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16th International LISA Symposium, June 22-26, 2026, College Park, Maryland

The 16th International LISA Symposium will highlight gravitational wave astrophysics, with a primary focus on the most up-to-date theory and analysis that will inform science to be performed by the Laser Interferometer Space Antenna.

Details on remote participation, which will be limited, will be announced when registration opens in early 2026.

The symposium will be held at the University of Maryland’s Adele H. Stamp Student Union on June 22-26, 2026 in College Park, Maryland, USA.

Scientific Organizing Committee

Shane Larson (Chair), Clarkson University Stanislav Babak, APC – Paris Richard Brito, Instituto Superior Técnico Maria José Bustamante Rosell, Fisk & Vanderbilt Universities Laurentiu Caramete, Institute of Space Science, Bucharest-Magurele Eleonora Castelli, University of Maryland, Baltimore County & NASA GSFC Maria Charisi, Washington State University & University of Crete Nelson Christensen, Observeratoire Cote d’Azur John Conklin, University of Florida Neil Cornish, Montana State University Daniel J. D’Orazio, Space Telescope Science Institute Deborah Ferguson, University of Rhode Island Alessia Franchini, Università degli Studi di Milano Daryl Haggard, McGill Unviersity, Trottier Space Instittue Zoltan Haiman, Institute of Science & Technology Austria Sarah Vigeland, University of Wisconsin Milwaukee Stefano Vitale, Università di Trento Gudrun Wanner, AEI – Hannover David Weir, University of Helsinki Helvi Witek, University of Illinois Urbana-Champaign William Joseph Weber, Università di Trento

Local Organizing Committee

Peter Shawhan, University of Maryland
Ann Hornschemeier Cardiff, NASA Goddard Space Flight Center
Ira Thorpe, NASA Goddard Space Flight Center
Elizabeth Ferrara, University of Maryland

First held in 1996, the International LISA Symposium is held every two years to celebrate and share infornation and science related to the Laser Interferometer Space Antenna mission, a three-arm space-based gravitational wave detector being developed by the European Space Agency (ESA).

History

A listing of prior LISA Symposia and links to their websites can be found here.

Conference Website

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Gravity2026: New Frontiers in Cosmology, April 27 – May 1 2026 in Daejeon

The aim of the workshop is to foster comprehensive and in-depth discussions on the rapidly expanding frontiers of gravitational physics. The program will cover a wide spectrum of topics central to cosmology, including gravitational waves, early- and late-time cosmology, and theories of modified gravity.

This workshop is mainly organized by the IBS Center CTPU-CGA and is held on-site at the Institute for Basic Science in Daejeon, Korea. There is no registration fee. f you wish to attend, please register by 29 March 2026, 23:59 KST. We will also accept a number of contributed talks: if you wish to give a contributed talk, please register for the workshop by the above date and submit a title and abstract by 5 Apeil 2026, 23:59 KST. The selection will be made by the organizing committee.  Please note that we are not able to support VISA applications from non-invited speakers except in special cases. 

For information about previous events, please see:

Gravity2022: Current challenges in black hole physics and cosmology

Gravity2023: Dawn of field theoretic approach

Gravity2025: New horizon of black hole physics

Important deadlines:

Registration: 29 March 2026, 23:59 KST

Abstract submission: 5 April 2026, 23:59 KST

Confirmed Invited Speakers:

Ana Achucarro (Leiden U, Netherlands)

Antonio De Felice (YITP, Japan)

Jaume Garriga (ICCUB, Spain)

Fawad Hassan (Stockholm U, Sweden)

Donghui Jeong (Penn State U, USA)

Matteo Magi (IBS, Korea)

Takahiro Matsubara (KEK, Japan)

Shinji Mukohyama (YITP/RESCEU, Japan)

Nils Albin Nilsson (IBS, Korea)

Changbom Park (KIAS, Korea)

Seong Chan Park (Yonsei U, Korea)

Mairi Sakellariadou (King’s Coll. London, UK)

Misao Sasaki (APCTP/IPMU, Korea and Japan)

Teruaki Suyama (Institute of Science Tokyo, Japan)

Gianmassimo Tasinato (Swansea U, UK)

Niels Warburton (University Coll. Dublin, Ireland)

Local Organizing Committee:

Sebastian Bahamonde, Mohammad Ali Gorji, Dong-Won Jung, Nils Albin Nilsson, Hyunbae Park, Masahide Yamaguchi

Scientific Advisory Committee:

Katsuki Aoki (YITP), Antonio De Felice (YITP), Francesco Di Filippo (Goethe U.), Mohammad Ali Gorji (IBS), Shinji Mukohyama (YITP/RESCEU), Naritaka Oshita (YITP), Masroor C. Pookkillath (Sogang U.), Kazufumi Takahashi (Nihon U.), Masahide Yamaguchi (IBS)

Contact:

For general inquiries, please use ctpu-cga-admin(AT)ibs.re.kr

Workshop Website

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WE Heraeus Physics School und 62. Karpacz Winter School in Theoretical Physics “Multimessenger Astrophysics and Cosmology”, February 28 – March 6 2026 in Karpacz

The WE Heraeus Physics School and the 62nd Karpacz Winter School in Theoretical Physics "Multimessenger Astrophysics and Cosmology" will be held from 28 February to 6 March 2026.

Compact stars, dense remnants of supernovae, compress about 1.4 solar masses into a 10 km radius—reaching densities beyond atomic nuclei. Their extreme compactness makes them unique laboratories for high-density matter. Gravitational-wave detections of binary neutron star mergers now allow direct probes of such conditions, with hot, dynamic post-merger remnants offering complementary insight to cold pulsars.

With next-generation observatories like the Einstein Telescope and Cosmic Explorer, multi-messenger astrophysics—combining gravitational waves, electromagnetic signals, and neutrinos—will sharpen constraints on the dense-matter equation of state, extreme gravity, and heavy-element nucleosynthesis. Mergers also serve as standard sirens, enabling independent measurements of the Hubble constant.

The school will cover the thermal history of the Universe after its first second, from the quark–hadron transition to neutrino decoupling, linking microphysics to cosmological observables. Topics include the Hubble tension, modified gravity, primordial magnetic fields, compact-object mergers, future gravitational-wave science, and primordial black holes as dark-matter or galaxy-seed candidates—offering a unified view across astrophysics, cosmology, and particle physics.

School Website

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Einstein Telescope science workshop for early career Researchers, February 18-20, 2026 at Sapienza University of Rome

The workshop wants to bring together young researchers actively involved in the activities of the Observational Science Board (OSB), Instrumental Science Board (ISB) and Site Characterization Board (SCB) of the Einstein Telescope. Leaving plenty of room for discussions, it will be a great occasion to share research and ideas, start projects, learn about new topics, and build collaborations.

It does not matter whether you like cosmology or pulsars, individual sources or backgrounds, data analysis, cryogenics, quantum noise reduction, or novel sensing and control systems … if you are young and interested in ET science, this is the right place!

After an opening session on the broad activities of ET ISB, OSB and SCB, the workshop is organized as a series of parallel sessions between OSB and ISB, each featuring two talks by expert early career researcher, laying the ground on the topics of relevance for each division, followed by ample room for discussion.

As additional information for all the ET enthusiasts: there is another workshop, the Einstein Telescope Research Infrastructure: Challenges and Long-Term Sustainability workshop, to be held in Rome at Sapienza University on February 16–17.

Key dates

Registration open: October 22nd 2025
Program announcement: mid-November 2025
Registration deadline: January 6th 2026
Start! February 18th 2026

Workshop Website

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Neutron Stars: Modelling and Detection – SIGRAV International School 2026, February 16-20 in Vietri sul Mare

This edition of the Italian Society of General Relativity and Gravitation (SIGRAV) International School is dedicated to the study of neutron stars as outstanding sources of gravitational and electromagnetic waves in the strong-field regime. The program is structured to promote scholarly interaction and collaboration, offering participants the opportunity to engage with leading experts in the field. Through a series of advanced lectures and discussions, the School aims to provide a comprehensive understanding of current developments in gravitational research and to equip attendees with the knowledge and tools necessary to advance their own scientific work in the study of gravity.

The School will take place in Vietri sul Mare (SA), Italy, 16-20 February 2026.

The program of the School comprises the following four courses:

  • B. Haskell (Milan Univ., IT): Modelling of Neutron Stars as Gravitational Wave Sources
  • T. Hinderer (Utrecht Univ., NL) : Gravitational Signal from Late Inspiral and Merger of Neutron Stars
  • M.A. Papa (AEI, Hannover, DE) : Detection of Continuous Gravitational Waves
  • G. Ghirlanda (INAF, Brera, IT): Multimessenger Astrophysics with Neutron Stars

A social excursion is planned for Wednesday, offering participants the opportunity to visit the Royal Palace of Caserta

The School is intended for PhD students and young post-docs. In order to receive the certificate of participation, all lectures and seminars should be attended.

The Participation Fee (350 EUR for non-SIGRAV members, 300 EUR for SIGRAV members) guarantee the access to all courses and activities, including lunch and coffee breaks.

A reduced participation fee (50 EUR) is available for those which will be only able to attend the lectures remotely.

The room should be booked in the Lloyd’s Baia Hotel. Please, reserve your room by using the form available in the section “Practical Info – Accomodation and Transport”.

The deadline for registration and payment of the relative fee is 06 February 2025 (see Registration section).

School Website

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Einstein Telescope Vacuum and Cryogenics Industrial Workshop: opportunities and challenges, April 21–22 2026 at CERN

The purpose of the workshop is to bring together the leading institutes which are designing the vacuum and cryogenic systems of the Einstein Telescope (the third generation gravitational wave detector which is currently being designed in Europe) and European Big Science industries specialised in vacuum and cryogenic technologies, to discuss the challenges and opportunities ahead.

The event will be held in CERN, where the ET vacuum pilot sector is housed. The technical challenges and aimed companies are available in the following link, and the topics for industry contribution in this link.

Registration fee is 85 CHF and includes coffee breaks and an evening aperitif at CERN on 21 April. We encourage participants to book accommodation at the CERN hostel. The rate is 62 CHF for a single room with bathroom.

Workshp Website

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YOUNGST@RS – Lost in Translation: The languages of Gravitational Waves, January 19-21 2026 at University of Mainz

In recent years, the modelling of gravitational wave sources has become a cornerstone of theoretical and numerical relativity. Multiple communities—working with distinct formalisms such as Self-Force, Effective One Body (EOB), Effective Field Theory (EFT) and post-Newtonian approximations—have developed powerful tools to describe the two-body problem with increasing precision. Each of these approaches is advanced enough to come with its own set of language, notation, conceptual framework, and computational tools.

The workshop aims to bridge this gap and bring these communities closer together. This will be done by providing a mix of beginner friendly lectures, hands on coding sessions, plenary overviews together with state of the art research talks for each of the fields.

Workshp Website

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Summer school on Multimessenger Astrophysics at ICE in Barcelona, July 6-14 2026

On behalf of the Institute of Space Sciences (ICE-CSIC), we are pleased to announce the 9th edition of the ICE Summer School devoted to Multimessenger Astrophysics. This intensive programme is designed for advanced Master’s and PhD students, early-career researchers, and others interested in the physics and observational techniques associated with multimessenger phenomena in the universe.

Scientific Scope
Multimessenger astrophysics is the framework for studying the Universe through the synergistic use of electromagnetic radiation, cosmic rays,neutrinos, and gravitational waves. By integrating these diverse channels, researchers can obtain a comprehensive view of violent and energetic astrophysical systems, such as compact object mergers,
active galactic nuclei, and cosmic accelerators. The School will cover both foundational theory and data-driven methods that are Shaping current and future research directions in high-energy astrophysics and relativity.

Topics and Programme Highlights
The scientific programme will consist of lectures and hands-on sessions delivered by experts from ICE and collaborating institutions.

Core themes will include, but are not limited to:
-Radiation processes and fundamental interactions
-Cosmic ray astrophysics and propagation
-Gamma-ray astronomy
-Neutrino physics and detectors
-Gravitational wave theory and data analysis
-Hands-on data analysis sessions (e.g., Fermi data, LIGO/Virgo)
-Machine learning applications in multimessenger research

Detailed session titles, lecturers, and the full list of topics can already be found on the school’s website.

Dates and Venue
The School will run from 6 to 14 July 2026 at the Institute of Space Sciences (ICE-CSIC), located on the Campus of the Universitat Autònoma de Barcelona (UAB) in Bellaterra (Barcelona). The ICE building and possible accommodation are within the UAB campus area.

Participation, Registration, Fellowships
Applications are welcomed from Master’s and PhD students, as well as early-career postdoctoral researchers with a strong interest in multimessenger astrophysics. Information on registration procedures, selection criteria, and possible financial support are provided on the school’s website. Registration will close on March 20, 2025. Announcements of accepted participants and fellowships are expected to happen before April 15.

Contact and Further Information
Further details, including the official registration link and programme are published on the Summer School website. Participants are encouraged to monitor the event page for announcements and logistical guidance, and register as soon as possible.

School Website

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Kavli-IAU Global Coordination Workshop (GCW) “International Coordination of the Time – Domain and Multi-Messenger Sky: New Opportunities and New Challenges”, Görlitz, Germany, 22-26 June 2026

The workshop, to be hosted at the new German Centre for Astrophysics (DZA) in June 2026, builds on the highly successful Kavli-IAU Global Coordination Workshop series. This will bring together approximately 50 astronomers and astrophysicists from around the world to discuss the global considerations of time-domain astronomy and multimessenger astrophysics. The drivers for these areas over the next decade will be large, international projects which require prompt and coordinated follow-up of new astronomical discoveries that may disappear in just a few days, or even sooner.


The primary objectives of the workshop will be to 1) define and prioritise the outstanding scientific questions that require coordinated, multi-wavelength follow-up in this time period, and 2) produce a series of recommendations to be implemented by the astronomical community in order to achieve these scientific goals. It will bring together key representatives from the major projects involved in these areas as well as the broader astronomical community around the globe (including theorists, instrumentalists, and observers).

Recommendations will be translated into a report titled “An Updated RoadMap for Global Coordination in the Time-Domain and Multi-Messenger Eras”.

Co-Organisers

Brad Cenko: NASA Goddard Space Flight Center (USA)
Samaya Nissanke: DZA and Deutsches Elektronen-Synchrotron (DESY), University of Potsdam (Germany); University of Amsterdam (NL)

The workshop will take place in Görlitz, Germany and will be invitation-only.

Please find here details.

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LIGO-Virgo-KAGRA Collaboration Meeting, March 9-13 2026 in Pisa

We are delighted to host the March 2026 LIGO–Virgo–KAGRA (LVK) Collaboration Meeting in Pisa, Italy, from March 9th to 13th, 2026, at Pala Todisco – Meetings and More. 

The meeting will be hosted by the European Gravitational Observatory (EGO).

Whether you are attending in person or online, we look forward to a week of engaging discussions and fruitful collaborations!

Why Pisa?

Located in the heart of Tuscany, Pisa is world-famous for its Leaning Tower. Just a few kilometers outside the city, in the countryside of Cascina (Province of Pisa), stands the Virgo interferometer, one of the four detectors of the global LIGO–Virgo–KAGRA (LVK) network — making Pisa the ideal venue for this meeting.

In addition to science, Pisa and the surrounding region of Tuscany offer a unique blend of history, culture, and natural beauty. Participants can explore the Duomo, the Botanical Garden of the University of Pisa, founded in 1543 and the oldest university botanical garden in the world, and other art and history museums, enjoying the charm of its historic streets and squares.

Pisa is also easily accessible, with its international airport and close proximity to Florence Airport, providing connections to destinations around the world.

The Venue

Pala Todisco – Meeting and more, located a few kilometers northeast of Pisa, is surrounded by greenery. The venue can host large-scale events and is equipped with advanced digital and audio-visual technologies, ensuring the best possible conference experience in comfortable and suitable spaces.

Dedicated transportation will be organized from key locations in the city center to Pala Todisco, with buses provided by the organizers for meeting participants.
For more information, please visit the [Accommodation & Travel page]

Key Event Dates

11 September 2025 | First Announcement
15 December 2025 | Registration Opens
20 January 2026 | Early-Bird Registration Closes
28 February 2026 | General Registration Closes
9–12 March 2026 | LVK Collaboration Meeting
13 March 2026 | Satellite Workshops at EGO and Virgo Tour

Local Organizing Committee:

Massimo Carpinelli (Director of the European Gravitational Observatory, University of Milano-Bicocca)
Nicolas Arnaud (Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3)
Gianluca Gemme (Istituto Nazionale di Fisica Nucleare)
Lorenzo Mirasola (Departament de Física, Universitat de les Illes Balears, IAC3–IEEC)
Vincenzo Napolano (European Gravitational Observatory)
Massimiliano Razzano (University of Pisa, Istituto Nazionale di Fisica Nucleare)
Viola Sordini (Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3)
Elisa Velcani (European Gravitational Observatory)

Conference Website