{"id":544,"date":"2021-06-04T03:30:04","date_gmt":"2021-06-04T03:30:04","guid":{"rendered":"http:\/\/localhost:10023\/?page_id=544"},"modified":"2021-06-04T03:30:04","modified_gmt":"2021-06-04T03:30:04","slug":"construyendo-una-imagen-de-tiempo-de-los-primeros-diez-yoctosegundos-tras-la-colision-de-particulas-elementales","status":"publish","type":"page","link":"https:\/\/igfae.usc.es\/yoctolhc\/construyendo-una-imagen-de-tiempo-de-los-primeros-diez-yoctosegundos-tras-la-colision-de-particulas-elementales\/","title":{"rendered":"CONSTRUYENDO UNA IMAGEN DE TIEMPO DE LOS PRIMEROS DIEZ YOCTOSEGUNDOS TRAS LA COLISI\u00d3N DE PART\u00cdCULAS ELEMENTALES"},"content":{"rendered":"\n

La luz tarda tres yoctosegundos en cruzar un prot\u00f3n. Para tener una idea de lo peque\u00f1o que es este tiempo, podemos pensar que si la edad del Universo fuera solo un segundo, este tiempo a\u00fan ser\u00eda un mill\u00f3n de veces m\u00e1s corto que un abrir y cerrar de ojos. Este peque\u00f1o tiempo aparentemente es suficiente para que, en colisiones de iones pesados en el Gran Colisionador de Hadrones (LHC) del CERN<\/a>, los quarks y gluones pierdan coherencia cu\u00e1ntica, interact\u00faen entre s\u00ed y formen el plasma de quarks y gluones que impregn\u00f3 todo el Universo microsegundos despu\u00e9s del Big Bang.<\/p>\n\n\n\n

El proyecto “Yoctosecond imaging of QCD collectivity using jet observables (YoctoLHC)” propone un uso novedoso de sondas espec\u00edficas, chorros de part\u00edculas de alta energ\u00eda, para construir una imagen temporal de los primeros 10 yoctosegundos de la colisi\u00f3n y desentra\u00f1ar el proceso de emergencia de complejidad de los componentes b\u00e1sicos de la naturaleza.<\/p>\n\n\n\n

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The project was awarded in April 2019 a 2.5 million euro Advanced Grant for a 5-year period by the European Research Council (ERC<\/a>).<\/p>\n\n\n\n

YoctoLHC is led by Carlos Salgado, professor of Theoretical Physics at the University of Santiago de Compostela <\/a>and director of the Galician Institute of High Energy Physics<\/a> (IGFAE)<\/a>, and it is carried out by an international team with researchers from the Laboratory of Instrumentation and Experimental Particle Physics (LIP)<\/a> and the University of Jyv\u00e4skyl\u00e4<\/a> in Finland.Carlos Salgado was previously awarded with another European Research Council Starting Grant \/ Consolidator as principal investigator in 2011, Hot and dense QCD in the LHC era (HotLHC), hosted at the Universidade de Santiago de Compostela and CERN. The project run from January 2012 to December 2017 and it can be visited here<\/a>.<\/p>\n\n\n\n

<\/div>\n\n\n\n

OBJECTIVE<\/strong><\/h1>\n\n\n\n

QCD is the only sector of the Standard Model where the exploration of the first levels of complexity, built from fundamental interactions at the quantum level, is experimentally feasible. An outstanding example is the thermalised state of QCD matter formed when heavy atomic nuclei are smashed in particle colliders. Systematic experimental studies, carried out in the last two decades, overwhelmingly support the picture of a deconfined state of matter, which behaves as a nearly perfect fluid, formed in a very short time, less than 5 yoctoseconds. The mechanism that so efficiently brings the initial out-of-equilibrium state into a thermalised system is, however, largely unknown. <\/p>\n\n\n\n

Most surprisingly, LHC experiments have found that collisions of small systems, i.e. proton-proton or proton-lead, seem to indicate the presence of a tiny drop of this fluid in events with a large number of produced particles. These systems have sizes of 1 fm or less, or time-scales of less than 3 ys. To add to the puzzle, jet quenching, the modifications of jet properties due to interactions with the medium, has not been observed in these small systems, while jet quenching and thermalisation are expected to be controlled by the same dynamics. <\/p>\n\n\n\n

Present experimental tools have limited sensitivity to the actual process of thermalisation. To solve these long-standing questions we propose, as a completely novel strategy, using jet observables to directly access the first yoctoseconds of the collision.<\/p>\n\n\n\n

<\/div>\n\n\n\n

SUBJECTS<\/h1>\n\n\n\n

This strategy needs developments well beyond the state-of-the-art in three subjects: <\/p>\n\n\n\n

  1. novel theoretical descriptions of the initial stages of the collision \u2014 the first 5 ys; <\/li>
  2. jet quenching theory for yoctosecond precision, with new techniques to couple the jet to the surrounding matter and novel parton shower evolution; and<\/li>
  3. jet quenching tools for the 2020\u2019s, where completely novel jet observables will be devised with a focus on determining the initial stages of the collision.<\/li><\/ol>\n\n\n\n
    <\/div>\n\n\n\n

    PARTNERSHIPS<\/h1>\n\n\n\n

    IGFAE<\/strong><\/h3>\n\n\n\n
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    The Galician Institute for High Energy Physics (IGFAE) at the Universidade de Santiago de Compostela (USC) is a research institute accredited as Mar\u00eda de Maeztu Unit of Excellence by the Spanish Ministry of Science. It hosts around 100 researchers, including more than 20 postdocs, 40 PhD students and two ERC grantees.<\/p>\n\n\n\n

    Puedes conocer el equipo que conforma este proyecto (aqu\u00ed) y nuestras vacantes abiertas en la investigaci\u00f3n (aqu\u00ed). <\/p>\n\n\n\n

    LIP<\/h3>\n\n\n\n
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    UNIVERSITY OF JVYASKYLA <\/h3>\n\n\n\n
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    LANGUAGES<\/strong><\/h2>\n\n\n\n