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12th LISA CosWG Workshop, June 2-6, 2025 in Tallinn

The 12th LISA Cosmology Working Group Workshop will take place in Tallinn on June 2-6, 2025.

The workshop's objective is to convene the LISA Cosmology Working Group community to examine recent advancements in cosmology pertinent to LISA. Its purpose is to kickstart collaborative projects and tackle unresolved issues in LISA cosmology.

The topics of discussion include:

  • Predictions for SGWBs from the early universe
  • Detection of stochastic backgrounds and foregrounds
  • Characterization of isotropic and anisotropic SGWB components
  • Standard sirens and cosmological tests of the late universe
  • Cosmological probes of general relativity and non-standard paradigms
  • Primordial black holes and dark matter
  • Gravitational-wave lensing
  • Structure formation

About half of the workshop will be devoted to CosWG collaborative projects.

The workshop is restricted to LISA CosWG members. Non-members interested in participating must write to membership(at)lisamission.org (with chairscoswg(at)gmail.com in cc).

This workshop is supported by the Estonian Research Council grant RVTT7.

Please beware of fake e-mails attempting to offer you to book accommodation. The only reliable communications are those that come directly from the organisers.

Workshop Website

Gravitational Wave Probes of Physics Beyond Standard Model 4, June 23-27, 2025 at University of Warsaw

The purpose of this workshop is to discuss how gravitational waves may serve as tools to explore possible fundamental physics beyond the Standard Model, such as first-order phase transitions in the early Universe, cosmic strings, primordial black holes and scenarios for cosmological inflation. In addition, it will explore how gravitational wave signals may reveal possible modifications of general relativity. With these aims in mind, the workshop will bring together experts in particle physics, cosmology and the gravitational wave community.

Confirmed speakers:

  • Lara Sousa (Porto U) [cosmic defects]
  • Fabrizio Rompineve (UA Barcelona) [cosmic defects]
  • Alberto Roper Pol (U Geneva) [phase transition]
  • Oliver Gould (Nottingham U) [phase transition]
  • David Mateos (ICREA and U Barcelona) [phase transition]
  • Simone Blasi (DESY) [phase transition]
  • Nicola Bartolo (U Padua) [inflation]
  • Marek Szczepańczyk (U Warsaw) [astrophysics]
  • Alexander Jenkins (Cambridge U) [phase transition]
  • Christoph Ringeval (CP3, Louvain) [cosmic defects]

Workshop Website

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

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.