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10th Physics and Astrophysics at the eXtreme Workshop and 3rd Cosmic Explorer Symposium in Urbana, Illinois on June 30 – July 3, 2025

The 10th Physics and Astrophysics at the eXtreme (PAX) Workshop and the 3rd Cosmic Explorer Symposium are events sponsored by the Physics Department of the University of Illinois at Urbana-Champaign and taking place in Urbana, Illinois on June 30 – July 3, 2025 at the Beckman Institute Auditorium (Room 1025) and Room 1005.

The meeting aims to explore how gravitational and electromagnetic wave observations can help us understand extreme physics, including strong gravitational fields, dark matter, nuclear physics, cosmology, and multimessenger astrophysics. The Cosmic Explorer Symposium will bring together the community to discuss important aspects of the design and operations of the Cosmic Explorer gravitational-wave observatories, covering both observational and instrument science. Together, PAX-X and the Cosmic Explorer Symposium will explore the science opportunities that come with the next-generation gravitational-wave detectors.

Workshop Website

2025 GW Open Data Workshop, May 12-14

Open Data Workshops provide participants with a hands-on introduction to working with data from LIGO, Virgo, and KAGRA. The workshops include lectures, software tutorials, and a data challenge that asks participants to find binary black hole merger signals in real observatory data.

This year’s workshop will use a hybrid format, where participants may join virtually through the online course or may join an in-person Study Hub. Participants are also encouraged to start their own Study Hubs if one in their area is not available. Workshop registration is free and enrollment is now open. We are also looking for mentors to update the tutorials and host Study Hubs – please contact Jonah Kanner if you are interested in helping.

Workshop details and enrollment are now available at https://learn.gwosc.org/

2025 North American Einstein Toolkit Workshop, June, 9-13 at University of Texas at Austin

The 2025 edition of the North American Einstein Toolkit Workshop will be held at the University of Texas at Austin. This is an opportunity for researchers and students to learn about the Einstein Toolkit (https://einsteintoolkit.org/), a community-driven software platform of core computational tools to advance and support research in relativistic astrophysics and gravitational physics.

The workshop will offer a mixture of talks and tutorials. The tutorials provide an opportunity for new users to become familiar with the Einstein Toolkit cyberinfrastructure. The talks are aimed at highlighting exciting science using the tools of numerical relativity, in particular, the Einstein Toolkit. At the end of the workshop, there will be a broad discussion on future directions of the Einstein Toolkit.

Workshop Website

PhD position on Teaching Einsteinian Physics at Schools, University of Western Australia

The Einstein-First project in the university of Western Australia is seeking PhD and Masters students with a background in modern physics (including quantum physics and relativity), strong interest in science communication, experience in science teaching and aptitude in quantitative and qualitative data analysis. Closing date: December 1st 2026.

Please find here full details and how to apply.

APPEC Town Meeting 2025, September 23–24 at Universidad de Zaragoza

Town Meeting 2025: Preparation of the 2027-2036 Strategic Roadmap

As input for the preparation of the roadmap, a community survey took place beginning of this year. A briefing book including all Astroparticle Physics topics from the survey will be prepared by the APPEC Scientific Advisory Committee and released this summer, stay tuned!

During the APPEC Town Meeting, we will further discuss each of these topics with respect to the European and international context, and the new developments in Astroparticle Physics and in the neighbouring fields that will shape the strategic recommendations of the next roadmap.

This event includes plenary talks as well as round table discussions for each topic, to ensure a large participation of the community to shaping the future of Astroparticle Physics strategic orientations.

The discussions at this Town Meeting will serve as input for the European Astroparticle Physics Strategy 2027-2036.

Meeting Website

35th Midwest Relativity Meeting and “EricFest”, October 31 – November 2, 2025 at University of Guelph

The 35th Midwest Relativity Meeting will be held at the University of Guelph on October 31 to November 2 (Friday to Sunday), 2025. The last day will be a scientific celebration of Eric Poisson's 60th birthday with invited speakers.

The Midwest Relativity Meetings bring together researchers from across the Midwest and beyond to discuss a broad range of topics in gravitational physics, including cosmology, gravitational waves, numerical relativity, and quantum gravity. The primary focus of this meeting is on graduate students and postdocs, all of whom are encouraged to give talks. The Blue Apple Award, sponsored by APS DGRAV, will be given for the best graduate student talk.

Meeting Website

XV ET Symposium, May 26-30 2025 in Bologna

The XV ET Symposium will take place in Bologna from May 26th until May 30th. 
The ET Symposium kicks off on Monday 26th after lunchtime and will end on Friday 30th at lunchtime.

The Symposium will be organized in parallel sessions, hosting workshops managed by the ET boards (EIB, ISB, OSB, and SPB), and plenary sessions. The complete timetable is under construction and will soon be released.

A social event for early career scientists will be organized during the Symposium week. More information will be available soon.

The abstract submission for talks & posters is open now. The submission deadline for your contributions is the 31st of March.

The registration is now open.

The fee for in-person participants is €400 (VAT included) and includes the social dinner. The limit for in-person attendees is 380 people.

Participants can also attend the Symposium remotely via Zoom. While registration is required, there is no fee for online participation.

Symposium Website

CDD researcher (M/F) : Ultra-dense matter equation of state and gravitational Waves, Caen, France

The determination of the equation of state and composition of ultra-dense matter from multi-messenger astrophysical observations remains a central challenge in nuclear physics and high-energy astrophysics. Within this context, the LuTH-Caen theory group, as part of the Virgo collaboration, itself part of the LIGO-Virgo-KAGRA consortium, has established a recognized expertise in the theoretical modeling of ultra-dense stellar matter and the development of advanced statistical methods for quantifying theoretical uncertainties and their impact on the confidence intervals of astronomical observables.

Application Deadline: March 27th 2025

This postdoctoral project aims to generate quantitative predictions for the key parameters governing the emission of detectable gravitational wave signals from compact objects, incorporating the uncertainties inherent in the underlying microphysics. Specifically, the successful candidate will focus on parameter estimation in one of two contexts: neutron star binary coalescence, either during the inspiral or post-merger phase, or the continuous gravitational waves emitted by isolated neutron stars.
Within this framework, the successful candidate will contribute to the interpretation of signals from past and ongoing LVK observational campaigns, as well as to the preparation for third-generation interferometers, including post-O5 and the Einstein Telescope. The research will specifically aim to constrain the microscopic properties of dense hadronic matter, such as the nuclear equation of state, and to identify potential signatures of deconfinement phase transitions.

Activities

The successful postdoctoral fellow will be responsible for maintaining and further developing the Bayesian analysis tools for equation-of-state inference within the LPC theory group. This work will be carried out in close collaboration with group members from GANIL and the Strasbourg Observatory, the latter being conducting numerical relativity simulations of post-merger remnants. Depending on the candidate’s previous research experience and interests, there may also be opportunities to contribute to the group’s theoretical developments related to the modeling of dense and superfluid matter in neutron stars. The candidate is expected to contribute to research activities and topics such as:

  • Development of the CUTER tool for the improvement of parameter estimation using microphysics informed equations of state, see https://zenodo.org/records/10781539
  • Numerical simulations for the physics case prospects of third generation interferometers
  • Theoretical modelling of the zero and finite temperature nuclear equation of state and its possible phase transitions, with both effective and microscopic models
  • Development and analysis of neutron star cooling simulations and applications to the measurable properties of the neutron star crust

Skills

The successful candidate must have a PhD in theoretical nuclear physics, gravitational wave data analysis or numerical hydrodynamics. Proficiency in scientific programming (C, C++, Python) and numerical simulations is expected. Familiarity with software development tools such as git and gitlab, while not essential, would be an advantage.

Work Context

The successful candidate will be assigned to the theory and phenomenology team, within the Corpuscular Physics Laboratory of Caen.
The team has a longstanding experience in theoretical nuclear modelling. Since 2020, it is part of the Virgo collaboration within a theoretical group including researchers from the astronomical observatory in Strasbourg, and the GANIL laboratory in Caen.
The LPC CAEN, with about 100 staff, is a joint research unit (UMR 6534) under the supervision of three institutions: the CNRS, the University of Caen Normandy (UCN) and the Ecole Nationale Supérieure d’Ingénieurs de Caen (ENSICAEN). It is located on Campus 2 of the University of Caen (Campus Côte de Nacre) and is part of the research park of ENSICAEN (www.lpc-caen.in2p3.fr/).

Please find here full details.

DESY-Fellowships in Experimental Particle Physics in Hamburg

DESY-Fellowships in Experimental Particle Physics; Remuneration Group 13; Limited: 2 years; Starting date: after Agreement; ID: FHFE001/2025; Deadline: 31.03.2025; Full-time/Part-time.

DESY, with more than 2900 employees at its two locations in Hamburg and Zeuthen, is one of the world’s leading research centres. Its research focuses on decoding the structure and function of matter, from the smallest particles of the universe to the building blocks of life. In this way, DESY contributes to solving the major questions and urgent challenges facing science, society and industry. With its ultramodern research infrastructure, its interdisciplinary research platforms and its international networks, DESY offers a highly attractive working environment in the fields of science, technology and administration as well as for the education of highly qualified young scientists.

We participate in leading roles in particle physics projects on our campus and in international laboratories such as CERN or KEK. We develop technologies for detectors and accelerators, and work on scientific computing. We operate important infrastructures such as the Tier2 centre or the test beam facility at DESY.

DESY Fellowships in Experimental Particle Physics are selected twice a year. Interested applicants who have recently completed their PhD are requested to submit their application including the scientific background and the usual documents (letter of motivation, research interest, CV, list of publications, copies of university degrees, three letters of reference) for the respective selection round via our application portal. The statement of future research should include both, physics analysis as well as detector or performance related interests. Application Deadline: March 31st, 2025.

The decision on the awarding of a fellowship for the 1/2025 selection round is presumably made on May 31.

About your role:

You are invited to take an active role in one or more of the following projects in Hamburg:

  • The ATLAS and CMS experiments at CERN or the Belle II experiment at KEK
  • Experimental activities on-site (ALPS II and preparation of future on-site experiments at DESY)
  • Preparations for future particle physics experiments, in particular detector and technology development
  • Scientific computing
  • Accelerator development (plasma wakefield)

Good reasons to join:

Look forward to a unique working environment on our international research campus. Respectful cooperation and the well-being of our DESY employees are particularly important to us. Gender equality is an important aspect for us. To support work life balance we offer flexible working hours, variable part-time, job-sharing models and participation in mobile work (up to 50%). You will benefit from our family-friendly and collegial atmosphere, our established health management and occupational pension provision. As a public funded employer, we offer you a secure workplace and facilitate your individual career with our comprehensive training and development opportunities. Remuneration is according to the regulations of the TV-AVH. DESY offers its employees a financial supplement for a German job ticket (Deutschland-Ticket) at both locations.

About you:

Ph.D. in physics (To be eligible, you have to take up the position at the latest 5 years after your doctorate)
Interest in particle physics, accelerator/detector development or scientific computing
Expertise relevant in at least one of the areas listed above

Further informations about the DESY-Fellowship can be found here: http://www.desy.de/FellowFH

Please arrange for three letters of reference to be sent to the DESY human resource department by using our online tool: Additional application documents.

Please find here full details.

Fourth MaNiTou Summer School on Gravitational Waves:A new window to the Universe, Jun 30 – July 5, 2025, Marseille

The school is collaboratively organized by scientific communities involved in Gravitational Waves, from 3 French locations in Southern France, namely Marseille, Nice and Toulouse, thus the MaNiTou name for the school.

The school will take place in Marseille this year, on the Luminy Campus of Aix Marseille Université, in the beautiful Calanques National Park (see here). It will be held in English.

Goals of the school

The school will cover the emerging field of gravitational wave detection and of its scientific exploitation. Following their discovery by the LIGO/Virgo consortia, many other gravitational wave detections are expected at the existing and future gravitational antennas. They will open up a new window of exploration, sometimes unique and sometimes complementary to what other messengers such as electromagnetic radiation (radio, IR, visible, UV, X-rays, gamma rays) and neutrinos can reveal of the physics at work in our Universe. The objective of the school is to provide the students with a solid introduction to most aspects of this interdisciplinary field in accelerated expansion 🙂

The school is open in priority to Master and PhD students, and also to young or not so young scientists who would like to get better acquainted with Gravitational Waves.

For attendees to fully benefit from the school programme, it is highly recommended that they have had at least an introductory exposure to General Relativity before. We also strongly suggest that prior to attending the school, the participants read some of the references that can be found here.

School Programme

GR and GW Theorie
Panorama of possible GW sources
GW Data Analysis
GW Instruments
– On Earth (LIGO/Virgo/Kagra, ET)
– In Space (LISA)
Hands on data
GW to study the Universe
– Astrophysics
– Cosmology
– Fondamental Physics
– Multi-Messager Astronomy
Advanced seminars
– Latest news from LIGO/Virgo/Kagra
– GW and Nuclear Physics
– Pulsar Timing Arrays (PTA)
– AI techniques
Preliminary list of speakers

  • Quentin Baghi – AstroParticule et Cosmologie (APC), Paris
    Space-based GW detectors: LISA
  • Oualid Chaibi – Artemis, Observatoire de la Côte d’Azur, Nice
    Ground-based GW interferometers and current observations
  • Francesca Gulminelli – Laboratoire de physique corpusculaire (LPC), Caen
    GWs and nuclear physics
  • Natalia Korsakova – AstroParticule et Cosmologie (APC), Paris
    Introduction to AI technique and AI applications to GWs
  • Astrid Lamberts – Artemis et Lagrange, Observatoire de la Côte d’Azur, Nice
    Astrophysics of GW sources
  • Frédérique Marion – Laboratoire d’Annecy de Physique des Particules (LAPP), Annecy
    Introduction to GW data analysis
  • Sylvain Marsat – Laboratoire des 2 infinis – Toulouse (L2IT), Toulouse
    Hands on GW data analysis
  • Simone Mastrogiovanni – Italian Institute for Nuclear Physics (INFN), Rome
    Cosmology with GWs
  • Joseph Romano – University of Texas Rio Grande Valley, Texas, USA
    Panorama of GW sources PTA science and stochastic background analysis
  • Mairi Sakellariadou – King’s College London, London
    Fundamental physics with GWs
  • Simone Speziale – Centre de Physique Théorique (CPT), Marseille
    GW Theory


School organization

In order to make the School efficient for the attendees in terms of knowledge transfer and training interaction with the scientists in charge of the different activities of the school, the attendance is limited to about 80 to 90 participants, not including organizers and teachers. If more than 90 people apply to the School, a selection will be applied based on the criteria outlined on the Registration page.

The School has no online attendance option. All participants are expected to attend in-presence.

No fee is required to attend the School.

The School will provide coffee breaks and lunches to all participants. Dinners, travel and accommodation expenses are not covered.

However, accommodation free of charge will be provided at CROUS at Luminy Campus for up to 50 master and PhD students who request it in the registration form. For more information about this opportunity and the selection, please see the Accommodation Section.

Moreover, since the school is labelled by CNRS as “Ecole Thématique”, the expenses to attend the school for CNRS employees (staff CNRS people and people with a CNRS term contract [PhD student, Postdoc,…]) will also be covered. Please do not forget to mention in the registration form if that case applies to you!


Apply to the school

To apply, please go to the Registration (Inscription) tab or directly follow the link here

Pre-registration will be open from March 4th to April 6th.
The pre-registered candidates will be informed of the result of the selection process during the first week of May.

School Website