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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

PhD Position in Gravitational Waves Physics at IFAE Barcelona

IFAE is an internationally recognized center for fundamental research in Particle Physics, Astroparticle Physics, and Cosmology. Its main mission is to advance these fields through theoretical, experimental, and technological research. IFAE offers an international, dynamic, and competitive environment for the training of young researchers. IFAE has been accredited three times with the “Severo Ochoa Centre of Excellence” distinction, most recently for the 2025-2029 period.

About the IFAE Gravitational Waves group
The detection of GWs from a black hole binary merger by LIGO in 2015 started a new era in the exploration of the universe. The addition of the Virgo antenna into the network led in 2017 to the detection of a neutron star binary merger that could be followed in electromagnetic signals, representing the beginning of multi-messenger astronomy. At the moment, LIGO and Virgo observation plans extend until 2030 with upgraded detectors. At the same time, work is beginning on the development of the third generation of detectors which will offer an order of magnitude increase in sensitivity.

The ET project, a third-generation experiment to be realized in Europe, has been included in the 2021 EU ESFRI roadmap and has recently entered into the preparatory phase. CE is the planned US contribution to the third-generation GW network, with significant funding from the US NSF and the UK’s STFC for design studies.

IFAE is a member institution of the LVK collaboration. A group of researchers from IFAE has taken significant responsibilities in the Virgo experiment related to the control of the stray light inside the experiment, which is considered a limiting factor for its sensitivity. The group plays an important role in the commissioning, operations and upgrade of the interferometer. For the latter, IFAE is leading the construction of new baffles instrumented with photo sensors around the test masses.

IFAE is actively participating in ET, coordinates the EU Horizon INFRA-DEV project for the ET preparatory phase, and has central responsibilities in the design of the stray light control systems. In addition, IFAE is deeply involved in the detector R&D and optical simulation activities of ET and CE. IFAE works with CERN in the design of the ET vacuum pipes.

The IFAE research program spans many topics in astrophysics and cosmology using LIGO-Virgo data. This includes searches for compact binary coalescence events and determining their mass/spin spectrum, for primordial black holes as candidates for dark matter, and for axion-like signals in continuous GW signals. We perform tests of exotic models for Gravity beyond General Relativity, and cosmological measurements using GWs such as Hubble constant and probes of inflation and phase transitions in the early universe. We are developing new data analysis methods like the use of deep learning and the use of robust statistics. This work is naturally extended to studying physics prospects for the next generation of detectors.

IFAE is supported by its own PIC computing center, a Tier1 LHC center fully integrated into the LIGO/Virgo distributed computing network. IFAE is in a privileged position to analyze the LIGO/Virgo/KAGRA data and, in collaboration with IFAE’s teams in CTA/MAGIC and Observational Cosmology, to fully profit from a multi-messenger approach.

As a PhD student in our group, you will get involved in one of the group’s detector-related activities including LV data characterization, optical simulation studies, or the active monitoring of the stray light inside the LV optical cavities with new photo sensors in an ultra-high vacuum environment. You will also be deeply involved in the physics analysis of the LIGO-Virgo data, in one or more of the subjects described above. In addition, and within the framework of IFAE’s GW research activities, you will be offered significant training and networking opportunities, including extended stays of research in top-level international research centres in Europe and USA.

Required skills and evaluation criteria

To be eligible for this position, candidates must meet the requirements for enrollment in the UAB doctoral program for the 2025/2026 academic year. Key requirements include:

  • Holding a Bachelor’s degree (or equivalent) in Physics or a related field.
  • Holding a Master’s degree in Physics, Astrophysics, or a related field, which must be completed by the contract start date.
  • Basic knowledge on Gravitation.
  • We are looking for candidates with a strong background in physics, a pro-active attitude and good communication skills. While not mandatory, previous experience in programming (especially Python or C++), data analysis. Previous experience in Gravitational Wave physics and related technologies will be appreciated.
  • Fluency in written and spoken English is required.

The process of evaluation and selection guarantees the principles of open competition, publicity and transparency, according to the following criteria:

  • University Records: 50 points
  • Computing Skills: 20 points
  • Experience on physics analysis: 20 points
  • Communication skills in English: 10 points

A Selection Committee will evaluate the received applications. Shortlisted candidates may be invited to give a brief online presentation, followed by a Q&A with the committee.

Offered contract

  • Full-time contract (40 h/week)
  • Predoctoral contract; 4 years
  • The position will correspond to a PhD student.
  • Salary will be proportional to experience and qualifications within the corresponding category range.
  • Work with interesting experimental science. Opportunity to gain first-hand learning experience.
  • Personal growth, innovation and learning every day.
  • The selected candidate is expected to join the IFAE as soon as possible.

Application and Selection process

Applicants should have a Master Degree in Physics and provide a motivation letter, a CV and full University Records (transcripts of Bachelor’s and Master’s studies), and arrange for one or two letters of reference, sent to alundgren(at)ifae.es , mmp(at)ifae.es and rrhh(at)ifae.es and including in the subject “IFAE2025/33_GW_SO_PhDStudent”.

All applications received within one month of the opening date will receive full consideration. Sending CVs to the above addresses implies consent to the IFAE’s legal warning on data privacy. For further information please contact: Prof. Andrew Lundgren (alundgren(at)ifae.es ) Prof. Mario Martínez (mmp(at)ifae.es )

Please find here full details.

One PhD position in Relativistic Astrophysics and Gravitational-Wave Physics at the University of Valencia

The Relativistic Astrophysics Group at the University of Valencia (Spain) invites applications for one 4-year PhD position in the Topic of gravitational-wave physics in theories beyond general relativity. This position is linked to the research project “Computational relativistic astrophysics and data analysis in the era of gravitational-wave astronomy” (PID2024-159689NB-C21) of the Spanish Research Agency. The position entails research work on modelling of astrophysical sources of gravitational waves, numerical relativity, and data analysis. Application deadline: October 15th 2025.

We are seeking a highly motivated candidate interested in strong field modifications of general relativity and their test through astrophysical observations of compact objects. The candidate will conduct gravitational-wave source modelling in such theories, with these three main goals: (1) Find new qualitative features in gravitational-wave signals and electromagnetic signals from binary black hole and binary neutron star mergers in modified gravity. (2)
Explore the core-collapse supernova gravitational-wave signature for a rotating progenitor in modified theories of gravity. (3) Model isolated rotating black holes and neutron stars beyond General relativity, studying their observational properties and stability.

The Relativistic Astrophysics Group at the University of Valencia comprises faculty members Pablo Cerdá-Durán, José Antonio Font, Samuel Santos, and Alejandro Torres-Forné, non-tenured faculty Daniela Doneva, Milton Ruiz and Nicolás Sanchis-Gual, and over ten PhD students. The group is part of the LIGO-Virgo-KAGRA Collaboration, the Einstein Telescope Collaboration and of the LISA Consortium.

The successful candidate will be supervised by Daniela Doneva.

Applicants should prepare a CV, a brief statement of research interests, the academic transcripts, and the names (address, e-mail) of two potential referees. This documentation has to be sent by email before Oct 15th, 2025 to Toni Font (j.antonio.font(at)uv.es) and Daniela Doneva (daniela.doneva(at)uv.es). The start dates are flexible, but we aim to fill the position as soon as possible.

The University of Valencia is an equal opportunity employer that is committed to diversity and inclusion encouraging applications from women and/or other underrepresented groups.

PhD position in gravitational-wave astronomy and massive binary evolution at Radboud University

Join a pioneering PhD project exploring how massive stars evolve into gravitational-wave sources. Combine stellar physics, simulations and cutting-edge data to uncover the origins of black holes and neutron stars, linking theory with the latest discoveries in this rapidly growing field. Application deadline October 31st 2025.

It has been just over a decade since the first detection of gravitational waves, marking the birth of a new field in astronomy. Since then, the number of detections has grown rapidly: from one, to a few, to hundreds, revealing entire populations of gravitational-wave sources. These signals are produced by black holes and neutron stars, the compact remnants of massive stars.

Many questions on how these populations form remain. To solve this puzzle, we must understand how massive stars are born, interact in binary systems, and how they end their lives as black holes or neutron stars. This will be the topic of this PhD thesis.

As a PhD candidate, you will conduct fundamental research on the evolution of massive binary stars, with a special focus on the systems that give rise to gravitational-wave sources.

This theoretical project will be at the intersection of stellar physics, computational astronomy and an unprecedented amount of data driven by observation. You will learn to run simulations on high-performance computing clusters, ranging from broad parameter studies with rapid binary-population synthesis codes to detailed stellar evolution calculations with 1D stellar evolution codes. The models you develop will be directly linked to new and upcoming observations, including the just-released 4th gravitational-wave observations (O4, released in August 2025) and the Gaia DR4 dataset (expected mid-2026).

Your duties as a teaching assistant cover about 10 percent of your work time, spread over the course of the appointment.

Would you like to learn more about what it’s like to pursue a PhD at Radboud University? Visit the page about working as a PhD candidate.
Does this sound like you?

You hold a Master's degree in astronomy/physics or a related field, or you expect to obtain your Master’s degree around the starting date of the appointment.
You bring curiosity and enthusiasm, enjoy thinking critically, communicate openly, and take initiative.
You are able to work in a team as well as independently.
You have excellent writing and verbal communication skills in English.

What we offer you

We will give you a temporary employment contract (1.0 FTE) of 1.5 years, after which your performance will be evaluated. If the evaluation is positive, your contract will be extended by 2.5 years (4-year contract).     
You will receive a starting salary of €3,059 gross per month based on a 38-hour working week, which will increase to €3,881 in the fourth year (salary scale P).
You will receive an 8% holiday allowance and an 8,3% end-of-year bonus.
We offer Dual Career Coaching. The Dual Career Coaching assists your partner via support, tools, and resources to improve their chances of independently finding employment in the Netherlands. 
You will receive extra days off. With full-time employment, you can choose between 30 or 41 days of annual leave instead of the statutory 20. 

Additional employment conditions

Work and science require good employment practices. Radboud University’s primary and secondary employment conditions reflect this. You can make arrangements for the best possible work-life balance with flexible working hours, various leave arrangements and working from home. You are also able to compose part of your employment conditions yourself. For example, exchange income for extra leave days and receive a reimbursement for your sports membership. In addition, you receive a 34% discount on the sports and cultural activities at Radboud University as an employee. And, of course, we offer a good pension plan. We also give you plenty of room and responsibility to develop your talents and realise your ambitions. Therefore, we provide various training and development schemes.
Where you will be working

Your PhD project will be supervised by Dr. Lieke van Son (Radboud University) and will be carried out in a highly international setting. Collaboration with international research groups across the globe is expected.

This PhD position is embedded in the Astrophysics Department at the Institute for Mathematics, Astrophysics and Particle Physics (IMAPP) at Radboud University (Nijmegen, Netherlands). We are a very tight-knit and socially active department, currently home to 18 faculty members (junior and senior) and about 65 postdoctoral researchers and PhD candidates. Research at the department covers a broad range of topics, including stellar physics, black hole and accretion physics, gravitational waves, cosmic rays, and instrumentation.

Faculty of Science
The Faculty of Science (FNWI), part of Radboud University, engages in groundbreaking research and excellent education. In doing so, we push the boundaries of scientific knowledge and pass that knowledge on to the next generation.

We seek solutions to major societal challenges, such as cybercrime and climate change and work on major scientific challenges, such as those in the quantum world. At the same time, we prepare our students for careers both within and outside the scientific field.

Currently, more than 1,300 colleagues contribute to research and education, some as researchers and lecturers, others as technical and administrative support officers. The faculty has a strong international character with staff from more than 70 countries. Together, we work in an informal, accessible and welcoming environment, with attention and space for personal and professional development for all.

Please find here full details.

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

Weinberg fellowships in gravitation, multi-messenger astrophysics and AI/ML

The Center for Gravitational Physics (CGP) within the Weinberg Institute at the University of Texas at Austin invites applicants for multiple Weinberg Institute Postdoctoral Fellowships. These are full-time postdoctoral positions starting in September 2026.

This position is open to candidates in gravitational-wave physics, astrophysics and data analysis, especially in (but not limited to) the areas of:

(1) Cosmological inference with gravitational-wave observations
(2) Applications of AI/ML techniques broadly to astrophysics, cosmology or gravitational wave data analysis
(3) Nuclear astrophysics with gravitational-wave observations
(4) Gravitational-wave multimessenger astrophysics
(5) Numerical simulations of compact binaries

Applicants must submit a cover letter (no more than 1 page), CV, list of publications, a short statement of research interests (no more than 3 pages in length) and arrange to have at least three letters of reference uploaded to AJO. Applications are due November 21, 2025. The completion of a PhD is required prior to the beginning of this appointment. The initial appointment is for two years, with the possibility of extension to a third year subject to available funding and research performance.

Inquiries may be sent to Profs. Hsin-Yu Chen (hsinyu(at)austin.utexas.edu) or Jay Wadekar (jay.wadekar(at)utexas.edu).

McWilliams Postdoctoral Fellowship at Carnegie Mellon

The Department of Physics at Carnegie Mellon University invites applications for the McWilliams Postdoctoral Fellowship. McWilliams Fellows are expected to carry out their own programs of original research, independently or in collaboration with Carnegie Mellon faculty, postdoctoral fellows, and students. We welcome applications from researchers working in any area of astrophysics and/or cosmology. For full consideration, all materials should be received by November 10, 2025.

McWilliams Postdoctoral Fellows are part of CMU’s McWilliams Center for Cosmology and Astrophysics. The McWilliams Center synergizes research carried out in CMU’s Departments of Physics, Computer Science, Machine Learning, and Statistics, and enjoys close relationships with the University of Pittsburgh’s Department of Physics and Astronomy. Carnegie Mellon’s physics faculty hold leadership roles in multiple large sky surveys and consortia, including DES, DESI, HSC, LISA, and Rubin LSST. CMU is also a co-host of LINCC Frameworks which is developing analysis software infrastructure to enable the use of Rubin LSST data. Theoretical and observational studies within the Center cover a wide range of astrophysical phenomena, including galaxy and structure formation, black holes and gravitational waves, stellar evolution, gravitational lensing, dynamical detection of dark matter (see list of center faculty here). The McWilliams Center benefits from the Vera computing cluster at the Pittsburgh Supercomputing Center, which provides high-performance computing resources on a variety of scales and works closely with our scientists.

Fellowship appointments are for 2 years, with renewal for a third year likely, contingent upon satisfactory progress. The position comes with a competitive salary, an annual research budget, health benefits, and relocation expenses.
Applicants should hold a Ph.D. in physics, astronomy, or an adjacent field by the time of appointment, which is anticipated to begin September 1, 2026.

Application Instructions:
Applications should be uploaded to the Interfolio website and must include a curriculum vitae, publication list, a statement of research interests, and a cover letter. The cover letter should identify the applicant’s scientific background and goals, explain any synergies that make CMU a good fit for the proposed work, and can include examples of the candidate’s engagement within both academic and general public communities. There are no formal page limits, but the AAS Postdoctoral Guidelines should be seen as a target for length and detail.

In addition, candidates should arrange for three letters of recommendation to be uploaded (a prompt will be sent automatically to the applicant’s references when their contact information is entered at the Interfolio site). For full consideration, all materials should be received by November 10, 2025.

Please find here details and how to apply.

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

Capra 29 in Brussels, June 26 – July 3, 2026

We are pleased to announce that the 29th Capra Meeting on Radiation Reaction in General Relativity will be hosted in Brussels from Monday June 29th to July 3rd 2026. It will take place as a Solvay workshop organised by the International Solvay Institutes.

Further information about Capra 2026 will be posted in the coming months on https://www.caprameeting.org/ and https://solvayinstitutes.be/home/activities/workshop/ .

The Capra meeting is an annual conference on the topic of radiation reaction in general relativity. The primary focus of these conferences is the development of the gravitational self-force approach to model extreme mass ratio inspirals and further our understanding of the two-body problem in general relativity. This is done in synergy with other well-known modeling techniques such as post-Newtonian theory and numerical relativity. The canonical example of an extreme-mass-ratio inspiral (EMRI) is the inspiral of a stellar-mass compact object into a supermassive black hole. Gravitational waves from these systems are a promising target for the future space-based detector LISA.

The study of radiation reaction and self-force is not limited to EMRIs, and a range of topics and applications to other areas of gravitational physics have been discussed at past Capra meetings; an example is the scattering of massive particles, which is currently an active area of research. The format of the meeting is an amalgamation of a daily invited review talk, short contributed talks and organised discussion sessions.

Following the tradition of past Capra meetings, no registration fee is charged. A contribution of 50 euros to the banquet will be requested at registration for the attendees that would like to join the banquet. Several selected early career researchers will be funded by providing up to 6 nights of accommodation during the conference. Applications will be reviewed by members of the local organising committee and the equity, diversity and inclusion team at Capra.

The international scientific committee
Leor Barack, Susanna Barsanti, Béatrice Bonga, Alvin Chua, Lisa Drummond, Scott Hughes, Adam Pound, Vojtěch Witzany

The local organizing committee
Geoffrey Compère, Lidia Gomes Da Silva, Marc Henneaux, Loïc Honet, Guillaume Lhost, Gabriel Piovano