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Teaching Professor in Astronomy and Astrophysics at Penn State

The Department of Astronomy and Astrophysics at Penn State invites applications for a full-time Teaching Professor position (non-tenure track) to begin in Fall 2025. Salary and benefits will be competitive and commensurate with the successful candidate’s qualifications and experience.

Responsibilities will include teaching up to 3 courses per semester and advising undergraduate majors. The courses include both classroom and online formats. The Department also plans to develop a Planetary Sciences Option for the undergraduate Astrophysics major. It is our hope to grow this into a Planetary Sciences major in concert with the Geosciences department and others. The successful candidate will have experience with similar duties and be expected to lead these efforts. Course relief and supplementary salary can be provided given additional service to the department including departmental committee work, New Student Orientation, contributions to outreach, and development of course materials, for example.

A Ph.D. in Astronomy or Physics is preferred, a PhD in a related field with strong astronomy teaching experience will be considered. Experience teaching pre-service or in-service teachers and/or experience in astronomy education research is also preferred. Planetarium presentations and volunteer training experience will be considered.

Applications must be submitted electronically and include a cover letter, CV, statement of teaching experience and interests as well as research interests, and a list of publications. In addition, please request three reference letters be sent to astro-jobs(at)psu.edu. Review of applications will begin immediately and continue until the position is filled.

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Launch of UPSaclay-STAR-phi Postdoctoral Fellowship Programme University Paris-Saclay

The Graduate School of Physics at Université Paris-Saclay (France) is launching a new postdoctoral fellowship programme: UPSaclay-STAR-phi, supported by the EU Marie Curie COFUND programme. Application deadline: July 31st, 2025.

The programme will recruit up to 41 international postdoctoral researchers over two calls, for 24-month research projects in one of the 40 laboratories of the Graduate School, at the SOLEIL synchrotron, or at the French National Metrology Lab (LNE). This includes 4 astrophysics laboratories: the Department of Astrophysics (DAp) of CEA Paris-Saclay, the Institut d’Astrophysique Spatiale (IAS), the Laboratoire Atmosphères et Observations Spatiales (LATMOS) and the Laboratoire de Physique des Plasmas (LPP).

  • First call opens: May 1st, 2025.
  • Application deadline: July 31st, 2025.
  • Expected start of fellowships: early 2026 (flexible).

Applicants will propose their own research project aligned with the School’s wide-ranging fields, from fundamental to applied physics.

Notice that the postdoctoral candidate must not have been based in France for more than 12 months, during the past 3 years.

Website of the programme: http://www.cofund-physics.universite-paris-saclay.fr/
Contact: Frédéric Galliano frederic.galliano(at)cea.fr

Please find here details.
https://inspirehep.net/jobs/2916789

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/).

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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.

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.

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)

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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.

One year postdoc position in Maastricht on ET mirror development – application deadline 11th Oct

The Gravitational Waves and Fundamental Physics (GWFP) at the University of Maastricht, member of the Nikhef partnership, has a position for a postdoctoral researcher under supervision of Dr. J. Steinlechner.

Job Description
Carrying out research and development on instrumentation for gravitational wave detection. In particular;

  • Development of silicon mirrors for future, cryogenic gravitational-wave detectors; the project includes characterisation and improvement of the silicon mirror substrate material and of the highly-reflective, low-noise coatings.
  • Collaborating with a variety of national and international research partners, including the Einstein Telescope collaboration, the Virgo collaboration, the LIGO Scientific Collaboration, and the ETpathfinder team.
  • This 1.0 FTE position is based in the Department of Gravitational Waves and fundamental Physics, located at Duboisdomein 30, Maastricht.

Requirements

  • PhD degree in physics or a related field
  • Proficient in English language and good communication skills
  • Experience in research relevant for gravitational wave instrumentation
  • You can work independently
  • You are flexible in collaboration with others
  • Experience in the characterization of mirror and coating materials for optical absorption and mechanical loss would be an advantage

What we offer
As Postdoctoral Researcher in mirror development for ET at Faculty of Science & Engineering, you will be employed by the most international university in the Netherlands, located in the beautiful city of Maastricht. In addition, we offer you:

  • Good employment conditions. The position is graded in scale 11 according to the UFO profile Researcher, function level 11 with corresponding salary based on experience ranging from € 4332 to € 5929 gross per month (based on a full-time employment of 38 hours per week). In addition to the monthly salary, an 8.0% holiday allowance and an 8.3% year-end bonus are applicable.
  • An employment contract for a period of 12 months with a scope of 1.0 FTE.
  • At Maastricht University, the well-being of our employees is of utmost importance, we offer flexible working hours and the possibility to work partly from home if the nature of your position allows it. You will receive a monthly commuting and internet allowance for this. If you work full-time, you will be entitled to 29 vacation days and 4 additional public holidays per year, namely carnival Monday, carnival Tuesday, Good Friday, and Liberation Day. If you choose to accumulate compensation hours, an additional 12 days will be added. Furthermore, you can personalize your employment conditions through a collective labor agreement (CAO) choice model.
  • As Maastricht University, we offer various other excellent secondary employment conditions. These include a good pension scheme with the ABP and the opportunity for UM employees to participate in company fitness and make use of the extensive sports facilities that we also offer to our students.
  • Last but certainly not least, we provide the space and facilities for your personal and professional development. We facilitate this by offering a wide range of training programs and supporting various well-established initiatives such as ‘acknowledge and appreciate’.

Apply now, no later than 11th October 2024 for this position. The application should include a motivation letter, a CV, and any relevant certificates. Final selection will take place through interviews.

Please find here full details.

Postdocoral researcher in cosmology at Leibniz-Institut für Astrophysik Potsdam

The Leibniz-Institute for Astrophysics Potsdam (AIP), Cosmography and Large-scale structure research group, invites applications for a Post-doctoral Researcher in Cosmology (w/m/d).

The position can focus on large-scale structure, galaxy formation, and the cosmic web. However research in the group is more expansive and includes dwarf galaxies, the structure and formation of the Milky Way, computational cosmology, observational cosmology, cosmographic reconstructions of the Local Universe and Constrained Simulations. We invite applicants with experience in either or both observations and simulations to apply.

The position is a research fellowship in the context of the Horizon-EU funded network including the Observatory at the University of Tartu (Estonia), the Kapteyn Institute of the Royal University of Groningen (The Netherlands), and The University of Lorraine (France). The position’s scope will also overlap within the Constrained Local UniversE Simulations (CLUES) collaboration, of which AIP is a node. In addition to the cosmography and large-scale structure group led by Dr Libeskind, the cosmology section at AIP includes Prof. Pfrommer and Dr Puchwein as well as around two dozen postdocs and students.

The start date is negotiable, but expected to be Fall 2024 or Winter of 2024/2025. The position will include generous travel and computing support. The initial appointment will be made for 2 years, with a possible extension, depending on performance and availability of funds. The successful candidate must have a Ph.D. in Physics, Astronomy, or a related field. Salary and benefits are standard for German academic institutions and set at the TV-L level E13. We also provide social benefits incl. company pension VBL as well as a subsidy for a so-called “job ticket” (ie for commuters).

To apply, please send a PDF file containing a research statement (up to 3 pages), a curriculum vitae and publication list, to Dr Noam Libeskind via bewerbung-2024-05(at)aip.de by November 1. Applicants should arrange for 3 letters of recommendation to be sent to the same address by the same date. For questions on the position please contact Dr. Libeskind at nlibeskind(at)aip.de

Please find here full details.