational physics under an ANRF Advanced Research Grant. Application deadline: May 23, 2026.

The position is part of an active research program in black hole physics and strong-field gravity, aimed at exploring fundamental aspects of gravity in both classical and quantum regimes. The work broadly connects to questions involving black hole spacetimes, tests of general relativity and its extensions, quantum effects near horizons, and the nature of ultra-compact objects. There is particular interest in linking theoretical developments with observational signatures, including those relevant for black hole imaging, using a combination of analytical and semi-analytical techniques.

Candidates should have a Ph.D. in Physics with a strong background in general relativity, black hole physics, or closely related areas. Applicants are expected to demonstrate high-quality research output and the ability to carry out independent research.

Tenure: The appointment will be for an initial period of one year, extendable up to a total duration of 2.5 years, based on satisfactory performance.

Consolidated salary: Rs. 57,000 per month + HRA (as applicable) per month.

Application Procedure
Interested candidates should apply through the online portal (https://www.iiap.res.in/iia_jobs/) by submitting a Curriculum Vitae including a publication list, a research statement, and the names and contact details of at least two referees, along with any additional documents specified in the application.

Contact: Informal inquiries may be addressed to: Sanved Kolekar (sanved.kolekar[AT]iiap.res.in)

Please find here full details.

Call for postdoctoral positions at Université Paris-Saclay

The Graduate School of Physics at Université Paris-Saclay, France, is launching the second call of its new postdoctoral fellowship program: UPSaclay-STAR-φ, supported by the EU Marie Skłodowska-Curie COFUND. The program will recruit up to 41 international postdoctoral researchers over two calls, for 24-month projects in one of the 40 laboratories of the Graduate School, working on various fields from fundamental to applied physics. The CMS group of CEA-Saclay IRFU (contact: julie.malcles(at)cea.fr) is a possible host group, among others. The application deadline for the first call is July 15, 2026 at 5pm and the expected start of fellowships early 2027 (flexible).

Applicants will have to propose their own research project, with freedom of choice (in agreement with the thematics of interest of the CEA-Saclay/IRFU CMS team).

The CMS CEA-Saclay group has contributed to the design, construction and operation of the ECAL of CMS and is involved in the upgrades of the CMS detector (ECAL, MTD and HGCal).
The group is involved in the ECAL calibration and our analysis activities in Run3 include Higgs to Zy, double Higgs in the bb tautau channel, deep learning for ECAL and MTD reconstruction and various topics related to the diphoton channel (ttH/tH and its CP properties, high mass searches, interference to constraint the Higgs boson natural width with the mass measurement).

To be eligible, applicants must not have resided or carried out their main activity in France for more than 12 months during the 3 years preceding the deadline for applications.

For further information, please visit: http://www.cofund-physics.universite-paris-saclay.fr/

Postdoc Position in Relativistic Astrophysics in Warsaw

The Relativistic Astrophysics group at the CTP PAS, led by prof. Agnieszka Janiuk, Center for Theoretical Physics PAS, Warsaw, Poland, would like to offer a 3-year full time postdoctoral position, within the project “Dynamics of processes around compact stars”. Application deadline: June 20th, 2026 - 12:00 CEST.

The primary responsibilities include scientific research related to the scope of the project. Additional duties will include consulting some of the tasks conducted by PhD students in our team. There are no teaching duties, as we are research institute of the PAS.

Required documents:

  • The scientific CV, including the progress in the university studies, scientific achievements (publications, participation in research projects and conferences), with the clause “I agree to the processing of my personal data contained in the application documents for the purposes necessary for the implementation of the process recruitment by CTP PAS”.
  • Cover letter.
  • A copy of the PhD degree diploma.
  • Copies of documents confirming scientific or professional achievements (for candidates without PhD at the time of application, a statement from their Supervisor is required, regarding prospective date of defence).
  • At least two letters of recommendation from a faculty researcher with at least a PhD degree, concerning the candidate and his/her current scientific activity.
  • Research plan related to the scope of the project.
  • Signed Data Privacy Statement.

Please find here full details.

Postdoc Position in Theoretical Physics at Jagiellonian University in Kraków

The Institute of Theoretical Physics at the Jagiellonian Univeristy in Kraków, Poland, invites applications for a postdoctoral position. The sucessfull candidate will be expected to conduct a research programme in theoretical physics. We offer stable employment based on an employment contract at the renowned university as well as cooperation with the interdisciplinary academic community represented by well-known scientists. Application deadline: May 17th, 2026, 23:59:59 Warsaw time.

The candidates should:

  • hold at least a Master’s degree, Master of Science degree or an equivalent degree;
  • exhibit aptitude for research work.

Duration of employment: 33 months starting from October 1, 2026

Required documents include:

  • resume (CV),
  • personal questionnaire filled in by the Candidate (F/M),
  • copy of the master’s diploma or a doctoral diploma, if applicable,
  • information on the Candidate’s (F/M) scientific, teaching and organisational achievements,
  • declaration of the Candidate (F/M), confirming that the Jagiellonian University will be their primary place of work, should they be selected in the selection procedure,
  • statement under Article 113 of the Law on Higher Education and Science,
  • statement on acknowledging and accepting the rules and regulations concerning intellectual property management and commercialisation in force at the Jagiellonian University,
  • motivation letter,
  • list of publications (along with the respective publishing houses and the number of pages),
  • information concerning educational activities carried out by the Candidate (F/M), if any,
  • two recommendation letters concerning the Candidate’s (F/M) research work. The recommendation letters must be sent by e-mail directly by their authors to: ift(at)uj.edu.pl (in the e-mail subject please include: „Asystent IFT 2026: Name and surname”. At the Candidate’s request, the letters of recommendation may be made available to her/him.

Declaration forms (no. 5‒7) and personal questionnaire template (no. 2) can be obtained at: https://cso.uj.edu.pl/en_GB/dokumkandyd

For other details, such as benefits or remuneration, concerning the opening see:
https://praca.bip.uj.edu.pl/documents/145868730/160698977/1227.1101.104.2026_assistant_WFAiIS.pdf/0f0e0479-48b8-4539-a890-f0283d35cf90

Applications should be sent by email to: ift(at)uj.edu.pl
Subject: “Asystent IFT 2026: Name and Surname”

Application deadline: 2026/05/17 23:59:59 Warsaw time.

For further information please contact Institute of Theoretical Physics, e-mail address: ift(at)uj.edu.pl .

Please find here full details.