Applications are invited for a PhD position in the Quantum Gravity group at the Institute for Mathematics, Astrophysics and Particle Physics (IMAPP) of the Radboud University in Nijmegen, the Netherlands. The successful applicant will work under the supervision of Dr. Timothy Budd and will be funded as part of the NWO START-UP project “New routes towards quantum gravity in the ultraviolet”, which aims at the study of spacetime geometry at the smallest of scales with the help of the latest mathematical techniques and numerical methods. The Quantum Gravity group, consisting of three full-time and two part-time faculty and several postdocs and PhD students, provides an active and stimulating environment for fundamental research in the quantum aspects of spacetime and gravity.

Applicants must have a university degree in physics or mathematics at the masters level or equivalent, with proven abilities in theoretical physics and interests in quantum gravity. Affinity in any of the following topics is considered an advantage but not essential: computer simulations and Monte Carlo methods, statistical physics and critical phenomena, probability and stochastic processes, enumerative combinatorics.

The PhD position is for four years, which is the expected time for obtaining a doctoral degree in the Netherlands, and is subject to review after one year. Salary and benefits are in accordance with the collective labour agreement (CAO) of the Dutch universities. Starting date of the position is to be agreed upon.

Applications will be considered until the position is filled, but those received by October 16th, 2018 are guaranteed full consideration. To apply the following documents should be sent electronically in pdf-format to T. Budd (T.Budd[AT]science.ru.nl): cover letter; CV; transcript of university courses and grades; (brief) statement of research interests.

We encourage applications from women, racial and ethnic minorities, and individuals with disabilities.

Institute of Physics, Jagiellonian University, invites applications for a PhD fellowship within the research project “Dynamics in spatially confined Hamiltonian systems” funded by the Polish National Science Centre.

The goal of this project is to advance understanding of propagation of nonlinear waves in spatially confined systems. We are looking for a well motivated student of physics or mathematics with good analytic solving skills.

Applications and inquiries should be sent to prof. Piotr Bizon at bizon[AT]th.if.uj.edu.pl. The deadline for applications is August 31, 2018.

The Gravitational Theory division at the University of Jena anticipates the opening of PhD positions with starting date in fall 2018 / early 2019. The positions are associated with the research group of Prof. Sebastiano Bernuzzi at the Theoretical Physics Institute. There is the opportunity to participate to a wide range of research activities in numerical relativity, gravitational-wave modeling and data analysis or related analytical and computational methods. Applicants with a background in the above areas are especially encouraged to apply. The successful candidates have the opportunity to join the Virgo Collaboration and participate to the LIGO-Virgo gravitational-wave astronomy effort.

For information on the Theoretical Physics Institute visit: https://www.tpi.uni-jena.de/HomePage
For information on the research group visit: http://www.tpi.uni-jena.de/~bernuzzi

Applications sent by June 1, 2018 will receive full consideration; applications after this date are still welcome until the positions are filled. In a situation where two candidates have otherwise equal qualifications, preference will be given to women, minorities, and handicapped applicants.

Please submit a cover letter, a curriculum vitae with a list of publications, a brief description of research interests, and a list of potential referees, who may be contacted separately. Please send applications to:

sebastiano.bernuzzi[AT]uni-jena.de
Theoretisch-Physikalisches Institut
Friedrich-Schiller-Universitaet Jena
MAX Wien Platz 1
D-07743 Jena, Germany
Office 209

Please use the string “Application for PhD position – SURNAME NAME” in the email subject and use the PDF format for all your files.

The Virgo group at Nikhef has openings for several PhD students in gravitational wave data analysis.

Nikhef is the national institute for subatomic physics in The Netherlands, where approximately 175 physicists and 75 technical staff members work together in an open and international scientific environment. Together they perform excellent theoretical and experimental research in the fields of particle and astroparticle physics. Among the research collaborations Nikhef participates in are the ATLAS, LHCb and ALICE experiments at CERN, the KM3NeT neutrino telescope in the Mediterranean, the Virgo interferometer in Pisa, the XENON Dark Matter detector in Gran Sasso and the Pierre Auger cosmic rays observatory in Argentina. Nikhef is a collaboration between 5 major Dutch universities and the Nikhef research institute.

The successful candidates will work on the development of novel methods for analysing gravitational wave data from the LIGO and Virgo detectors, with a view on directly probing the structure of compact objects such as black holes and neutron stars. They will be members of the Virgo Collaboration, and will have full access to all Virgo and LIGO data.

A master degree in physics is required, and strong programming skills are highly desirable. The students will be employed by the NWO-I-foundation as junior scientists. They will receive a 4 year contract with a competitive salary. The conditions of employment of the NWO-I-foundation are excellent and can be found on the website of the employer: http://www.nwo-i.nl.

The educational programme of the Dutch research school for subatomic physics offers annual graduate schools for PhD students, as well as frequent series of lectures on advanced topics in (astro)particle physics.

Qualified applicants are encouraged to apply through the online portal: https://www.nikhef.nl/en/vacancies/. Please be prepared to upload a curriculum vitae and have the email address ready of at least one referee who is willing to send a letter of recommendation on your behalf. The deadline for applications is May 15th, 2018.

Further information on these positions can be obtained from Prof. Dr. Chris Van Den Broeck (vdbroeck[AT]nikhef.nl).

PPGCosmo is an international PhD program on Astrophysics, Cosmology and Gravitation that aims to give PhD students the opportunity to develop a successful international scientific career. The research topics range from theoretical to observational aspects of Astrophysics, Cosmology and Gravitation, including participation in collaborations such as LIGO, Euclid, J-PAS and DES. PPGCosmo is a Brazilian program consisting of five institutions from Brazil and four institutions from outside Brazil.

The call for applications for four 4-year PhD positions starting in August 2018 is now open. The student will be supervised by a Professor at a Brazilian institution and co-supervised by a Professor at an institution outside Brazil. For the compulsory postgraduate courses the student will be mainly based in Vitória (Espirito Santo, Brazil). It is expected that the student will have opportunities to visit the other Brazilian participating institutions and the co-supervisor’s non-Brazilian institution.

Please go to http://ppgcosmo.cosmo-ufes.org/home.html for further information.

The Relativity group at the University of Otago, New Zealand invites applications for a PhD position in General Relativity, in particular on the gravitational wave emissions of rotating neutron stars. The position comes with a 3-year scholarship which covers tuition fees as well as an annual stipend of 25000 NZD.

The position is related to a Catalyst:Seeding grant from the Royal Society of New Zealand to J. Frauendiener to work on neutron star mountains and their gravitational wave signals. The project is joint with Prof. Andrew Melatos (University of Melbourne, Australia) and Prof. Susan Scott (Australian National University, Canberra) both members of OzGrav, the Australian Centre of Research Excellence for Gravitational Wave Discovery.

We are looking for a motivated person with a degree equivalent to MSc or BSc(Hons) in Theoretical or Mathematical Physics. Good mathematical skills are essential. Prior research experience in General Relativity or relativistic astrophysics is desirable.

The starting date of the position is on 1.6.2018. The position will be open until filled.

Please send applications (including CV and certificates) or any enquiries to joergf[AT]maths.otago.ac.nz.

This PhD project is mainly devoted to the study of cosmological inhomogeneities in two different “bounce” scenarios, in which the classical Big Bang singularity is resolved by quantum effects. The first of these scenarios describes the Universe as a “condensate” of a large number of quantum atoms of geometry within the group field theory approach to quantum gravity. The second scenario uses symmetry-reduced models with in which the Universe can make a quantum transition from a contracting to an expanding phase. The project will study cosmological perturbations within these two bounce models, explore potential observational signatures, and focus on the connection to other bounce scenarios and formalisms for quantum cosmology, such as loop quantum cosmology or the no-boundary proposal for quantum cosmology.

The PhD studentship is associated to the Royal Society University Research Fellowship project “Addressing the Big Bang singularity in quantum gravity and quantum cosmology” by Dr Steffen Gielen.

We are looking for an enthusiastic applicant with a first class degree in Theoretical/Mathematical Physics or equivalent (strong mathematical background is essential), preferably at MSc/MMath level, or equivalent non-UK degree. Candidates with a 2:1 degree can be considered in exceptional cases. Prior research experience in quantum cosmology or cosmological perturbation theory would be an advantage, but is not essential.

The studentship is for four years, and covers tuition fees at the Home/EU rate as well as a stipend of currently £14,553 per year.

Starting date can be October 2018 or earlier; the position will be open until filled.
Review of applications will begin shortly, so early application is strongly recommended. Please write to the email address above if you are interested in applying.

The Faculty of Physics, Astronomy and Informatics of the Nicolaus Copernicus University invites applications for a stipend for a three-year PhD student position in theoretical/observational inhomogeneous cosmology. A substantial fraction of the successful candidate’s research work will be expected to focus on the possible links between inhomogeneous cosmology and dark matter. The candidate’s main thesis research topic will be negotiated with his/her thesis supervisor.

The PhD stipend will be a part of the Theme 3: Theoretical investigation of general-relativistic effective contributions to dark matter fields of the A next-generation worldwide quantum sensor network with optical atomic clocks project, carried out within the TEAM programme of the Foundation for Polish Science.

More info and how to apply: https://euraxess.ec.europa.eu/jobs/278460

The Institute of Theoretical Physics IFT UAM-CSIC in Madrid (Spain) is offering a PhD position in theoretical cosmology

The position will have a duration of 3 years and is funded by an “Atraccion de Talento Investigador” grant awarded by the regional government of Madrid to Dr. Guillermo Ballesteros. An eventual extension of the position to a fourth year will be subject to the availability of funding.

The position should begin in autumn 2018, although the starting date is flexible. Candidates interested in topics such as inflation, dark energy, dark matter and wanting to work at the interface between cosmology and particle physics are encouraged to apply. They must hold an M. Sc. (or an equivalent degree) by their intended starting date.

Applications (in PDF format) can be sent by e-mail to guillermo.ballesteros[AT]uam.es with the subject “PhD-IFT-MAD Application”. They must contain: a curriculum vitae, a transcript of academic records and a brief statement of motivation, research interests and previous research experience. Two reference letters should be sent separately to the same e-mail address, with the subject “PhD-IFT-MAD Reference + name of the applicant”.

Review of applications will start around the 5th of April, but applications that arrive after this date will also be considered.

Candidates who have recently applied for a SO(IFT) PhD position do not need to send their materials again, but should write an e-mail indicating their interest in this new position.

Knowledge of Spanish language is not needed, but a good command of English is required.

Enquires about the position can be sent to guillermo.ballesteros[AT]uam.es

PhD scholarships are available at the Nicolaus Copernicus Astronomical Center in Warsaw, Poland. In particular there are projects available in the neutron star group, on neutron star superfluidity and pulsar glitches and on gravitational wave emission in neutron stars, both under the supervision of Dr Brynmor Haskell.

The Nicolaus Copernicus Astronomical Center is one of the leading astronomical institutes in Poland, and the neutron star group is involved in cutting edge research on the equation of state of dense matter, neutron star superfluidity, gravitational wave detection and pulsar glitches.The neutron star group is currently composed of 4 staff members (Pawel Haensel, Leszek Zdunik, Michal Bejger and Brynmor Haskell), 4 postdocs and 3 students.

Warsaw is a vibrant European capital, rich in history and culture, and well connected to other European and international destinations by rail, road and air.

A detailed description of the projects, together with instructions to apply, can be found on the website: https://www.camk.edu.pl/en/phd/

Applications must be received by the Nicolaus Copernicus Institute before March 25th 2018. Applicants are, however, encouraged to contact Brynmor Haskell (bhaskell[AT]camk.edu.pl) well in advance, to discuss potential projects.

PPGCosmo is an international PhD program on Astrophysics, Cosmology and Gravitation that aims to give PhD students the opportunity to develop a successful international scientific career. The research topics range from theoretical to observational aspects of Astrophysics, Cosmology and Gravitation, including participation in collaborations such as LIGO, Euclid, J-PAS and DES. PPGCosmo is a Brazilian program consisting of five institutions from Brazil and four institutions from outside Brazil.

Four 4-year PhD positions are now available starting in mid-March 2018. The student will be supervised by a Professor at a Brazilian institution and co-supervised by a Professor at an institution outside Brazil. For the compulsory postgraduate courses the student will be mainly based in Vitoria (Espirito Santo, Brazil). The student will have opportunities to visit the other Brazilian participating institutions and will have to spend one year at the co-supervisor’s non-Brazilian institution.

Please go to http://ppgcosmo.cosmo-ufes.org/home.html for further information.

The numerical relativity group at the University of Jena anticipates the availability of a PhD position in April 2018.

The position is associated with the research group of Prof. Bernd Bruegmann at the TPI Jena. There is the opportunity to participate in a wide range of research activities. Applicants with a background in numerical relativity, especially in the area of gravitational wave science or associated computational and mathematical methods are especially encouraged to apply.

Please submit a cover letter, a curriculum vitae with a list of publications, a brief description of research interests, and a list of three potential referees, who may be contacted separately.

Applications should be received no later than January 22, 2018, but applications will be considered until the position is filled. In a situation where two candidates have otherwise equal qualifications, preference will be given to women, minorities, and handicapped applicants.

Please send applications referring to Reg.-Nr. 364/2017 to:
lisann.schmidt[AT]uni-jena.de

Lisann Schmidt
Theoretical Physics Institute, University of Jena
Max Wien Platz 1
D-07743 Jena
Germany

The DFG Research Training Group ‘Models of Gravity’ invites applications for positions of Research Assistants, Salary Group (Entgeltgruppe) 13 TV-L 66%, to be appointed April 1, 2018. The positions are limited up to three years.
The Research Training Group consists of gravity groups working at the Universities of Bremen, Oldenburg, Bielefeld, Hannover, Copenhagen, as well as at the Jacobs University Bremen. We intend to obtain a better understanding of Einstein’s General Relativity and of generalised theories of gravity as given by, e.g., string theory. These investigations are also related to observations. More information can be found on the website http://www.models-of-gravity.org

Responsibilities and Duties:
The successful applicants will have the opportunity to work towards a doctoral degree in Gravitational Physics. They are expected to contribute to the teaching programme of the Research Training Group.

Employment conditions:
To qualify for the position, applicants must hold a Master’s degree or a Diploma in Physics, Mathematics or any other relevant discipline, with an above-average success in the present courses of studies. We expect high dedication and teamwork.
All participating universities aim, in particular, to promote women within the scope of the statutory provisions and, hence, emphatically invite qualified women to apply for these positions. Severely disabled applicants are given preferential consideration in the event of equal qualification. Applicants with a migration background are highly welcome.

Application:
The application with a curriculum vitae, certifications, a description of the scientific interest, a conception of the own career, and, if applicable, a list of publications should be sent as one single pdf document via field e-mail to secretariat@models-of-gravity.org
Also two letters of reference should be sent. Closing date is December 15, 2017, although applications will be accepted until the positions are filled.

We are selecting a motivated candidate for the Joint Phd Program between Southern University of Science and Technology (SUSTech, Shenzhen, China) and Hong Kong Science and Technology University and Institute of Advanced Studies (HKUST and IAS, Hong Kong, China). The PhD candidate is suppose to start the program next academic year (September 2018) and the completion of the program will take 4 years. We are particularly interested in candidates with advanced knowledge of General Relativity and Quantum Field Theory.

Title of the project: Classical and Quantum Gravity, String Theory, and Cosmology.
Research Plan — The candidate is suppose to address the cosmological implications of effective string field theory and/or a class of nonlocal gravitational theories finite and unitary at quantum level. Two are the main issues to address: the cosmological constant’s problem and the physics of the early Universe. The consistent theories mentioned above should provide a mechanism for fixing the cosmological constant to the observed value and solve the problem of the initial Big Bang singularity, while also provide a natural mechanism for inflation. Since the nearby location of the two Universities the student will be co-supervised by both the supervisors during the all duration of the PhD program. However, the Phd candidate will have also to attend courses and other duties if required by the agreement of the two Universities: HKUST and SUSTech.
In the first two years we will mostly concentrate on the Dark energy problem and possibly Dark matter problem, while in the second part of the Phd program we will focused on inflations and the computation of two and eventually three point correlation’s functions.

The candidate will work under the supervision Prof. Henry Tye (HKUST and IAS) and Prof. Leonardo Modesto (SUSTech). The Gravitational and High Energy Physics at SUSTech consist on 1 Research Associate Professor, 3 PostDocs, and several undergraduate students.
Interested candidates should send their CV (including, among other things, date of birth and nationality) and a short statement of research interests and/or experience to:
Prof. Leonardo Modesto
E-mail: lmodesto[AT]sustc.edu.cn
Please arrange also at least 2 recommendation letters to be sent separately to the same email address.
Applications received by November 30 will receive full consideration.

The Virgo group at Nikhef has an opening for a PhD student in gravitational wave data analysis.

Nikhef is the national institute for subatomic physics in The Netherlands, where approximately 175 physicists and 75 technical staff members work together in an open and international scientific environment. Together they perform excellent theoretical and experimental research in the fields of particle and astroparticle physics. Among the research collaborations Nikhef participates in are the ATLAS, LHCb and ALICE experiments at CERN, the KM3NeT neutrino telescope in the Mediterranean, the Virgo interferometer in Pisa, the XENON Dark Matter detector in Gran Sasso and the Pierre Auger cosmic rays observatory in Argentina. Nikhef is a collaboration between 5 major Dutch universities and the Nikhef research institute.

The successful candidate will work on the development of novel methods for analysing gravitational wave data from the LIGO and Virgo detectors, with a view on directly probing the structure of compact objects such as black holes and neutron stars. Understanding the neutron star equation of state is a major open problem in astrophysics, which can now be addressed by studying gravitational wave signals from binary neutron star mergers. The student will work on this as part a collaborative effort of the Virgo and ALICE groups at Nikhef. He or she will be a member of the Virgo Collaboration, and will have full access to all Virgo and LIGO data.

The successful candidate has a master in physics. Strong software skills are highly desirable. The student will be employed by the NWO-I-foundation as a junior scientist. He or she will receive a 4 year contract with a competitive salary. The conditions of employment of the NWO-I-foundation are excellent and can be found on the website of the employer: http://www.nwo-i.nl.

The educational programme of the Dutch research school for subatomic physics offers annual graduate schools for PhD students, as well as frequent series of lectures on advanced topics in (astro)particle physics.

Qualified applicants are encouraged to apply through the online portal: https://www.nikhef.nl/jobs/vacatures/. Please be prepared to upload a curriculum vitae and have the email address ready of at least one referee who is willing to send a letter of recommendation on your behalf. The deadline for applications is January 3rd, 2018.

Further information on this position can be obtained from Prof. Dr. Chris Van Den Broeck (vdbroeck@nikhef.nl).

The high energy astrophysics group at Fudan University (Shanghai, China) has a few PhD positions for the next academic year (starting in September 2018). The successful candidates must have a Master degree in Physics or in a related area before September 2018. Courses and research are conducted in English. The PhD program normally lasts for 3 years, but it can be extended to 4-5 years.

We are particularly interested in candidates with interest/experience in:
1) X-ray data analysis of black holes (in particular for spin measurements)
2) Astrophysical codes (fortran, C/C++, python)
We will also consider applications from candidates interested in other lines of research in high energy astrophysics, as well as from candidates interested in theoretical aspects of general relativity and alternative theories of gravity.

The group is led by Prof. Cosimo Bambi and currently consists of 2 postdoctoral researchers and several graduate and undergraduate students. More details on the possible projects can be found on the group webpage.

Interested candidates should send their CV (including, among other things, date of birth and nationality) and a short statement of research interests and/or experience to:

Prof. Cosimo Bambi
E-mail: bambi[AT]fudan.edu.cn

Please arrange also at least 2 recommendation letters to be sent separately to the same email address.

Applications received by November 30 will receive full consideration.

The Department of Mathematical, Physical and Computer Sciences [1] at the University of Parma [2] invites applications for its Ph.D. program. The Ph.D. fellowships start November 1st 2017 and have a duration of 3 years.

The Ph.D. program covers several scientific areas in theoretical physics, including Cosmology, Gravitational physics, Numerical Relativity, Gravitational Waves, Fundamental interactions at high energy, Quantum Field Theory, Lattice Field Theory and Strings, Statistical Physics, Quantum Mechanics and Complex Systems. (See [3] for a summary of the research activity of the Theoretical Physics group).

The submission deadline is September 5th 2017. In the application the candidate must indicate the main research topic (and a second-priority choice) amongst the research topics proposed by the Research Doctorate Program in Physics at the Department of Mathematical, Physical and Computer Sciences. The selection will be based on the curriculum of the candidate and an interview. The interview will focus on the previous research experience and on the research project that the candidate proposes.

Details of the call, on-line application, list of research topics and selection procedures can be found at: http://smfi.unipr.it/it/node/2349

For more information please contact Prof. Cristiano Viappiani (cristiano.viappiani[AT]unipr.it) and Prof. Luca Griguolo (luca.griguolo[AT]unipr.it).

Other links:

[1] http://smfi.unipr.it/it
[2] http://en.unipr.it/
[3] http://www.pr.infn.it/

The Physics department of the University of Trento invites applications for PhD fellowships starting in November 2017.

The PhD fellowships have a duration of 3 years and a gross salary of 13638.47 EUR per year (about 1000 EUR per month after taxes).

The PhD program covers several scientific areas, including also Theoretical and Computational Physics. More details about the doctoral school in Physics can be found at http://web.unitn.it/en/drphys

The Department of Physics includes faculty members working on computational astrophysics (Giacomazzo), nuclear astrophysics (Leidemann, Lovato, Pederiva), gravitational wave detectors (Dolesi, Perreca, Prodi, Vitale, Weber), theory of general relativity and cosmology (Rinaldi, Vanzo, Zerbini). Students with interests in one of these areas are strongly encouraged to apply.

Applications for the doctoral positions are accepted from candidates, regardless of gender, age, and nationality, who have a Master’s degree (equivalent to the Italian “laurea magistrale”). Any degree in Physics or related disciplines will be given preferential status. Applications are also accepted from students who expect to get their degree by October 31 2017.

The University of Trento is ranked among the top 5 universities in Italy and it is characterized by an international and diverse student population. The city of Trento is located on the Italian Dolomites and it is very well connected with several destinations in Italy and Europe.

The deadline for applications is August 30 2017 at 4 pm Italian time. The selection will be based on the curriculum of the candidate and on an oral exam (candidates permanently residing abroad by the date of the oral exam may take the exam by phone or videoconference in their country of residence).

More information about the application process can be found here:
http://www.unitn.it/en/ateneo/1940/announcement-of-selection

One PhD studentship is open at the Institute of Cosmos Sciences at University of Barcelona (ICCUB). It is funded by the ERC Advanced Grant of Prof Roberto Emparan “A New Strategy for Gravity and Black Holes” (ERC2015AdG 692951 GravBHs).

The successful applicant will work directly with Prof Emparan on novel theoretical approaches to black hole physics and gravity. They will be members of a very active group doing research on many areas of gravitational theory, string theory and cosmology.

Candidates must hold an MSc or equivalent in a field that is closely related to theoretical physics, with excellent performance in General Relativity.

The start date is expected to be October 2017. The position will be funded for up to 4 years, and includes travel money.

Applications must be made online at the link below, and will contain a CV

Applications are invited for PhD projects at the Centre for Theoretical Cosmology in the Department of Applied Mathematics and Theoretical Physics.

Project 1: Fundamental physics from gravitational lensing of the CMB

The CMB is gravitationally lensed along its path to us and this signal contains information about early universe physics, the properties of neutrinos and dark energy, and dark matter distributions. The study of CMB lensing at high precision is therefore crucial for the success of future CMB cosmology. This studentship offers a leading role in this exciting new field at the interface of theoretical and observational cosmology. The research can span both novel theoretical development and innovative, computationally intensive data analysis for AdvancedACT and Simons Observatory.

Project 2: Investigating methods for optimal estimation of correlation functions on incomplete domains.

Realistic cosmological data sets have a restricted domain because of experimental effects and foregrounds. This means transforming to harmonic space to find correlation functions is complicated because harmonics are no longer orthogonal. This leads to mode coupling which increases error bars on cosmological observables. Recently we discovered that inpainting of masked regions significantly reduced this coupling allowing for almost optimal estimation of CMB power spectra. This project will apply this methodology to Planck CMB data producing new parameter constraints and then generalize to other data sets like galaxy surveys.

Project 3: Halo clustering and galaxy surveys

Galaxy and weak lensing surveys provide an unprecedented map of the late-time galaxy and matter distribution, which can be used to constrain fundamental physics. This requires an accurate understanding of the non-linearities in the matter distribution and the mapping from the matter to the galaxy formation sites. The latter can be achieved by studying the clustering of peaks in the initial Gaussian field and following the subsequent evolution using perturbation theory. This project will apply this to observational redshift space and statistics beyond two-point functions, like the bispectrum.

Project 4: Detecting new particles in the sky

This proposal will develop the tools to constrain signatures from massive particles in CMB maps.. Such particles are hypothesized in string theory and they have a well determined hierarchy. Interactions of these particles with the inflaton lead to unique signatures in the CMB, including sourcing non-Gaussianities that can be observed in temperature and polarisation measurements. The main outcome of this project will be the first analysis looking for massive particles in CMB polarisation data.

These studentships are part of new STFC Centre for Doctoral Training in Data Intensive Science. The four-year tenure includes training courses in the first year and a flexible six month placement with industrial partners. Applicants should have a masters in mathematics or physics (majoring in theoretical physics or astrophysics) and should be UK or EU nationals. Further information is available at the group website http://www.ctc.cam.ac.uk and preliminary enquiries can be made to contact potential supervisors through James Parke gr-secretary[AT]damtp.cam.ac.uk.

Please submit a formal PhD application to Applied Mathematics and Theoretical Physics at
http://www.graduate.study.cam.ac.uk/how-do-i-apply and send an expression of interest email to grad-administrator[AT]maths.cam.ac.uk explaining which studentship you are interested in and why.

Closing date: 29th June 2017.

Applications will be reviewed on a rolling basis as they are received. Offers may be made before the closing date.

The University values diversity and is committed to equality of opportunity. The Department particularly welcomes applications from women.

Applications are invited for 3-year PhD scholarships in Mathematical or Computational Relativity, at the University of Otago, New Zealand.

The Relativity Group at the University of Otago consists of three permanent staff (F. Beyer, J. Frauendiener and J. Hennig) and, currently, two PhD students and one Master student. The research interests include mathematical and numerical properties of the conformal field equations, gravitational waves, Fuchsian methods, cosmological space-times, exact solutions, transformation optics etc.

A University of Otago Doctoral Scholarship provides an annual emolument of 25,000NZD plus tuition fee waiver for 3 years. Applicants should have a First Class honours degree, Masters degree, or equivalent, specialising in an area of Applied Mathematics, preferably with some prior knowledge in General Relativity and numerical methods. The scholarships are available to both International and Domestic students.

Interested? Then, you should apply for a University of Otago Postgraduate Scholarship by downloading the appropriate application form the Scholarships Office website at http://www.otago.ac.nz/study/scholarships

Enquiries to: Prof. J. Frauendiener
(Phone: +64 3 479 7770, Email: joergf[AT]maths.otago.ac.nz )