🇬🇧🇯🇵 Postdoc in GW Astronomy, Cardiff, UK and Tokyo, Japan 🇬🇧🇯🇵
The Institute for Cosmic Ray Research hosts the large-scale cryogenic gravitational-wave telescope KAGRA and is actively involved in instrumental design and commissioning, and gravitational-wave data analysis (Hideyuki Tagoshi, Soichiro Morisaki).
The post is full-time and fixed term until March 2027 with a flexible start date.
Salary: 39,347 GBP per annum (Grade 6.32).
IMPORTANT NOTE TO CANDIDATES: It is the University’s policy to use the person specification as a key tool for short-listing and we only invite candidates to interview who clearly evidence that they meet (or partially meet) each of the essential criteria. During the application process you will be asked to attach a supporting statement. This statement must outline how you meet the criteria below and we recommended formatting this by using each criteria as a sub-heading and providing your relevant experience/evidence below each sub-heading. It is crucial that you save your supporting statement with the vacancy number (eg. 1234BR) in the filename as failure to do so may result in it being omitted from your application.
For informal enquiries about the post please contact Vivien Raymond (raymondv[AT]cardiff.ac.uk), Soichiro Morisaki (soichiro[AT]icrr.u-tokyo.ac.jp)
For informal enquiries about working at Cardiff School of Physics and Astronomy please contact PhysicsHR[AT]cardiff.ac.uk
Job Reference: 18835BR
Link to Online Application: https://krb-sjobs.brassring.com/TGnewUI/Search/Home/Home?partnerid=30011&siteid=5460#jobDetails=2169999_5460
Closing date: Tuesday, 20 August 2024
Please be aware that Cardiff University reserves the right to close this vacancy early should sufficient applications be received.
The Institute for Cosmic Ray Research hosts the large-scale cryogenic gravitational-wave telescope KAGRA and is actively involved in instrumental design and commissioning, and gravitational-wave data analysis (Hideyuki Tagoshi, Soichiro Morisaki).
The post is full-time and fixed term until March 2027 with a flexible start date.
Salary: 39,347 GBP per annum (Grade 6.32).
IMPORTANT NOTE TO CANDIDATES: It is the University’s policy to use the person specification as a key tool for short-listing and we only invite candidates to interview who clearly evidence that they meet (or partially meet) each of the essential criteria. During the application process you will be asked to attach a supporting statement. This statement must outline how you meet the criteria below and we recommended formatting this by using each criteria as a sub-heading and providing your relevant experience/evidence below each sub-heading. It is crucial that you save your supporting statement with the vacancy number (eg. 1234BR) in the filename as failure to do so may result in it being omitted from your application.
For informal enquiries about the post please contact Vivien Raymond (raymondv[AT]cardiff.ac.uk), Soichiro Morisaki (soichiro[AT]icrr.u-tokyo.ac.jp)
For informal enquiries about working at Cardiff School of Physics and Astronomy please contact PhysicsHR[AT]cardiff.ac.uk
Job Reference: 18835BR
Link to Online Application: https://krb-sjobs.brassring.com/TGnewUI/Search/Home/Home?partnerid=30011&siteid=5460#jobDetails=2169999_5460
Closing date: Tuesday, 20 August 2024
Please be aware that Cardiff University reserves the right to close this vacancy early should sufficient applications be received.
Brassring
Job Search Welcome | Cardiff University
Search for Internet job openings.
Forwarded from Particle Physics (Fatemeh Irani)
پژوهشگران در سرن، دقت اندازهگیری جرم کوارک بالا را به طور قابل توجهی افزایش دادهاند.
در سال ۱۹۹۵، زمانی که دانشمندان کوارک بالا را کشف کردند، جرم این ذره را بین 151 تا 197 GeV/c2 تخمین زدند که آن را به سنگینترین ذرهی بنیادیِ شناخته شده، تبدیل کرد. همچنین، از آنجاییکه این مقدار یک ورودی کلیدی برای محاسبات مدل استاندارد (برای پیشبینی پارامترهای مربوط به فرآیندهای نادر) بهشمار میآید، دقت اندازهگیری آن حائز اهمیت است.
اکنون کولبریشنهای CMS و ATLAS در LHC، با جمعآوری پانزده اندازهگیری مختلف، دقیقترین مقدار جرم کوارک بالا را تا به امروز، این مقدار گزارش کردهاند:
172.52 ±0.33 GeV/c2
https://physics.aps.org/articles/v17/s57
در سال ۱۹۹۵، زمانی که دانشمندان کوارک بالا را کشف کردند، جرم این ذره را بین 151 تا 197 GeV/c2 تخمین زدند که آن را به سنگینترین ذرهی بنیادیِ شناخته شده، تبدیل کرد. همچنین، از آنجاییکه این مقدار یک ورودی کلیدی برای محاسبات مدل استاندارد (برای پیشبینی پارامترهای مربوط به فرآیندهای نادر) بهشمار میآید، دقت اندازهگیری آن حائز اهمیت است.
اکنون کولبریشنهای CMS و ATLAS در LHC، با جمعآوری پانزده اندازهگیری مختلف، دقیقترین مقدار جرم کوارک بالا را تا به امروز، این مقدار گزارش کردهاند:
172.52 ±0.33 GeV/c2
https://physics.aps.org/articles/v17/s57
Physics
The Most Precise Value of the Top-Quark Mass to Date
Researchers at CERN have significantly increased the precision of the measured value of the top-quark mass, a key input for making standard-model calculations.
Forwarded from انجمن فیزیک ایران
نشست دویست و شانزدهمین باشگاه فیزیک تهران روز سهشنبه دوم مرداد ماه ۱۴۰۳ به صورت حضوری در سالن آمفی تئاتر دانشکده فیزیک دانشگاه تهران برگزار میشود. برنامه ساعت ۱۵:۳۰ با اخبار فیزیک و مسابقه آغاز می شود. سخنران این نشست دکتر سیما قاسمی، کنشگر ارتباطات علم هستند و درباره «آموزش علم یا آموزش دانش؟» صحبت خواهند کرد.
استفاده از باشگاه فیزیک برای همهی علاقهمندان به علم فیزیک آزاد است.
نشانی صفحه باشگاه فیزیک: www.psi.ir/f/bashgah
⏪ وبگاه انجمن فیزیک ایران:
🌍 http://www.psi.ir
✅ به کانال خبرى انجمن فیزیک ايران بپيوندید:
👇👇🏽👇👇🏽👇👇🏽👇
http://t.me/psinews
استفاده از باشگاه فیزیک برای همهی علاقهمندان به علم فیزیک آزاد است.
نشانی صفحه باشگاه فیزیک: www.psi.ir/f/bashgah
⏪ وبگاه انجمن فیزیک ایران:
🌍 http://www.psi.ir
✅ به کانال خبرى انجمن فیزیک ايران بپيوندید:
👇👇🏽👇👇🏽👇👇🏽👇
http://t.me/psinews
✳️ ستاره شناسان 21 ستاره نوترونی را کشف کردند که به دور ستاره های خورشید مانند می چرخند ✳️
لینک گزارش
@PDATLAB
لینک گزارش
@PDATLAB
phys.org
Astronomers discover what may be 21 neutron stars orbiting sun-like stars
Most stars in our universe come in pairs. While our own sun is a loner, many stars like our sun orbit similar stars, while a host of other exotic pairings between stars and cosmic orbs pepper the universe. ...
School of Particles and Accelerators
Journal Club: Experiments & Phenomenology / Hybrid Format
Date:
Monday, Jul 22, 2024 / دوشنبه، 1 مرداد 1403
Time:
11:00 AM - 12:00 PM (Tehran time)
Speaker:
Mr. Behrad Taghavi
Affiliation:
School of Particles and Accelerators, IPM
Title:
What is (conformal) anomaly?
Title in Persian:
نابهنجاری (همدیس) چیست؟
Abstract:
Inspired by the “What is…?” column in the Notices of the AMS, this talk aims to provide an informal, nontechnical exposition of the fundamental ideas behind various characterizations of anomalies. In the first part of the talk, I will offer a brief summary of multiple mathematical approaches to classifying and characterizing anomalies in quantum field theories. The second part will focus on the specific example of conformal anomaly in two dimensions, illustrating the concepts discussed earlier and highlighting connections with 2D induced gravity and AdS3/CFT2 duality whenever possible.
Meeting Place: Seminar Room, School of Particles and Accelerators, IPM
Link to Join Virtually: https://meet.google.com/bda-vsem-tuv
Journal Club: Experiments & Phenomenology / Hybrid Format
Date:
Monday, Jul 22, 2024 / دوشنبه، 1 مرداد 1403
Time:
11:00 AM - 12:00 PM (Tehran time)
Speaker:
Mr. Behrad Taghavi
Affiliation:
School of Particles and Accelerators, IPM
Title:
What is (conformal) anomaly?
Title in Persian:
نابهنجاری (همدیس) چیست؟
Abstract:
Inspired by the “What is…?” column in the Notices of the AMS, this talk aims to provide an informal, nontechnical exposition of the fundamental ideas behind various characterizations of anomalies. In the first part of the talk, I will offer a brief summary of multiple mathematical approaches to classifying and characterizing anomalies in quantum field theories. The second part will focus on the specific example of conformal anomaly in two dimensions, illustrating the concepts discussed earlier and highlighting connections with 2D induced gravity and AdS3/CFT2 duality whenever possible.
Meeting Place: Seminar Room, School of Particles and Accelerators, IPM
Link to Join Virtually: https://meet.google.com/bda-vsem-tuv
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School of Particles and Accelerators
Special Seminar / Virtual Format
Date:
Monday, Aug 5, 2024 / دوشنبه، 15 مرداد 1403
Time:
10:30 AM (Tehran time)
Speaker:
Prof. Galileo Violini
Affiliation:
Co-chair of the Executive Committee of the Great Caribbean Light Source;
Former UNESCO Representative to Islamic Republic of Iran and Director of Tehran Office
Title:
Synchrotron in the Souths - A Science Diplomacy Challenge
Title in Persian:
سنکروترون در جنوب- یک چالش در دیپلماسی علمی
Abstract:
An advanced light source for research would drive growth in the Wider Caribbean region. In addition to analyzing the need for such a facility to meet Latin America's scientific priorities, the challenges to its construction are discussed. These are very similar to those faced by the African Light Source (AfLS): training of users, ensuring sustainable financing, the possibility of international financial support and the role of international organizations. This perspective of South-South cooperation has attracted the attention and support of other similar facilities, such as SESAME and LNLS, which can play an important role in training and, in the case of GCLS, in project design. The development and success of the corresponding actions, aimed at obtaining political support from the governments of the region and international organizations, mainly UNESCO, may be favored by the current political scenarios in both regions.
Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/seminar
Special Seminar / Virtual Format
Date:
Monday, Aug 5, 2024 / دوشنبه، 15 مرداد 1403
Time:
10:30 AM (Tehran time)
Speaker:
Prof. Galileo Violini
Affiliation:
Co-chair of the Executive Committee of the Great Caribbean Light Source;
Former UNESCO Representative to Islamic Republic of Iran and Director of Tehran Office
Title:
Synchrotron in the Souths - A Science Diplomacy Challenge
Title in Persian:
سنکروترون در جنوب- یک چالش در دیپلماسی علمی
Abstract:
An advanced light source for research would drive growth in the Wider Caribbean region. In addition to analyzing the need for such a facility to meet Latin America's scientific priorities, the challenges to its construction are discussed. These are very similar to those faced by the African Light Source (AfLS): training of users, ensuring sustainable financing, the possibility of international financial support and the role of international organizations. This perspective of South-South cooperation has attracted the attention and support of other similar facilities, such as SESAME and LNLS, which can play an important role in training and, in the case of GCLS, in project design. The development and success of the corresponding actions, aimed at obtaining political support from the governments of the region and international organizations, mainly UNESCO, may be favored by the current political scenarios in both regions.
Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/seminar
Speaker
Mohammadreza Zakeri
Affiliation
University of Kentucky
Title of talk
Does the Sun Have a Dark Disk?
آیا خورشید دارای دیسک تاریک است؟
Date and time
Tuesday, August 3rd, 2024 (Mordad 13th, 1403), 5:00 pm (Tehran zone)
Link
https://www.skyroom.online/ch/schoolofphysics/highenergyseminar
Abstract
The Sun’s oblateness has been measured using optical observations. Its gravitational quadrupole moment has been deduced through helioseismology and measurements of its gravitational effects on Mercury’s orbit. The distribution of mass within Mercury’s orbit would only impact the orbital determination, suggesting that discrepancies among various types of assessments may indicate the possible existence of a non-luminous mass. For the first time, we have developed a method to combine these differing measurements to yield new, highly sensitive constraints on the mass distribution within Mercury’s orbit. In this talk, we will show that the most precise measurements indicate the existence of a non-luminous disk within Mercury’s orbit, with a mass significantly heavier than the modeled mass for the circumsolar dust ring observed by the Solar TErrestrial RElations Observatory (STEREO) mission. This suggests a substantial dark matter contribution. Furthermore, the long-standing inconsistency between the element abundances determined from the spectroscopy of the Sun’s surface, and those inferred from its interior through helioseismology, can be reconciled if the Sun formed within a protoplanetary disk. We will discuss how our findings limit the presence of a dark disk or a spherical halo near the Sun and highlight the potential of future orbital measurements of Mercury and near-Sun asteroids to refine these constraints further.
Mohammadreza Zakeri
Affiliation
University of Kentucky
Title of talk
Does the Sun Have a Dark Disk?
آیا خورشید دارای دیسک تاریک است؟
Date and time
Tuesday, August 3rd, 2024 (Mordad 13th, 1403), 5:00 pm (Tehran zone)
Link
https://www.skyroom.online/ch/schoolofphysics/highenergyseminar
Abstract
The Sun’s oblateness has been measured using optical observations. Its gravitational quadrupole moment has been deduced through helioseismology and measurements of its gravitational effects on Mercury’s orbit. The distribution of mass within Mercury’s orbit would only impact the orbital determination, suggesting that discrepancies among various types of assessments may indicate the possible existence of a non-luminous mass. For the first time, we have developed a method to combine these differing measurements to yield new, highly sensitive constraints on the mass distribution within Mercury’s orbit. In this talk, we will show that the most precise measurements indicate the existence of a non-luminous disk within Mercury’s orbit, with a mass significantly heavier than the modeled mass for the circumsolar dust ring observed by the Solar TErrestrial RElations Observatory (STEREO) mission. This suggests a substantial dark matter contribution. Furthermore, the long-standing inconsistency between the element abundances determined from the spectroscopy of the Sun’s surface, and those inferred from its interior through helioseismology, can be reconciled if the Sun formed within a protoplanetary disk. We will discuss how our findings limit the presence of a dark disk or a spherical halo near the Sun and highlight the potential of future orbital measurements of Mercury and near-Sun asteroids to refine these constraints further.
www.skyroom.online
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Forwarded from انجمن علمی ژرفا
مدل_کیهان_شناسی_دوره_ای_همدیس_راجر_پنروز_به_زبان_ساده.pdf
465.7 KB
🔰 مقاله آموزشی «مدل کیهانشناسی دورهای همدیس راجر پنروز»
🔸 این نوشتار به معرفی مدل کیهانشناسی پنروز میپردازد؛ مدلی که ادعا میکند در آینده بسیار دور، کیهان از ذرات جرمدار خالی میشود، و در نتیجه از منظر همدیسی با ابتدای کیهان همارز است. بنابرین کیهان در آینده، گذشته خود را فراموش و دورههایی طولانی را به صورت متناوب تکرار خواهد کرد. همچنین به مسئله آنتروپی بسیار پایین کیهان اوّلیه و فرضیۀ انحنای ویل نیز پرداخته شده است.
👤 حامد منوچهری کوشا
▫️ برگرفته از کانال علم، فلسفه و الهیات
#مقاله_آموزشی #کیهانشناسی
🆔 @Zharfa90
🔸 این نوشتار به معرفی مدل کیهانشناسی پنروز میپردازد؛ مدلی که ادعا میکند در آینده بسیار دور، کیهان از ذرات جرمدار خالی میشود، و در نتیجه از منظر همدیسی با ابتدای کیهان همارز است. بنابرین کیهان در آینده، گذشته خود را فراموش و دورههایی طولانی را به صورت متناوب تکرار خواهد کرد. همچنین به مسئله آنتروپی بسیار پایین کیهان اوّلیه و فرضیۀ انحنای ویل نیز پرداخته شده است.
👤 حامد منوچهری کوشا
▫️ برگرفته از کانال علم، فلسفه و الهیات
#مقاله_آموزشی #کیهانشناسی
🆔 @Zharfa90
School of Particles and Accelerators
Special Seminar / Virtual Format
Date:
Monday, Aug 5, 2024 / دوشنبه، 15 مرداد 1403
Time:
10:30 AM (Tehran time)
Speaker:
Prof. Galileo Violini
Affiliation:
Co-chair of the Executive Committee of the Great Caribbean Light Source;
Former UNESCO Representative to Islamic Republic of Iran and Director of Tehran Office
Title:
Synchrotron in the Souths - A Science Diplomacy Challenge
Title in Persian:
سنکروترون در جنوب- یک چالش در دیپلماسی علمی
Abstract:
An advanced light source for research would drive growth in the Wider Caribbean region. In addition to analyzing the need for such a facility to meet Latin America's scientific priorities, the challenges to its construction are discussed. These are very similar to those faced by the African Light Source (AfLS): training of users, ensuring sustainable financing, the possibility of international financial support and the role of international organizations. This perspective of South-South cooperation has attracted the attention and support of other similar facilities, such as SESAME and LNLS, which can play an important role in training and, in the case of GCLS, in project design. The development and success of the corresponding actions, aimed at obtaining political support from the governments of the region and international organizations, mainly UNESCO, may be favored by the current political scenarios in both regions.
Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/seminar
Special Seminar / Virtual Format
Date:
Monday, Aug 5, 2024 / دوشنبه، 15 مرداد 1403
Time:
10:30 AM (Tehran time)
Speaker:
Prof. Galileo Violini
Affiliation:
Co-chair of the Executive Committee of the Great Caribbean Light Source;
Former UNESCO Representative to Islamic Republic of Iran and Director of Tehran Office
Title:
Synchrotron in the Souths - A Science Diplomacy Challenge
Title in Persian:
سنکروترون در جنوب- یک چالش در دیپلماسی علمی
Abstract:
An advanced light source for research would drive growth in the Wider Caribbean region. In addition to analyzing the need for such a facility to meet Latin America's scientific priorities, the challenges to its construction are discussed. These are very similar to those faced by the African Light Source (AfLS): training of users, ensuring sustainable financing, the possibility of international financial support and the role of international organizations. This perspective of South-South cooperation has attracted the attention and support of other similar facilities, such as SESAME and LNLS, which can play an important role in training and, in the case of GCLS, in project design. The development and success of the corresponding actions, aimed at obtaining political support from the governments of the region and international organizations, mainly UNESCO, may be favored by the current political scenarios in both regions.
Link to Join Virtually: https://www.skyroom.online/ch/ipm-particles/seminar
🇩🇪 The "International Max Planck Research School for Astronomy and Cosmic Physics at the University of Heidelberg" (IMPRS-HD) invites applications for its PhD program 🇩🇪
The school aims to offer outstanding research and training opportunities with excellent instrumental, observational, and theoretical research facilities at the Max Planck Institute for Astronomy, the Max Planck Institute for Nuclear Physics, the Astronomisches Rechen-Institut, the Landessternwarte Koenigstuhl, the Institute of Theoretical Astrophysics, and the Heidelberg Institute for Theoretical Studies.
Main research topics carried out at these institutions are planet and star formation; exoplanets and substellar objects; astrometry; formation, evolution and dynamics of galaxies and supermassive black holes; gravitational lensing; cosmology and structure formation; high energy astrophysics; and state-of-the-art instrumentation for astronomy and astroparticle physics.
The IMPRS-HD is an independent part of the Heidelberg Graduate School for Physics.
Several fellowships are available with 1600-1800 Euro monthly average net income.
Interested students are invited to apply by November 1, 2024, for the academic year starting in September 2025.
An earlier start of the thesis research is possible.
Applicants must have a Master's degree (or equivalent) in Physics/Astronomy including a corresponding thesis and a very good physics background. Applicants with a 4-yr degree in physics may be accepted conditionally.
Further details on IMPRS-HD and the application process can be found at http://www.imprs-hd.mpg.de/
The school aims to offer outstanding research and training opportunities with excellent instrumental, observational, and theoretical research facilities at the Max Planck Institute for Astronomy, the Max Planck Institute for Nuclear Physics, the Astronomisches Rechen-Institut, the Landessternwarte Koenigstuhl, the Institute of Theoretical Astrophysics, and the Heidelberg Institute for Theoretical Studies.
Main research topics carried out at these institutions are planet and star formation; exoplanets and substellar objects; astrometry; formation, evolution and dynamics of galaxies and supermassive black holes; gravitational lensing; cosmology and structure formation; high energy astrophysics; and state-of-the-art instrumentation for astronomy and astroparticle physics.
The IMPRS-HD is an independent part of the Heidelberg Graduate School for Physics.
Several fellowships are available with 1600-1800 Euro monthly average net income.
Interested students are invited to apply by November 1, 2024, for the academic year starting in September 2025.
An earlier start of the thesis research is possible.
Applicants must have a Master's degree (or equivalent) in Physics/Astronomy including a corresponding thesis and a very good physics background. Applicants with a 4-yr degree in physics may be accepted conditionally.
Further details on IMPRS-HD and the application process can be found at http://www.imprs-hd.mpg.de/
www.imprs-hd.mpg.de
IMPRS HD
Welcome to the Webpage of the International Max Planck Research School for Astronomy and Cosmic Physics at the University of Heidelberg (IMPRS HD)
🇩🇪 PhD in Astronomy / Astrophysics 🇩🇪
Call for applications / fully funded PhD grants for successful applicants
You want to boost your career in Astrophysics? Then do your PhD in one of the largest centers for Astronomy and Astrophysics in Europe and work with the leading scientists in the field to accelerate your scientific career!
The International Max Planck Research School on Astrophysics at the Ludwig Maximilians University Munich (IMPRS on Astrophysics) is soliciting applications for its PhD program. Located in the beautiful Munich-Garching area in southern Bavaria (Germany), the school offers a unique environment for graduate students due to the presence of four internationally renowned institutes which form the school:
The Max Planck Institute for Extraterrestrial Physics (MPE)
The Observatory of the University of Munich (LMU/USM)
The Max Planck Institute for Astrophysics (MPA)
The European Southern Observatory (ESO)
IMPRS offers a highly competitive PhD program, including lectures, seminars and a research project supervised by leading scientists at one of the participating institutions.
Course language is English. Students have access to the world largest ground- and spaced-based observatories and instrumentation operated by the participating institutes as well as to supercomputers for advanced numerical simulations and theoretical studies.
Applications for the PhD-program are open to students from all countries. Successful applicants will get a work contract / fellowship with a monthly income that covers the living costs. We will assist our students with all administrative matters for a smooth on-boarding. This means "Concentrate on your research -- we do the rest!"
For more details see: https://www.imprs-astro.mpg.de/
The closing date for applications for the program starting in September 2025 is November 1, 2024. If for any reason you have difficulty meeting the deadline, please inform us in advance and we will extend it upon request.
Call for applications / fully funded PhD grants for successful applicants
You want to boost your career in Astrophysics? Then do your PhD in one of the largest centers for Astronomy and Astrophysics in Europe and work with the leading scientists in the field to accelerate your scientific career!
The International Max Planck Research School on Astrophysics at the Ludwig Maximilians University Munich (IMPRS on Astrophysics) is soliciting applications for its PhD program. Located in the beautiful Munich-Garching area in southern Bavaria (Germany), the school offers a unique environment for graduate students due to the presence of four internationally renowned institutes which form the school:
The Max Planck Institute for Extraterrestrial Physics (MPE)
The Observatory of the University of Munich (LMU/USM)
The Max Planck Institute for Astrophysics (MPA)
The European Southern Observatory (ESO)
IMPRS offers a highly competitive PhD program, including lectures, seminars and a research project supervised by leading scientists at one of the participating institutions.
Course language is English. Students have access to the world largest ground- and spaced-based observatories and instrumentation operated by the participating institutes as well as to supercomputers for advanced numerical simulations and theoretical studies.
Applications for the PhD-program are open to students from all countries. Successful applicants will get a work contract / fellowship with a monthly income that covers the living costs. We will assist our students with all administrative matters for a smooth on-boarding. This means "Concentrate on your research -- we do the rest!"
For more details see: https://www.imprs-astro.mpg.de/
The closing date for applications for the program starting in September 2025 is November 1, 2024. If for any reason you have difficulty meeting the deadline, please inform us in advance and we will extend it upon request.
Forwarded from انجمن فیزیک ایران
✅ مدال دیراک سال 2024 برای فهم آنتروپی کوانتومی
#اخبار_علمی_و_پژوهشی
مدالِ دیراک سال 2024 به فیزیکدانانی رسید که در فهم آنتروپی کوانتومی در نظریه های گرانش کوانتومی و نظریه های میدان سهم داشته اند. (در تصویر فوق از چپ به راست) هوراسیو کاسینی Horacio Casini و مارینا هویرتا Marina Huerta از شورای علمی، فنی و مرکز اتمی باریلوکه آرژانتین، شینسِی رو Shinsei Ryu از ...
📣 متن کامل را در Instant View ⚡️ (دکمه پایین صفحه) و یا در وبگاه انجمن فیزیک ایران بخوانید:
🚩http://www.psi.ir/news2_fa.asp?id=4101
⏪ وبگاه انجمن فیزیک ایران:
🌍 http://www.psi.ir
✅ به کانال خبرى انجمن فیزیک ايران بپيوندید:
👇👇🏽👇👇🏽👇👇🏽👇
http://t.me/psinews
#اخبار_علمی_و_پژوهشی
مدالِ دیراک سال 2024 به فیزیکدانانی رسید که در فهم آنتروپی کوانتومی در نظریه های گرانش کوانتومی و نظریه های میدان سهم داشته اند. (در تصویر فوق از چپ به راست) هوراسیو کاسینی Horacio Casini و مارینا هویرتا Marina Huerta از شورای علمی، فنی و مرکز اتمی باریلوکه آرژانتین، شینسِی رو Shinsei Ryu از ...
📣 متن کامل را در Instant View ⚡️ (دکمه پایین صفحه) و یا در وبگاه انجمن فیزیک ایران بخوانید:
🚩http://www.psi.ir/news2_fa.asp?id=4101
⏪ وبگاه انجمن فیزیک ایران:
🌍 http://www.psi.ir
✅ به کانال خبرى انجمن فیزیک ايران بپيوندید:
👇👇🏽👇👇🏽👇👇🏽👇
http://t.me/psinews
t.me
مدال دیراک سال 2024 برای فهم آنتروپی کوانتومی
🇦🇺 PhD Scholarships in Observational, Computational & Theoretical Astrophysics 🇦🇺
The Centre for Astrophysics and Supercomputing (CAS) at Swinburne University of Technology in Melbourne invites applications from high-calibre students of any nationality for its PhD program. CAS is one of Australia's largest astronomy research institutes, with about 20 faculty, 20 postdoctoral researchers, and 40 PhD students. Swinburne has guaranteed access to the 10-m Keck telescopes, with our astronomers and students regularly obtaining time at the world's major optical and radio observatories. They also study gravitational wave sources with LIGO, and use OzSTAR, the next generation Australian Supercomputer for theoretical and observational astrophysics.
PhD scholarships include a tax free stipend, of approximately $33,500 AUD p.a., receive a tuition waiver, and have access to funding for travel to telescopes, international conferences, and collaborative meetings. For details about the program see the associated web links.
http://astronomy.swin.edu.au/study/PhDEoI/
The Centre for Astrophysics and Supercomputing (CAS) at Swinburne University of Technology in Melbourne invites applications from high-calibre students of any nationality for its PhD program. CAS is one of Australia's largest astronomy research institutes, with about 20 faculty, 20 postdoctoral researchers, and 40 PhD students. Swinburne has guaranteed access to the 10-m Keck telescopes, with our astronomers and students regularly obtaining time at the world's major optical and radio observatories. They also study gravitational wave sources with LIGO, and use OzSTAR, the next generation Australian Supercomputer for theoretical and observational astrophysics.
PhD scholarships include a tax free stipend, of approximately $33,500 AUD p.a., receive a tuition waiver, and have access to funding for travel to telescopes, international conferences, and collaborative meetings. For details about the program see the associated web links.
http://astronomy.swin.edu.au/study/PhDEoI/
astronomy.swin.edu.au
CAS - Expression of Interests
Centre for Astrophysics and Supercomputing