| Feb. 13, 2024, 4:19 p.m. |
Created
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[{"model": "core.projectfund", "pk": 62536, "fields": {"project": 10731, "organisation": 11097, "amount": 1721563, "start_date": "2017-10-01", "end_date": "2022-09-30", "raw_data": 177441}}]
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| Jan. 30, 2024, 4:24 p.m. |
Created
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[{"model": "core.projectfund", "pk": 55380, "fields": {"project": 10731, "organisation": 11097, "amount": 1721563, "start_date": "2017-10-01", "end_date": "2022-09-30", "raw_data": 153294}}]
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| Jan. 2, 2024, 4:15 p.m. |
Created
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[{"model": "core.projectfund", "pk": 48179, "fields": {"project": 10731, "organisation": 11097, "amount": 1721563, "start_date": "2017-10-01", "end_date": "2022-09-30", "raw_data": 132498}}]
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| Dec. 5, 2023, 4:23 p.m. |
Created
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[{"model": "core.projectfund", "pk": 40932, "fields": {"project": 10731, "organisation": 11097, "amount": 1721563, "start_date": "2017-09-30", "end_date": "2022-09-29", "raw_data": 98777}}]
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| Nov. 27, 2023, 2:14 p.m. |
Added
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{"external_links": []}
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| Nov. 21, 2023, 4:37 p.m. |
Created
43
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[{"model": "core.projectfund", "pk": 33637, "fields": {"project": 10731, "organisation": 11097, "amount": 1721563, "start_date": "2017-09-30", "end_date": "2022-09-29", "raw_data": 57326}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
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[{"model": "core.projectorganisation", "pk": 97459, "fields": {"project": 10731, "organisation": 12574, "role": "LEAD_ORG"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
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[{"model": "core.projectperson", "pk": 61201, "fields": {"project": 10731, "person": 15671, "role": "RESEARCH_COI_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
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[{"model": "core.projectperson", "pk": 61200, "fields": {"project": 10731, "person": 15672, "role": "RESEARCH_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61199, "fields": {"project": 10731, "person": 15673, "role": "RESEARCH_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61198, "fields": {"project": 10731, "person": 15677, "role": "COI_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61197, "fields": {"project": 10731, "person": 15438, "role": "COI_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61196, "fields": {"project": 10731, "person": 15674, "role": "COI_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61195, "fields": {"project": 10731, "person": 15678, "role": "COI_PER"}}]
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| Nov. 21, 2023, 4:37 p.m. |
Created
40
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[{"model": "core.projectperson", "pk": 61194, "fields": {"project": 10731, "person": 15482, "role": "PI_PER"}}]
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| Nov. 20, 2023, 2:04 p.m. |
Updated
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{"title": ["", "Edinburgh Nuclear Physics Group Consolidated Grant Proposal"], "description": ["", "\nThe research programme aims at understanding the processes that forge the elements in stars and the big bang and obtaining a deeper understanding of nuclear matter. This requires remarkable experiments underground that let us study reactions at the very low energies occurring in stars such as the sun, and with beams of radioactive nuclei to understand the reactions that take place in explosive events such as supernovae which occur at higher temperatures and involve unstable isotopes. The astrophysical origin of the elements heavier than iron remains a particular mystery - they may for example be produced in thermally pulsing stars, supernovae and merging neutron stars. Fusion reactions with neutrons play a vital role in producing these elements but we do not understand these reactions, and the properties of radioactive isotopes produced by them, well enough. We will study reactions with neutron beams and study the properties of highly neutron-rich nuclei existing very far from stability. The nature of matter in neutron stars themselves remains a mystery. These are like large nuclei but bound by the gravitational force rather than the strong force. We will perform measurements of the neutron skin which forms on the surface of nuclei with intense high energy photon beams. The neutron skin is a mini laboratory for neutron star matter and by accurately measuring its properties we can access new information on neutron star structure and cooling mechanisms. The nature of matter inside neutron star cores is a great mystery, and it has been suggested that matter containing strange quarks may be present - a remarkable hypothesis. Our experiments will test the nature of nuclear matter for the conditions found in neutron stars. There is evidence that quarks can exist as a group of 6, a hexaquark, and may even be present inside neutron stars and influence their properties. This is not something found in textbooks but the theory of the strong force, quantum chromo dynamics, allows this exotic possibility. We will perform experiments to provide stronger evidence for the existence of the hexaquark and probe its properties.\n\n"], "extra_text": ["", "\n\nPotential Impact:\nThis proposal outlines an exciting research programme to explore the origins of the \nchemical elements, the impact of nuclear physics on the behaviour of exotic environments\nsuch as neutron stars and provide our first detailed understanding of how large groups\nof quarks might behave.\n\nTo achieve these research objectives we will need to use all of our decades of\ncollective expertise and knowledge and then - we will need to take the next step -\nand develop new and better experimental techniques, methods and equipment.\n\nIt is in these new developments that we find opportunities to exploit our research\ntechniques and methods in different ways and widen their impact. \n\nDetector technologies have been developed which could provide significantly improved\nmedical scanners - better quality images faster. This concept has now been patented \nand a proposal is now being prepared to make this innovation commercially available.\n\nMedical research has recently indicated that ultra-fast bursts of gamma rays may be\nmore effective at killing tumour cells than conventional, continuous sources of\ngamma-rays. Detecting ultra-fast bursts of gamma-rays is difficult but we have\nrecently devised a new method to detect such bursts - can we use this\nto enable the development of safe, controllable and effective therapy?\n\nAdvanced nuclear reactor designs provide increased efficiency, reliability and safety.\nBut these designs are critically dependent on a detailed understanding of how neutrons\ninteract with, for example, the materials used to build the reactor. How will these\nmaterials age during reactor operation? Neutrons are also used to target tumours and\nit is important to understand how to control and manage the impact of neutrons on\nhealthy tissue and maximise their effect on cancerous tissue. Our research at facilities\nwhich produce high fluxes of neutrons will help us understand both of these issues.\n\nThe nuclear physics research programme provides excellent training opprtunities\nfor PhD students. The size and scope of nuclear physics experiments means that\nPhD students must actively engage with all of the scientific and technical aspects\nof the experiments from beam transport to the experimental target, to the analysis\nand interpretation of experimental data, and all points in between. The research\nprogramme produces young scientists with a wide range of scientific and technical\ncompetencies with employment opportunities in industry, business and academia.\n\n\n"], "status": ["", "Closed"]}
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| Nov. 20, 2023, 2:04 p.m. |
Added
35
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{"external_links": [44480]}
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| Nov. 20, 2023, 2:04 p.m. |
Created
35
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[{"model": "core.project", "pk": 10731, "fields": {"owner": null, "is_locked": false, "coped_id": "bf768461-20c8-46cf-9b81-9efea08b4c37", "title": "", "description": "", "extra_text": "", "status": "", "start": null, "end": null, "raw_data": 57309, "created": "2023-11-20T13:40:08.676Z", "modified": "2023-11-20T13:40:08.676Z", "external_links": []}}]
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