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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.

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.

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.

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.

PhD positions in Theory and Phenomenology of High Energy Physics at RWTH Aachen

Prof. M. Czakon and Prof. M. Worek invite applications for Ph.D. positions in theoretical particle physics (hep-ph) with a starting date in the fall of 2024. The PhD projects concern precision Standard Model predictions for the LHC, perturbative QCD, top quark and Higgs boson physics. The recipients will be hosted by the Institute for Theoretical Particle Physics and Cosmology, RWTH Aachen University, Aachen, Germany. The deadline for applications is June 7, 2024.

We explicitly encourage applications from qualified women. Applicants with disabilities will be given preference if equally qualified.

More information about the Institute for Theoretical Particle Physics and Cosmology, RWTH Aachen University can be found at:

https://www.particle-theory.rwth-aachen.de

The PhD positions are funded by the German Research Foundation (DFG) and by the German Federal Ministry of Education and Research (BMBF). The PhD students will be eligible for association with

  • the Research Training Group: Physics of the Heaviest Particles at the LHC – http://www.rwth-aachen.de/rtg2497
  • the Transregional Collaborative Research Centre: P3H – Particle Physics Phenomenology after the Higgs Discovery – https://p3h.particle.kit.edu/.

Please enclose in the application:

  • cover letter stating your interests, motivation, and preference for either Prof. Czakon or Prof. Worek
  • research statement,
  • curriculum vitae,
  • degree certificates and study transcripts with a description of the grading scheme,
  • abstract (maximum half a page) of your diploma or masters thesis,
  • list of your publications (if any).

Please arrange for 2 letters of recommendation to be submitted via AcademicJobsOnline.org.

Shortlisted candidates will be invited for a job interview shortly after the deadline. The job interview will include:

  • an oral scientific presentation (20 minutes) given by you on a subject of your choice,
  • an interview to gain a deeper understanding of your knowledge and motivation.

Please find here full details.