伦敦大学学院PhD position in Event horizon-scale modelling of radiation from black holes申请条件要求-申请方
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伦敦大学学院
PhD直招介绍
About the Project
In 2019 the Event Horizon Telescope (EHT) Collaboration published the first image of a supermassive black hole (SMBH) from the galaxy M87. In 2022 the EHT then published an image of the SMBH in the heart of our galaxy. These images revealed a bright emission ring enclosing the ‘event horizon’ of the SMBH. Accurate measurements of these images provide new constraints on BH mass and spin, the mechanisms powering accretion and relativistic jet collimation, and even enable novel tests of general relativity. Multi-frequency polarimetric observations from black-hole systems are essential to understand their fundamental properties and governing physical processes. Modelling the electromagnetic (EM) emissions from BHs requires performing magnetohydrodynamics (MHD) simulations of relativistic plasmas in strong gravity for later post-processing using polarised radiative transfer.
The student will begin by learning to perform MHD simulations of BH accretion, calculating the multi-frequency EM emissions from the vicinity of the event horizon using radiative transfer. The student will then choose to continue with one of the following research directions: (1) flaring events in the Galactic Centre, (2) particle production and acceleration processes around BHs, or (3) strong-field tests of gravity. These directions all provide new observable signatures which will help guide future astronomical observations of strong gravity systems. Throughout the project the student will learn experimental techniques underpinning interferometric imaging of BHs and their research outcomes will contribute to science working groups within the EHT Collaboration.
Additional information
This project is based in the Department of Space & Climate Physics, located at the Mullard Space Science Laboratory (MSSL) in Holmbury, Surrey. MSSL is located in remote countryside in Surrey. There is limited public transport to reach the site. Before you apply to study for a PhD in our department, please check our location carefully and consider how you will regularly commute to MSSL.
Additional eligibility requirements( https://www.findaphd.com/common/clickCount.aspx?theid=177016&type=184&DID=4060&url=https%3a%2f%2fwww.ukri.org%2fwhat-we-offer%2fdeveloping-people-and-skills%2fstfc%2ftraining%2fstudentship-information-for-students%2f )
伦敦大学学院 PhD position in Event horizon-scale modelling of radiation from black holes项目有没有奖学金，是不是全奖Phd招生，下面我们一起看一下【大学名称】Phd的奖学金资助情况
项目资助情况
The STFC studentship will pay your full tuition fees and a maintenance allowance for 3.5 years (subject to the PhD upgrade review)
伦敦大学学院Phd申请条件和要求都有哪些？PhD position in Event horizon-scale modelling of radiation from black holes项目是不是全奖？有没有奖学金？下面我们一起看一下伦敦大学学院申请Phd直招需要具备哪些条件和要求，以及托福、雅思语言成绩要到多少才能申请。
申请要求
Desired Knowledge and Skills
Required: Undergraduate or MSc in physics or astrophysics
Required: firm foundation in general relativity, radiative transfer, and magnetohydrodynamics
Required: strong background (and demonstrable prior experience) in analytic and numerical computational approaches
Required: creativity and determination
Desirable: knowledge in astronomy and interferometric imaging
Desirable: running computational codes on shared and distributed memory architectures (OpenMP and MPI)
Entry requirements
An upper second-class Bachelor’s degree, or a second-class Bachelor’s degree together with a Master's degree from a UK university in a relevant subject, or an equivalent overseas qualification.
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