{ "meta": { "api_type": "NWO Projects API", "version": "1.0.2", "licence": { "name": "CC0 1.0 Universal", "url": "https://creativecommons.org/publicdomain/zero/1.0", "description": "To the extent possible under law, all copyright and related or neighbouring rights have been waived worldwide to the data made available through this API." }, "documentation": "https://doi.org/10.5281/zenodo.14918287", "release_date": "2025-08-20T00:00:00", "funder": "https://doi.org/10.13039/501100003246", "ror_id": "https://ror.org/04jsz6e67", "date": "2026-11-04T00:00:00", "count": 1, "per_page": 100, "pages": 1, "page": 1 }, "projects": [ { "project_id": "OCENW.XL21.XL21.038", "title": "Probing the phase diagram of quantum chromodynamics", "funding_scheme_id": 4273, "funding_scheme": "Open Competitie ENW XL (voorheen OC ENW-GROOT) Ronde 2021", "department": "Exacte en Natuurwetenschappen", "sub_department": "Exacte en Natuurwetenschappen", "start_date": "2022-11-01T00:00:00", "reporting_year": 2022, "summary_nl": "Quantum chromodynamics (QCD), the theory of the strong nuclear interaction that holds together atomic nuclei and is ultimately responsible for all the matter around us, remains the least understood ingredient of the Standard Model of particle physics. Particularly the way matter behaves under extreme conditions of temperature, pressure, and magnetic fields has proved to be elusive. At ultra-high temperatures, a quark-gluon plasma is formed, a state of matter that existed in the early universe and which can be recreated at the Large Hadron Collider through collisions of heavy ions; however, its basic properties are not understood. At the opposite extreme there are neutron stars, in which temperature is low but the density of matter so high that any further increase would lead to a black hole. The mysterious structure of neutron stars is now being accessed by LIGO and Virgo, through gravitational wave observations of binary neutron star collisions. The “kilonova”, the electromagnetically powered transient of such cataclysmic events, is yielding insight into the formation of heavy elements in the universe, while observations of the accompanying gamma ray bursts have also provided information on the behaviour of dense matter, along with accurate X-ray measurements of neutron star masses and radii with NICER. However, until now the regimes of astrophysical observations and those of particle collider experiments have been studied in virtual isolation. This proposal brings together gravitational wave scientists, astronomers and astrophysicists, nuclear and collider physicists, and theoreticians that are in close geographical proximity, in an effort to jointly bridge the gap and provide a unified theoretical and observational framework – based on relativistic magneto-hydrodynamics - for understanding the behaviour of nuclear matter under the most extreme conditions. This will enable a full exploration of the rich physics that occurs across the “QCD phase diagram”.", "summary_en": "Quantum chromodynamics (QCD), the theory of the strong nuclear interaction that holds together atomic nuclei and is ultimately responsible for all the matter around us, remains the least understood ingredient of the Standard Model of particle physics. Particularly the way matter behaves under extreme conditions of temperature, pressure, and magnetic fields has proved to be elusive. At ultra-high temperatures, a quark-gluon plasma is formed, a state of matter that existed in the early universe and which can be recreated at the Large Hadron Collider through collisions of heavy ions; however, its basic properties are not understood. At the opposite extreme there are neutron stars, in which temperature is low but the density of matter so high that any further increase would lead to a black hole. The mysterious structure of neutron stars is now being accessed by LIGO and Virgo, through gravitational wave observations of binary neutron star collisions. The “kilonova”, the electromagnetically powered transient of such cataclysmic events, is yielding insight into the formation of heavy elements in the universe, while observations of the accompanying gamma ray bursts have also provided information on the behaviour of dense matter, along with accurate X-ray measurements of neutron star masses and radii with NICER. However, until now the regimes of astrophysical observations and those of particle collider experiments have been studied in virtual isolation. This proposal brings together gravitational wave scientists, astronomers and astrophysicists, nuclear and collider physicists, and theoreticians that are in close geographical proximity, in an effort to jointly bridge the gap and provide a unified theoretical and observational framework – based on relativistic magneto-hydrodynamics - for understanding the behaviour of nuclear matter under the most extreme conditions. This will enable a full exploration of the rich physics that occurs across the “QCD phase diagram”.", "award_amount": 3103383, "grant_id": "https://doi.org/10.61686/RMOHL62194", "project_members": [ { "role": "Researcher", "member_id": 515448, "last_name": "Bosch Gomez", "degree_pre_nominal": "dr.", "initials": "P.", "first_name": "Pablo", "organisation": "Universiteit van Amsterdam||Faculteit der Natuurwetenschappen, Wiskunde en Informatica (Faculty of Science)||Anton Pannekoek Instituut voor Sterrenkunde", "organisation_id": 77831, "ror": "https://ror.org/04dkp9463", "active": false }, { "role": "Researcher", "member_id": 547907, "last_name": "Bosch Gomez", "degree_pre_nominal": "dr.", "initials": "P.", "first_name": "Pablo", "organisation": "Universiteit Utrecht||Faculteit Bètawetenschappen||Centrum voor Didactiek van Wiskunde & Natuurwetenschappen", "organisation_id": 78065, "ror": "https://ror.org/04pp8hn57", "active": false }, { "role": "Researcher", "member_id": 531311, 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