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Post-doctoral position in Computing for Gravitational Wave Experiments at INFN, Turin

A postdoc level position is opened at INFN Torino to work on Distributed Computing for the Einstein Telescope and in general Gravitational Wave Experiments. The topic is:Design and Implementation of a Multi-Research Infrastructure Data Access and Discovery model with Rucio for Gravitational Wave experiments. The position is initially funded for 24 months and can be extended for additional 12 months. Application deadline: January 26th, 2025.

We are looking for motivated researchers and developers to contribute to a cutting-edge project at the frontier of physics and computing. In the context of the EU-funded project MADDEN, we aim at building a data lake where multiple experiments in the Gravitational Wave community can seamlessly share and analyse experiment data based on FAIR principles. The work will be carried out within a multidisciplinary team of physicists, software engineers, and computer scientists collaborating in a stimulating and international environment.
For details, check out the MADDEN project here.

To apply:

  • go to: https://jobs.dsi.infn.it/index.php and search for grant number 27414.
  • Deadline for application is January 26, 2025 and it will be possible to take the interview for the selection process in videoconference.
  • Candidates should hold a second level degree in Engineering, Computer Science, Physics, Mathematics (or an equivalent degree obtained outside Italy) for no more than 9 years.
  • The annual gross salary is € 25.183,00. The net salary according to the current regulations is €1.850,04. This number might be subject to change. There will be compensation for winners who obtained their degree outside Turin, in the interest of encouraging mobility.

Feel free to contact federica.legger(at)to.infn.it for further details and information.

Please find here details.

Geometric Foundations of Gravity 2025, June 30 – July 4 in Tatu

is a conference dedicated to the various approaches to gravity that venture beyond the basic formalism of general relativity, i.e., the description in terms of a massless metric field in Riemannian geometry derived from the Einstein-Hilbert action. The topics will range from the foundational issues to the applications in cosmology, gravitational waves, black holes, and other objects.

The meeting will take place on June 30 – July 4, 2025 in Tartu, Estonia. It is a continuation of a series of earlier conferences and workshops on the related subjects.

The topics under discussion include for instance:

  • Extensions of general relativity (metric-affine gravity, Poincare gauge gravity, scalar/vector/tensor gravity, teleparallel gravity, massive gravity, bi-metric gravity, etc)
  • Phenomenology of extended gravity (black holes, ordinary/neutron/boson/grava stars, gravitational waves, cosmology, dark energy, dark matter, galaxies, early universe etc)
  • Beyond Lorentzian geometry in classical and quantum gravity (doubly/deformed relativity, standard model extension, Hamilton geometry, Finsler geometry, etc).

The last day of the conference is planned for hands on tutorial workshops on using computer algebra in gravity theory calculations, focussing on free specialized software packages Cadabra and SymPy (tensor).

The conference is organized by the gravity research group at the Laboratory of Theoretical Physics, Institute of Physics, University of Tartu.

Invited speakers

  • Kirill Krasnov (Nottingham)
  • Prado Martín-Moruno (Madrid) TBC
  • Nicoleta Voicu (Brasov)
  • Thomas Złośnik (Gdansk)
  • TBA

Organizing committee

  • Sebastián Bahamonde (Tokyo)
  • Daniel Blixt (Napoli)
  • María José Guzmán Monsalve (Tartu)
  • Manuel Hohmann (Tartu)
  • Damianos Iosifidis (Tartu)
  • Laur Järv (Tartu)
  • Sotirios Karamitsos (Tartu)
  • Purnendu Karmakar (Tartu)
  • Tomi Koivisto (Tartu)
  • Christian Pfeifer (Bremen)
  • Margus Saal (Tartu)
  • Jorge G. Valcárcel (Pohang)
  • Aneta Wojnar (Wrocław)

Conference Website

28th Capra Meeting on Radiation Reaction in General Relativity, July 21-25, 2025 in Southampton

The 28th Capra Meeting on Radiation Reaction in General Relativity will be hosted by the Gravitational Waves Group at the University of Southampton from 21st - 25th July 2025.

The conference will be hosted at the Centenary Building (Building 100) on the University of Southampton’s Highfield Campus. The five days will be filled with contributed talks and extensive discussion sessions.

The conference will be held primarily as an in-person event with live remote participation via Zoom.

There is no registration fee. The registration page is here. All participants are expected to adhere to the Capra Code of Conduct.

Organising committee: Adam Pound, Jonathan Thompson, Zachary Nasipak, Leor Barack, Alexander Grant, Lorenzo Kuchler, Jack Lewis, Ayush Roy, David Trestini, Sam Upton, Aditya Vaswani

Please contact capra28(at)caprameeting.org for any queries.

Meeting Website

PhD opportunities at the Institute of Space Sciences (ICE-CSIC & IEEC)

Possibility of pursuing a PhD in gravitational wave physics at the Institute of Space Sciences (ICE-CSIC) in Barcelona [see a description below] through the: Doctoral INPhINIT Incoming fellowship program of the LaCaixa Foundation. Application deadline: January 23rd, 2025, at 2 pm CET.

Candidates must not have resided or carried out their main activity (work, studies, etc.) in Spain for more than twelve months in the three years immediately preceding the closing date of the call.

The ICE-CSIC, as a research centre accredited with the Spanish Seal of Excellence María de Maeztu will support applications of interested candidates to work in any aspect of gravitational wave astronomy, from instrumentation to theory. ICE members participate in LISA, LVK, and ET.

Contact: Carlos F. Sopuerta (carlos.f.sopuerta(at)csic.es), Sascha Husa (sascha.husa(at)csic.es), Miquel Nofrarias (nofrarias(at)ice.csic.es)

Please find here full details.

Postdoctoral position in theoretical gravitational Physics at Charles University, Prague

The Institute of Theoretical Physics at Charles University, Prague, invites applications for a postdoctoral position in general relativity and modified theories of gravity within Dr. Ivan Kolar’s research group. This position is funded by the Charles University PRIMUS grant “Spacetimes and Fields in Higher-Derivative Theories” (PRIMUS/23/SCI/005).

Research areas include higher-derivative gravity, exact solutions (e.g., black holes), spacetime symmetries, and algebraic classification.

Applicants should hold a Ph.D. in theoretical or mathematical physics with a strong background in general relativity. Familiarity with computational tools such as xAct/Mathematica is advantageous.

Expected Start Date: March 01, 2025, or negotiable

Duration of Contract: 2 years

Application Submission Deadline: January 10, 2025 at 23:59 CET

Documents Required for the Application:
-structured CV
-education credentials, proof of academic degrees, and ranks
-list of scientific and publication activity
-motivation letter
-two letters of recommendation

See the attached link for more details on the position and application instructions.
Contact: Kolar, Ivan (positions(at)matfyz.cuni.cz)

Please find here details.

2nd School on Black Holes and Gravitational Waves, February 10-14, 2025, Chennai

Centre for Strings, Gravitation and Cosmology (CSGC) - a research centre instituted as part of Institute of Excellence (IoE) initiative of the Government of India at the Indian Institute of Technology Madras (IIT Madras), Chennai, India is organizing the  

2nd School on Black Holes and Gravitational Waves
Feb 10 (Mon) - Feb 14 (Fri), 2025

The proposed school is intended to introduce beginning Ph.D. students and Postdoctoral fellows to research themes of current interest in Black hole physics and Gravitational waves. The lectures will be complemented by tutorial sessions that will help provide hands-on experience to the participants in employing the tools and techniques discussed in the lectures directly in their research work. Topics that will be the focus of the lectures are:

  1. Gravitational self-force and tidal effects in black hole dynamics
  2. Numerical Relativity and its applications in cosmology, astrophysics and black hole physics
  3. Observational aspects of black holes and gravitational waves, including experimental tests of GR

We invite the interested researchers to register for the school before Nov 30, 2024. For registration details and other relevant information, please follow the links on the top of the page.

Scientific Organising Committee:

  • Guillaume Faye (IAP, Paris, France)
  • B S Sathyaprakash (Penn State University, US & Cardiff University, UK)
  • Dawood Kothawala, Chandra Kant Mishra, L Sriramkumar (IIT Madras, India)

Local Organising Committee:
Subhodeep Sarkar, Syed Naqvi, Dawood Kothawala & Chandra Kant Mishra (IIT Madras)

School Website

NEB-21: Recent Developments in Gravity, September 1-4, 2025, Corfu, Greece

The 21st conference in the series "Recent Developments in Gravity" (NEB) is co-organized by the "Hellenic Society for Relativity, Gravitation and Cosmology" (HSRGC) and the Research Laboratory "Mathematical Physics and Computational Statistics" of the Ionian University. It will take place in Corfu, in September 1-4, 2025. The conference is hosted by the Ionian University in Corfu Town.

The topics of the conference are:

Gravitational Waves
Relativistic Astrophysics
Alternative Theories of Gravity
Mathematical Relativity
Cosmology
Quantum Gravity

Plenary Speakers are:

Leor Barack (University of Southampton)
Sebastiano Bernuzzi (University of Jena)
Fabrizio Canfora (San Sebastian University)
Katerina Chatziioannou (California Institute of Technology)
Peter Dunsby (University of Cape Town)
Lavinia Heisenberg (Zurich, ETH)
Vladimir Karas (Astronomical Institute, Czech Academy of Sciences)
Claudia De Rham (Imperial College London)
Alicia Sintes (Balearic Islands University)
Constantinos Skordis (Institute of Physics, Czech Academy of Sciences)
Nikolaos Stergioulas (University of Thessaloniki)

You will find the Registration information in this link.

ERC-funded Postdoc and PhD positions on gravitational-wave theory, source modeling, and science interpretation at the MPI for Gravitational Physics in Potsdam

The "Astrophysical and Cosmological Relativity" (ACR) department at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute, AEI) in Potsdam Science Park announces the opening of several Ph.D. students and postdoctoral appointments in gravitational-wave theory, source modeling, and science interpretation. Successful candidates will join the GWSky project, which an ERC Synergy Grant  has recently funded. We are particularly interested in hiring creative and highly motivated candidates who can work collaboratively and independently in a vibrant, welcoming, and synergistic group. The deadline for full consideration is December 6, 2024.

The ERC-funded project called “Making sense of the unexpected in the gravitational-wave sky (GWSky)” is led by PIs Alessandra Buonanno, head of the ACR department, Enrico Barausse (SISSA, Trieste, Italy), Zvi Bern (University of California, Los Angeles, US), and Maarten van de Meent (Niels Bohr Institute, Copenhagen, Denmark). Given the synergistic aspect of the GWSky project, we anticipate that for a few postdoctoral scholars, there will be the opportunity to spend two years at the AEI and the subsequent two years in another node. One of the supervisors of the Ph.D. students at the AEI may be located in another node.

The aim of the GWSky project is to use gravitational-wave measurements by existing and future observatories on the Earth and in space as precision laboratories for fundamental physics, cosmology, and astrophysics. This includes the current LIGO-Virgo-KAGRA detectors, as well as the future ground-based observatories Cosmic Explorer and Einstein Telescope, and the space-based detector LISA. By leveraging the PIs and their groups’ expertise, the GWSky project aims to develop a groundbreaking framework capable of solving the highly nonlinear equations by Einstein’s General theory of Relativity, creating waveform models with unprecedented accuracy, and translating these results into practical tools for interpreting the data.

As a consequence, we are looking at candidates in the following research areas: post-Minkowskian formalism, scattering amplitudes, gravitational self-force, post-Newtonian theory, effective-one-body formalism, numerical-relativity surrogate models, methods to accelerate waveform generation, numerical-relativity simulations in General Relativity and alternative theories of gravity, environmental effects for binary systems, tests of General Relativity, gravitational-wave data analysis and machine learning.

To apply, please submit your application via our job portal
for the postdoctoral positions here.
for the PhD positions here.

You will be asked to upload a cover letter, curriculum vitae, list of publications and a statement of past and future research activities of not more than 3 pages. Ph.D. applicants will also be asked to upload their university transcripts and Master thesis (if applicable). Applicants will need to indicate the names of three referees for recommendation letters. Please Register an account with our job portal and fill in the contact information for the referees well before the deadline, so that reference letters can be received in time. Referees will receive an email with instructions on how to upload their letters. In case of technical problems with the application form, please contact jobs(at)aei.mpg.de.

The four nodes of GWSky will have positions in a variety of subdisciplines that feed into precision theoretical studies of gravitational waves. Those interested in potential positions at other nodes may follow the links:

Candidates are encouraged to apply as soon as possible. The deadline for full consideration, including receipt of reference letters, is December 6, 2024. The anticipated start date of the positions is Fall 2025. Applications will be considered until all positions are filled.

The salary and social benefits (e.g., health insurance) are based on the collective labor agreement “TVöD Bund” for the German public sector, usually at pay grade E13 (if the qualifications according to TVöD are met). In case an offer is made, a projection of the gross and net salary based on the TVöD regulations will be prepared.

The Max Planck Institute for Gravitational Physics is an equal opportunity employer and is committed to providing employment opportunities to all qualified applicants without regard to race, color, religion, age, gender identity, sexual orientation, or national origin. The Max Planck Society is committed to increasing the number of individuals with disabilities in its workforce and, therefore, encourages applications from such qualified individuals. The AEI and the Max Planck Society welcome persons with diverse backgrounds, experiences, and ideas who embrace and value diversity and inclusion (Code of Conduct). The institute promotes a healthy work-life balance by offering all employees a family support service, cooperation with a nearby international kindergarten, and an in-house parent-child office and nursing room.

For further information, please contact acr-jobs(at)aei.mpg.de.

Please find here full details.

Scientific Machine Learning for Gravitational Wave Astronomy, June 2-6, 2025 in Providence, Rhode Island

The aim of this workshop is to bring together participants from computational mathematics and gravitational wave astronomy to tackle computational challenges in leveraging data-driven methods in key areas of gravitational wave data analysis in order to maximize the science output of the ongoing and upcoming observations. The areas of focus will be: (i) noise classification and detection, (ii) waveform modeling and uncertainty quantification, and (iii) source parameter and astrophysical population Bayesian inference.

The participants will develop and apply new mathematical and computational techniques including: (i) neural network classifiers for distinguishing signals from instrumental noise, (ii) generative machine learning models for simulating realizations of non-Gaussian and non-stationary stochastic processes, (iii) surrogate models including uncertainty quantification, (iv) stochastic sampling, neural posterior estimation leveraging deep neural networks with normalizing flows or diffusion models, and (v) hierarchical Bayesian inference with non-parametric models such as Gaussian processes and simulation-based / approximate Bayesian approaches.

Workshop Website