موقعیت‌های خالی در دانشگاه‌های خارج از کشور

[m.arash]

با سلام
این تاپیک در واقع هدفی مشابه تاپیک قبلی با همین عنوان را دنبال می کند با این تفاوت که این تاپیک مختص رشته فیزیک و گرایش های مربوط به آن می باشد!
لطفا برای مشاهده پست های قبلی بر روی لینک قرار داده شده در عبارت زیر کلیک کنید:

* موقعیت‌های خالی در دانشگاه‌های خارج از کشور(تاپیک قدیم)

- یادآوری چارچوب تاپیک:

این موضوع به منظور اعلام موقعیت‌های خالی در گروه‌های تحقیقاتی خارج از کشور ایجاد شده است، تا استادهای دانشگاه‌های خارج از کشور یا سایر اعضایی که از این موقعیت‌ها اطلاع دارند، با اعلام آنها بتوانند دانشجویان مستعد ایرانی را جذب نمایند.

۱. لطفاً از این موضوع تنها برای اعلام موقعیت‌های موجود استفاده نمایید و از ارسال تقاضا برای دریافت کمک هزینه خودداری نمایید.
۲. لطفاً در متن آگهی به نام دانشگاه، کشور، نام رشته و عنوان پروژه اشاره نمایید.
۳. لطفاً شرایط مورد نظر برای دانشجویان علاقمند، مانند مقطع تحصیلی، معدل،‌ حد نصاب برای نمره‌ی امتحانات و ...، را در صورت وجود در متن آگهی اعلام فرمایید.
۴. لطفاً بهترین نحوه‌ی تماس با شما و آدرس وب‌سایت (در صورت وجود) را در متن آگهی بنویسید.
۵. به منظور جلوگیری از سو‌استفاده شرکت‌هایی که اقدام به ارسال دانشجو می‌کنند، آدرس ایمیل باید متعلق به یکی از دانشگاه‌های خارج از کشور باشد.

[m.arash]

درود

من در آینده سعی می کنم از منبع های مختلف و معتبر موقعیت های خالی موجود برای رشته فیزیک رو در اینجا معرفی کنم. موقعیت هایی رو معرفی خواهم کرد که Scholarship حتما داشته باشند. موقعیت های خالی که دارای Scholarship باشند بسیار محدود هستند و شاید تعداد اون ها از انگشت های یک دست در سال تجاوز نکنه! اما سعی می کنم در صورت تاپ بودن موقعیت های عالی که Scholarship برای دانشجوهای Interbnational ندارند رو به صورت موازی نیز معرفی کنم.

یکی از سایت های مفید که تقریبا برای همه رشته ها کاربرد داره سایت زیر هست که شما می تونید خودتون به این سایت برید و موقعیت های مربوط به خودتون رو چک کنید یا در قسمت Subscribe Scholarship Newsletter ایمیل خودتون رو وارد کنید تا به صورت دوره ای از اخبار این سایت که پیرامون موقعیت های خالی است بهره ببرید.

http://scholarship-positions.com

[m.arash]

OPEN POSITION TITLE: AstroMundus 2012 – Erasmus Mundus Masters Course in Astronomy and Astrophysics for International
Announcement Date: August 3, 2011
Study Subject(s):Astronomy and Astrophysics
Course Level:Masters
Scholarship Provider: Erasmus Mundus
Scholarship can be taken at: Austria, Italy, Germany, Serbia

Eligibility:The course is open to students of all nationalities.
Eligible students have a certified good knowledge of the English Language and hold a Bachelor’s Degree in Astronomy, Astrophysics, Physics, or Mathematics, or an equivalent amount of certified learning (3 years of previous studies corresponding to at least 180 ECTS credits) in the same field(s).


Scholarship Open for International Students: Yes

Scholarship Description: A number of Erasmus Mundus scholarships are available both for non-European and European students. The admission to the Masters Course and assignment of scholarships are based on excellence. Admitted students will study in at least 2 and up to 4 of the partner Universities and, upon successful completion of their studies, they will be awarded a Joint Master Degree by all partner universities where they studied during the Masters Course. The course is held in the English language, however students will have the possibility to learn the language of the host countries through courses offered by the host universities.

How to Apply: Online

Scholarship Application Deadline: November 30th, 2011 for both Non-European and European students

Further Scholarship Information and Application

[M.jorfi]

PhD in Physics: Soft Condensed Matter and Photonics.
“Phase transitions of colloidal systems confined to nano-scale architectures”
The Soft Matter and Photonics group (SMP) at the University of Fribourg is offering a Ph.D.
position to a highly motivated and dynamic student who wish to deepens her/his knowledge in
the field of experimental soft condensed matter physics and obtain a doctoral degree in
physics. The Ph.D. will start the first semester of 2012 for a period of three years, which may
be extended by one year.
The aim of the PhD project is to obtain an understanding of the effect of confinement on the
phase behavior of liquids. In particular, we will investigate critical phenomena and ordering
of confined colloidal systems consisting of micrometer size particles. The structure and
dynamics of colloidal systems will be studied by direct observation using modern microscopy
techniques, and we will use two-photon lithography to engineer complex three dimensional
confinement-geometries.
Our group is working on a broad range of topics in soft matter physics and photonics, and the
successful candidate will take part in our ongoing national and international collaborations.
The candidate will also gain expertise in experimental techniques such as laser scanning
confocal microscopy, static and dynamic light scattering, diffusing wave spectroscopy and
rheology.
Eligibility
The candidate should have a background of excellence in experimental and/or theoretical
physics and an internationally-recognized master degree. A previous research experience as
well as computer programing skills are highly recommended but not required. No restrictions
of citizenship apply to the fellowships.
Application procedure
The formal application should be submitted by e-mail to: smpjobs2012@gmail.com . E-mail
submissions must include the mailing label “SMP job” and your last name printed before the
label.
Suitable candidates are requested to submit:
A Curriculum Vitae, including a full address, a contact phone number and e-mail
address and a copy of the passport,
A scanned copy of your University academic transcripts in English,
A scanned copy of the degree, if available at the time of application,
A recommendation letter.

[krig1960]

University of Mainz, Germany Institute for Physics of the Atmosphere PhD Position in Atmospheric Modelling We like to announce a PhD Position at the Institute for Physics of the Atmosphere (IPA), Mainz, Germany This PhD position is part of the project ``Regional Decadal Predictability (DecReg)'', which is funded by the German Federal Ministry of Education and Research (BMBF) in the framework of MiKlip (``Mittelfristige Klimaprognose''). As member of the Earth System Modelling group of the IPA the candidate will work in with the newly developed one-way on-line coupled model system MECO(n) combining the two atmospheric chemistry climate models EMAC and COSMO-CLM/MESSy (www.messy-interface.org). The nominee will evaluate the dependency of the skill of a regional climate model prediction on the setup of the driving (global) model and on the coupling strategy. We are looking for a candidate holding a university degree (master/diploma) in Meteorology, Atmospheric Sciences, Physics or a closely related discipline. Experience in a higher programming language (preferably Fortran90/95), in UNIX/Linux and in numerical modelling of atmospheric processes are advantageous. Interest in numerical modelling of dynamical and chemical processes in the atmosphere is a prerequisite. The position is limited to 3 years. A salary according to TV-L E13 (50 %) is paid. The Johannes Gutenberg University Mainz is an equal opportunity employer and explicitly encourages applications from women. Among equally qualified applicants, disabled candidates will be given preference. For further information contact Ms. Dr. A. Kerkweg (kerkweg@uni-mainz.de, Tel.: +49 6131 3924144) Applications with CV and 2-3 references should be sent via email to Dr. A. Kerkweg (kerkweg@uni-mainz-de). Applications will be screened immediately until the position is filled. The Johannes Gutenberg-University of Mainz in Germany is an Equal Opportunity Employer.

[krig1960]

قابل توجه دوستان رشه ژئوفیزیک گرایش لرزه شناسی:

Call for a PhD in Computational Geodynamics Project Summary The Computational Geoscience Department is seeking a clever and motivated PhD candidate to work on a collaborative project with the University of California, San Diego. The project will concentrate on solving fundamental problems of continental rifting in the presence o a mantle plume using the Afar as a case study. The project will involve strong collaboration with the University of California, San Diego (UCSD) and join an active group of researchers in the Computational Geoscience Department in geology, geophysics, plate tectonics, geodynamics and high performance computing. Project Description Modelling continental rifting is a challenging research topic because continental lithosphere is extremely heterogenous in composition. The material properties of the lithosphere are dependent on this composition as well as pre-existing weaknesses in the material. Complicating the matter further, the rifted part of the continental is usually underneath signicant amounts of water and sediment, perhaps several kilometers. In only two places in the world can these rift flanks be seen on the surface of the planet: Iceland and the East African rift. In the case of Iceland however, the rift occurs through uplifted oceanic crust, while in the African rift system the rift occurs through the African continent. In earlier times, such as the breakup of Pangea, these rifts would have appeared all through the supercontinent seperating it into the continents we know today. Thus, studying the rift allows us to see back in time and look at the early formation of basins along the rift, analogues to the rich oil-bearing basins around the Atlantic for example. The aim is to model rift formation, particularly in the early period, replicating features observed in basins along the East African Rift. Project Aims The project aims at solving some of the fundamental questions regarding the formation of rifting using the Afar as a laboratory: Is rifting in the Afar plume-driven or caused by far-field effects such as boundary forces? Why did rifting initiate in the Red-Sea-Afar-Gulf of Aden triple junction? What is the picture of the mantle flow around East Africa? Why is the volcanism concentrated on the Arabian plate? Is the East Africa rift a failed arm of the triple junction? If so, why? What is the role of pre-exiting lithospheric heterogeneities in influencing the development of the rift? What's Expected The successful candidate engage in high quality research as directed by the project manager and supervisors as well as interact and communicate with other scientist in the department, at UCSD and at international conferences. The candidate must be able to travel and spend time at UCSD for significant periods of time during the 3 year project. Simula offers Excellent opportunities for doing high quality research, as part of a highly competent and motivated team of international researchers Is an equal opportunity employer Generous support for travel and equipment Good office facilities located close to the Oslo fjord and 10 minutes drive from the centre of Oslo, the capital of Norway. Competitive Salary: for a PhD student the starting salary is NOK 395,000 (about EUR49,000 or USD67,000 at current exchange rates) Selection Criteria Essential A Masters degree in geoscience or computational science or equivalent Interest in Earth simulations and computational geoscience Interest in publishing and presenting scientific results Excellent oral and written communication skills in English Strong capacity for team work and for interacting with industry contacts Strong analytical skills Discipline to communicate and document work as it occurs and an ability to work independently and to complete tasks within given deadlines Desirable Programming skills International publication record Application Requirements Interested and qualified applicants should provide the following information by the deadline of June 15, 2012, via email to jobs@simula.no: Cover letter Statement addressing the selection criteria Curriculum Vitae or Resume including a publication list and two references The subject field of your email must include "JOBS 1206 Computational Geodynamics". Applications not meeting these requirements may not be considered. We are interested in how you first came to learn about this position — please let us know in your email. For more information please contact: Stuart Clark, PhD Head of Computational Geoscience stuart@simula.no, +47 47 45 28 70 Martin Linges vei 17, Fornebu, Norway PO Box 134, Lysaker NO-1325 www.simula.no/people/stuart

[TheGeek]

Doctoral position on AGB stars and Optical Interferometry in Vienna, Austria Closing date: 2012-06-15
Contact: Josef Hron
The working group for Asymptotic Giant Branch Stars at the Institute of Astronomy, University of Vienna, is inviting applications for one Doctoral position in the area of stellar atmospheres and optical interferometry.
▾ more
The position is for 3 years and candidates shall have some background in the theory and observation of stellar atmospheres and good programming skills. Knowledge of optical interferometry is an advantage but not required. The PhD work shall be devoted to radiative transfer calculations based on dynamic model atmospheres and a comparison with existing and new interferometric data, in particular those acquired within our own ESO large program. The salary is about €19.000,- per annum (take home, no university fees).

The Institute of Astronomy offers a broad choice of astronomy education and research topics and a very good working environment. The interests and expertise of the AGB-group comprise model atmospheres, molecular and dust spectroscopy, interferometry, abundance determinations, AGB-stars in stellar systems, stellar variability, mass loss and laboratory astrophysics. The group collaborates with many researchers at international level and is involved in HERSCHEL-PACS, MATISSE and ALMA. Further information can be found at www.univie.ac.at/astro .

The position is funded via an Austrian Science Fund project (see www.fwf.ac.at for financial details) and work should start in summer/fall 2012. Applications for the PhD position should consist of a CV, publication list, a statement on the research interests and at least one reference letter.

The material should be sent by June 15, 2012 to:
Prof. Josef HRON
Institute of Astronomy
University of Vienna
Türkenschanzstraße 17
A-1180 Vienna
AUSTRIA
Fax number: +43-1-4277-9518

[abcdeng]

یک موقعیت کاری در انگلستان با حقوق عالی که به عنوان کارمند دانشجو مشغول به کار شده و در پایان قرارداد مدرک دکترا نیز دریافت خواهید کرد.

http://www.jobs.ac.uk/job/AJD762/research-assistant/

موفق باشید

[maryamf]

PhD thesis proposal

Title:
Nuclear magnetic resonance investigations on paramagnetic relaxation enhancement of ultra-high spin clusters

Financing:
International strategic partnership - IDEX program of Université Grenoble Alpes
Monthly gross salary: 1768,55 €

Starting date:
October 2020

Topic:
The Grenoble site of the French National High Magnetic Field Laboratory (Laboratoire Nationale des Champs Magnetiques Intenses, LNCMI) operates a high magnetic field nuclear magnetic resonance (NMR) facility up to 36 T that is used for in-house research and open for external users. The NMR team at LNCMI in collaboration with research groups at Karlsruhe Institute of Technology (KIT, Germany) started a research and development activity on paramagnetic relaxation enhancement (PRE) of NMR relaxivities with paramagnetic polyoxometalates (PM-POMs) as relaxation agents. In the scope of the project a PhD position is available at Grenoble for (i) the development of an NMR PRE platform at Grenoble adapted to the particular conditions of ultra-high field resistive magnets and nuclear magnetic resonance (NMR) frequencies beyond 1 GHz and (ii) systematic NMR PRE studies and modelling over the entire magnetic field range using the NMR facilities at Karlsruhe and Grenoble.

We are looking for a person holding a master’s degree in physics or a related discipline (physical chemistry, biological physics) with strong interest in experimental NMR and instrumentation development.

Application:
Application platform: https://www.abg.asso.fr/fr/candidatO...id_offre/92795
Applicants will have to send an application letter in English and attach:
- Their last diploma
- Their CV
- Letters of recommendation are welcome

More information:
Dr. Steffen Krämer
steffen.kramer@lncmi.cnrs.fr
https://nextcloud.grenoble.cnrs.fr/s/Lq4A9eRPYaGNgFR


--

[TheGeek]

Study of the formation conditions of the first solids in protoplanetary disks and their effect on th Closing date: 2012-06-10
Contact: Jean-Marc Petit
The planetesimals, from which the planets and small bodies of the solar system
are fromed, have a composition that strongly depends on the carbon and oxygen
abundances in the protoplanetary disk, on the reduced state of carbon
(i.e. regions rich in CO compared to those rich in CH4), and on the fraction of
carbon trapped in organic solids. One must thus develop a model linking the
composition of planetesimals created in the disk to its gas phase and its
thermodynamic evolution.
▾ more
Scientific Rationale:
Spectroscopic data from transiting exoplanets allow nowaday to study their atmospheric composition. In the Solar System, gas and icy giants are known to be significantly enriched in heavy elements and volatile species with respect to the Sun. In the case of Jupiter, in situ measurements from the Galileo probe have shown that its atmosphere is enriched in both condensable elements and noble gases (Mahaffy et al. 2000 ; Wong et al. 2004). Spectroscopic observations, in particular from the Cassini spacecraft, have measured similar enrichements in several species in Saturn’s atmosphere (Fletcher et al. 2009a, 2009b). These enrichements are thought to result from the accretion and devolatilization of ice-rich planetesimals during the formation of planetary envelopes. Actually, these enrichements are reproduced from the determination of the volatile phase compostion trapped in planetesimals and the total mass of heavy elements predicted to be in the envelopes by internal structure models (Mousis et al. 2009a). This method was used in the case of the hot Jupiter HD189733b in order to explain how a low metalicity with respect to its host star could be compatible with existing giant planet formation models (Mousis et al. 2009b, 2011). This kind of models also permits to establish a link between the planet's composition and that of the protoplanetary disk from which it formed (Madhusudhan et al. 2011; Mousis et al. 2012).

Thesis objectives:
One of the first goals of this thesis consists in proposing a consistent model describing the chemical composition of planetesimals formed beyond the snow-line as a function of the protoplanetary disk metallicity. The planetesimals composition is supposed to strongly depends on the carbon and oxygen abundances in the disk, on the reduced state of carbon (i.e. regions rich in CO compared to those rich in CH4), and on the fraction of carbon trapped in organic solids. All these parameters strongly influence the fractions of silicates, metals and volatile elements existing in the solid phase. One must thus develop a model linking the composition of planetesimals created in the disk to its gas phase and its thermodynamic evolution. To generate the thermodynamic conditions of the various environments considered in this study, the student will use the EvAD1 model of turbulent accretion disk developed in Besançon. The large variations of metallicity measured in some transiting exoplanets suggest that the accretion conditions of these giant planets may differ widely from those expected for Jupiter and Saturn. The second part of this thesis will consist in simulating the accretion conditions of planetesimals onto the giant planets during their formation via N-body dynamical simulations. This methods allows to better understand the required initial conditions for exoplanets in order to explain their current metallicity. All this work will be conducted in the framework of i) the preparation of the analysis the data from the JUNO mission, currently en route to Jupiter and ii) the interpretation of the forthcoming observations from the future James Webb Space Telescope (JWST).

Expected skills:
The proposed study requires an important modelling effort. Good knowledge and understanding in computer science and numerical analysis (FORTRAN programming, UNIX shell scripting, …) are required. The successful applicant will have solid knowledge in thermodynamics and astrophysics. The work implies strong international collaborations ; fluency in English is needed. Prior knowledge of French, or a demonstrated will to learn it would be a definite plus.

Bibliography:
Madhusudhan, N., Mousis, O., Johnson, T. V., Lunine, J. I. 2011. Carbon-rich Giant Planets: Atmospheric Chemistry, Thermal Inversions, Spectra, and Formation conditions. The Astrophysical Journal, in press (ArXiv e-prints arXiv:1109.3183).

Mahaffy, P. R., Niemann, H. B., Alpert, A., Atreya, S. K., Demick, J., Donahue, T. M., Harpold, D. N., Owen, T. C. 2000. Noble gas abundance and isotope ratios in the atmosphere of Jupiter from the Galileo Probe Mass Spectrometer. Journal of Geophysical Research 105, 15061-15072.

Mousis, O., Madhusudhan, N., Lunine, J. I., Johnson, T. V. 2012. Could Jupiter be a carbon-rich planet ? The Astrophysical Journal Letters, submitted.

Mousis, O., and 15 colleagues 2011. On the Volatile Enrichments and Heavy Element Content in HD189733b. The Astrophysical Journal 727, 77.

Mousis, O., Lunine, J. I., Tinetti, G., Griffith, C. A., Showman, A. P., Alibert, Y., Beaulieu, J.-P., The Holmes Collaboration 2009b. Elemental abundances and minimum mass of heavy elements in the envelope of HD 189733b. Astronomy and Astrophysics 507, 1671-1674.

Mousis, O., Marboeuf, U., Lunine, J. I., Alibert, Y., Fletcher, L. N., Orton, G. S., Pauzat, F., Ellinger, Y. 2009a. Determination of the Minimum Masses of Heavy Elements in the Envelopes of Jupiter and Saturn. The Astrophysical Jou