{"id":2337,"date":"2020-11-17T19:55:39","date_gmt":"2020-11-17T18:55:39","guid":{"rendered":"https:\/\/us.edu.pl\/instytut\/ifiz\/?page_id=2337"},"modified":"2024-05-28T17:31:16","modified_gmt":"2024-05-28T15:31:16","slug":"badanie-produkcji-powabu-w-zderzeniach-ciezkich-jonow","status":"publish","type":"page","link":"https:\/\/us.edu.pl\/instytut\/ifiz\/badanie-produkcji-powabu-w-zderzeniach-ciezkich-jonow\/","title":{"rendered":"Badanie produkcji powabu w zderzeniach ci\u0119\u017ckich jon\u00f3w"},"content":{"rendered":"<p>[vc_row][vc_column][vc_single_image image=&#8221;2725&#8243; img_size=&#8221;medium&#8221; alignment=&#8221;center&#8221;]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        <h3 class=\"page-title text__title\">Charm in heavy ion collision<\/h3>\r\n                        <div class=\"text-modules__content\"><p>The project received funding under the GRIEG competition.<\/p>\n<p>GRIEG is one of the three calls funded from the Norway and EEA Grants 2014\u20132021 under the Basic Research Programme operated by the National Science Centre. The objective of the programme is to enhance research-based knowledge development, strengthen the Polish-Norwegian research cooperation, improve the quality of publications<\/p>\n<h2><strong>The objectives of the project<\/strong><\/h2>\n<ul>\n<li>measure charm hadron production (mainly D mesons) in central Pb+Pb<br \/>\ncollisions<\/li>\n<li>understand the charm production phenomenology<\/li>\n<li>upgrade NA61\/SHINE detector, upgrade of the readout electronics of the Time Projection Chambers part of the NA61\/SHINE detector upgrade during the CERN accelerator Long Shutdown 2 period (2020 and 2021)<\/li>\n<\/ul>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><p><strong>Charm in heavy-ion collision<\/strong><\/p>\n<p>The charm here means property of strongly interacting elementary particles, hadrons, build-out of their sub-elementary fundamental components \u2013 quarks and gluons. These components, with a generic name partons, carry specific charges called colors \u2013 red, green, and blue. Colors are sources of strong interactions binding partons into hadrons, hadrons into nucleons, nucleons into nuclei. The theory describing strong interaction is called Quantum Chromodynamics (QCD). Hadrons are constructed out of partons in such a way that they do not carry any color &#8211; so they are called colorless. In other words &#8211; the colors of partons are not inherited by hadrons. Colors are not observable. These are different from other charges carried by partons, e.g. electric charge, isotopic spin, and flavors. The flavor here means strangeness possessed by the quark <em>s<\/em>, charm possessed by the quark <em>c<\/em>, true (called also top) by the quark <em>t, <\/em>and beauty (called also bottom) by the quark <em>b<\/em>. Quarks <em>s,c,t,b<\/em>, ordered by the masses, \u00a0are preceded by the lightest quarks <em>u<\/em> (up) and <em>d<\/em> (down) having the same mass, but different components of the isotopic spin\u00a0 \u00b1\u00bd. Gluons are just massless, appearing in eight coloring combinations. Any quark <em>q<\/em> has its antiquark \u00a0\u2013 the same mass, all charges opposite.\u00a0 All hadrons can be systematized as they are build out of pair quark-antiquark<em> q<\/em><em>\u00a0<\/em>(mesons) or three quarks <em>qqq<\/em> (baryons) \u2013 with quarks glued by gluons.<\/p>\n<p>Almost all hadrons of the Universe are build out of light quarks <em>u<\/em> and <em>d<\/em>. Higher flavors <em>s,c,t,b<\/em> are formed only under special conditions when \u201cnormal\u201d hadrons collide at high energy. Then the excitation energy is transformed into the production of new particles, and if high enough, into the production of heavy flavor hadrons \u2013 i.e. composed also out of heavy flavor quarks. Such conditions appear \u2013 when Big Bang ignited the Universe, in the cores of stars, and when a beam of particles accelerated in the accelerator hits the target (fixed target experiment) or collides with the opposite beam coming out of the accelerator (collider experiment). Such experiments give the unique possibility to research in a controlled way process and forces on the most fundamental partonic level, to imitate conditions inside star\u2019s core, not excluding some Big Bang conditions.<\/p>\n<p>Particularly interesting situations appear when colliding objects are not single hadrons but nuclei. There is a theoretical possibility, based on QCD suggestions, that within such collision a new form of matter would appear, a kind of hot and dense partonic soup \u2013 called Quark-Gluon Plasma (QGP). Hot means here a temperature of the order \u00a0K\u00b0, dense means 3-15 times normal nuclear matter density. Similar QGP existed during the first milliseconds of Bing Bang, can appear also at the supernova explosions. The main physical problem here, beyond all technological challenges, is to recognize signatures of the QGP appearance. The QGP, composed of deconfined quarks and gluons cools down within <em>s<\/em>, partons pass into confined phase and freshly created hadrons find their way into detectors system. Now, one should decipher out of this experimental data if some signatures of QGP appeared.<\/p>\n<p>NA61\/SHINE, CERN SPS (Super Synchrotron) experiment is a fixed target heavy ion collision experiment. Different sizes of nuclei, from Be+Be till Pb+Pb, are colliding at different energies. The main goal of this project is to upgrade the main detector parts \u2013 the Time Projection Chambers to make possible detection of open charm mesons made of charm\/no-charm pair. There is a well-established hypothesis, that the dumping in the\u00a0 J\/\u03c8 production as compared to the direct charm production is attributed to the QGP medium. \u00a0Unambiguous evidence of the QGP state is still missing, however. The rich and precise results from RHIC and LHC heavy-ion programs did not change the conclusion.<\/p>\n<p>This charm program requires a tenfold increase in the data taking rate. The NA61\/SHINE charm program is a natural extension of the previous studies of the phase transition to the quark-gluon plasma. It addresses the question of the validity and the limits of statistical and dynamical models of high energy collisions in the new domain of quark mass. The objective of charm hadron production measurements in Pb+Pb collisions is to obtain the \ufb01rst data on the mean number of pairs produced in the full phase space in heavy-ion collisions. Moreover, \ufb01rst results on the collision energy and system size dependence will be provided. This, in particular, should signi\ufb01cantly help to answer the questions:<\/p>\n<ul>\n<li>What is the mechanism of open charm production?<\/li>\n<li>How does the onset of decon\ufb01nement impact open charm production?<\/li>\n<li>How does the formation of a quark-gluon plasma impact J\/\u03c8 production?<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>[\/vc_column][\/vc_row][vc_row][vc_column]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><\/p>\n<h3>Participating entities:<\/h3>\n<ol>\n<li class=\"ui-panelgrid-cell ui-grid-col-4\"><span id=\"entityListForm:j_idt394_data_table:0:institutionNameEn\">University of Silesia in Katowice<\/span><\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\"><span id=\"entityListForm:j_idt394_data_table:1:institutionNameEn\">University of Oslo<\/span><\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\"><span id=\"entityListForm:j_idt394_data_table:1:institutionNameEn\"><\/span>Warsaw University of Technology<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">University of Bergen, Department of Physics and Technology<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">Western Norway University of Applied Sciences<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">Jagiellonian University in Cracow<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">Jan Kochanowski University in Kielce<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">University of Wroc\u0142aw<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">University of Warsaw<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">National Centre for Nuclear Research<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">The Henryk Niewodnicza\u0144ski Institute of Nuclear Physics Polish Academy of Sciences<\/div>\n<\/li>\n<li>\n<div class=\"ui-panelgrid-cell ui-grid-col-4\">AGH University of Science and Technology<\/div>\n<\/li>\n<\/ol>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>[\/vc_column][\/vc_row][vc_row][vc_column][vc_single_image image=&#8221;2726&#8243; img_size=&#8221;large&#8221; alignment=&#8221;center&#8221;][\/vc_column][\/vc_row][vc_row][vc_column]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><\/p>\n<h3>Project initiation meeting (kick-off meeting)<\/h3>\n<p><a href=\"https:\/\/indico.cern.ch\/event\/892056\/\">Web page<\/a><\/p>\n<p>Slides from meeting<\/p>\n<ul>\n<li><a class=\"mtli_attachment mtli_pdf mtli_attachment mtli_pdf mtli_attachment mtli_pdf\" href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/IArsene_NA61CollabMeeting_2020Sep23-3.pdf\" data-mtli=\"mtli_filesize3,43MB\" data-mtli=\"mtli_filesize3,43MB\" rel=\"mtli_filesize3,43MB\">Phenomenology of open charm production in heavy-ion collisions<\/a>, \u00a0<span class=\"\">Ionut Arsene Arsene<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Oslo)<\/span><\/span><\/span><\/li>\n<li><a class=\"mtli_attachment mtli_pdf mtli_attachment mtli_pdf mtli_attachment mtli_pdf\" href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/cmos_23Sept2020..pdf\" data-mtli=\"mtli_filesize2,00MB\" data-mtli=\"mtli_filesize2,00MB\" rel=\"mtli_filesize2,00MB\">Open charm measurements in NA61\/SHINE<\/a>\u00a0Pawel Piotr Staszel<span class=\"affiliation\">\u00a0<span class=\"text\">(Jagiellonian University)<\/span><\/span><\/li>\n<li><a class=\"mtli_attachment mtli_pdf mtli_attachment mtli_pdf mtli_attachment mtli_pdf\" href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/upgrade_PS.pdf\" data-mtli=\"mtli_filesize12,37MB\" data-mtli=\"mtli_filesize12,37MB\" rel=\"mtli_filesize12,37MB\">Overview of NA61\/SHINE detector upgrade<\/a>, \u00a0<span class=\"\">Piotr Podlaski<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Warsaw)<\/span><\/span><\/span><\/li>\n<li><a class=\"mtli_attachment mtli_pdf mtli_attachment mtli_pdf mtli_attachment mtli_pdf\" href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/Nieprzypisane\/GRIEG_call_for_Polish-Norwegian_research_projects.pdf\" data-mtli=\"mtli_filesize347,45kB\" data-mtli=\"mtli_filesize347,45kB\" rel=\"mtli_filesize347,45kB\">Grieg grant for funding of the NA61\/SHINE detector upgrade<\/a>, Seweryn Kowalski<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Silesia)<\/span><\/span><\/li>\n<\/ul>\n<h2><\/h2>\n<ul>\n<li>\n<h2><strong>Project main tasks and activities in 2020 and 2021:<\/strong><\/h2>\n<\/li>\n<\/ul>\n<h3>Upgrade of the Time Projections Chambers<\/h3>\n<p>The significant modification of the NA61\/SHINE spectrometer was planned for 2019 &#8211; 2022. The upgrade was motivated by the charm program, which requires a tenfold increase of the data taking the rate to about 1 kHz &#8211; the main topic connected with this upgrade and covered by this project is the upgrade of the TPCs chambers. The following tasks cover this topic:<\/p>\n<ul>\n<li>Development of a 3D model of detectors with electronics, cooling system, and mechanical support elements<\/li>\n<li>Design, manufacturing, and mounting of the mechanical support of electronics and cooling elements<\/li>\n<li>Design and mounting of the low-voltage system<\/li>\n<li>Design, construction, and maintenance of the readout chain<\/li>\n<li>Maintenance and further development of the detector control system<\/li>\n<li>Maintenance and upgrade of the gas system<\/li>\n<\/ul>\n<h3>Test of the detector<\/h3>\n<p>Before the test on the beam, the FEC was tested to check each readout element for noise and connectivity.<br \/>\nThe connectivity to the readout chambers was tested using the calibration pulser system. The LV system (Wiener PS) in its final setup was used for the tests described above. Moreover, the comparison of the noise level to the one measured previously by ALICE (where this electronics operated). The noise level is generally higher than in ALICE because the protection circuitry and the trace length on the adapter circuit boards introduce additional noise.<\/p>\n<p>The TPC was tested on the beam in the fall of 2021 with the magnetic field switched on, and the first tracks were observed. Analyzing the data collected during the test allows for tuning the detector parameters.<\/p>\n<h3>Software<\/h3>\n<p>The new Trigger and Data AcQuisition system (TDAQ) were prepared. All crucial components of the data flow software have been developed and tested. We are now in the stage of configuration fine-tuning. In addition, new features are being added, such as a web-based user interface and additional monitoring. From the point of view of the calibration and analysis software, the implementation of new software for calibration of the energy loss (dE\/dx) in the TPC&#8217;s where done. A preliminary validation on p+Pb data at 158 GeV\/c was performed, and an automation system was built to facilitate the unsupervised running of the multiple calibration steps.<br \/>\nAdditionally, a detailed inspection of gain variations over the TPCs has been performed by means of pad gain maps per TPC sector, obtained from charge spectra per pad resulting from injection and subsequent decay of the 83Kr isotope in the chambers. The upgraded TPC electronics deliver data in a new raw data format, and corresponding decoding and parsing software infrastructure must be available in the SHINE Offline Framework. During the TPC electronics testing, a detector raw data parser was written and used for the quality assessment of TPC raw data. This parser will be moved into the Offline Framework I\/O libraries. A second parser was written to translate raw TPC front-end electronics channels to physical TPC pad objects, a crucial step toward data reconstruction.<br \/>\nThe work connected with Monte Carlo simulations was mostly devoted to implementing the new version of the GEANT 4.0, a toolkit for the simulation of the passage of particles through matter, and implementing the Kalman Filter-based tracking algorithm.<\/p>\n<p>The most critical achievement regarding the maintenance of IT resources was the transition from Jenkins to GitLab CI. This provided versioning of the CI setup, the tested software, automatic checks of all branches, and the division of pipelines into stages. Four software releases were delivered, supporting the development of the new reconstruction software, improvements in the Monte Carlo, and providing multiple bug fixes and optimizations.<\/p>\n<h3>Charm physics<\/h3>\n<p>The main activities were mainly connected with analyzing the pilot data collected before the upgrade of the TPCs. Moreover, analysis to obtain the yield of the open charm production, the pilot data with different statistical and string models, and previous measurements (the NA60\/NA50 experiment) were performed. The work is still in progress.<\/p>\n<ul style=\"list-style-type: circle\">\n<li>\n<h2><strong>Project main tasks and activities in 2023:<\/strong><\/h2>\n<\/li>\n<\/ul>\n<h3>Upgrade of the Time Projections Chambers<\/h3>\n<p>The LS2 detector upgrade was completed. The new and upgraded detectors were commissioned using hadron beams in spring 2022. The commissioning with 150A GeV\/c Pb beam and the first data taking on open charm production in Pb+Pb collisions was done in \u00a0November 2022.<\/p>\n<p>The physics run proved that the primary goal of the upgrade was achieved. The maximum data-taking rate reached 1.6 kHz, much higher than the assumed 1 kHz. The upgrade of the TPC electronics has influenced the quality of collected data, as shown in the figure below:<\/p>\n<p><img class=\"aligncenter\" src=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/Bez-kategorii\/Picture1-1.png\" \/><\/p>\n<p>The considerable effort the participants invested in the detector upgrade opens new options for physics measurements and ensures the operation of the experiment for the next few years.<\/p>\n<h3>Software<\/h3>\n<p>The reconstruction and calibration software is continuously maintained and developed. Significant effort was dedicated to developing the software for the upgraded detector. This has allowed efficient online and offline monitoring during the physics data taking in 2022, as well as the Kr calibration of the upgraded Time Projection Chambers.<\/p>\n<h3>Charm physics<\/h3>\n<p>In 2023, the Pb beam at a momentum of 150A GeV\/c was delivered to the NA61\/SHINE experiment on the 16th of November. After one week of setup, the production data taking started with a 3 mm lead target, providing 6% interaction probability. The data were taken with the unbiased interaction T2 trigger (identified interaction) and beam T1 trigger (identified beam) scaled down by a factor of 100. The total number of interaction trigger events collected during one week of the production data-taking period amounts to 50 million. This includes about 30 million Pb+Pb collisions. It was the first NA61\/SHINE measurement with a lead ion beam performed after the hardware upgrade during the Long Shutdown 2<\/p>\n<h3>Project meeting (in medium meeting)<\/h3>\n<p><a href=\"https:\/\/indico.cern.ch\/event\/1241273\/\">Web page\u00a0<\/a><\/p>\n<p>\n<style type=\"text\/css\">a[data-mtli~=\"mtli_filesize3,43MB\"]:after {content:\" (3,43 MB)\"}a[data-mtli~=\"mtli_filesize2,00MB\"]:after {content:\" (2,00 MB)\"}a[data-mtli~=\"mtli_filesize12,37MB\"]:after {content:\" (12,37 MB)\"}a[data-mtli~=\"mtli_filesize347,45kB\"]:after {content:\" (347,45 kB)\"}<\/style><\/div>\r\n                    <\/div>\r\n                <\/div>[\/vc_column][\/vc_row]<\/p>\n<p>&nbsp;<\/p>\n<hr \/>\n<p>[vc_row][vc_column][vc_single_image image=&#8221;2636&#8243; alignment=&#8221;center&#8221;]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        <h3 class=\"page-title text__title\">Badanie produkcji powabu w zderzeniach ci\u0119\u017ckich jon\u00f3w<\/h3>\r\n                        <div class=\"text-modules__content\"><\/div>\r\n                    <\/div>\r\n                <\/div><div class=\"container\"><div class=\"separator\" style=\"background-color: #EBEBEB\"><\/div><\/div>\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><p>Projekt otrzyma\u0142 finasowanie w ramach konkursu GRIEG.<\/p>\n<p>GRIEG\u00a0to jeden z trzech konkurs\u00f3w finansowanych z funduszy norweskich i funduszy EOG na lata 2014\u20132021 w ramach programu \u201eBadania\u201d.<\/p>\n<p>Celem programu jest rozw\u00f3j wiedzy opartej na badaniach, wzmacnianie polsko-norweskiej wsp\u00f3\u0142pracy badawczej, podnoszenie jako\u015bci publikacji, szczeg\u00f3lnie w naukach humanistycznych, wspieranie rozwoju m\u0142odych naukowc\u00f3w oraz budowanie pozytywnego odbioru bada\u0144 naukowych w spo\u0142ecze\u0144stwie<\/p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><\/p>\n<h4><strong>Cele Projektu:<\/strong><\/h4>\n<ul>\n<li>pomiar\u00a0 produkcji hadron\u00f3w powabnych (g\u0142\u00f3wnie mezon\u00f3w D) w centralnych zderzeniach\u00a0 Pb + Pb<\/li>\n<li>fenomenologia wytwarzania powabu<\/li>\n<li>aktualizacja detektora NA61 \/ SHINE modernizacja elektroniki odczytowej kom\u00f3r projekcji czasowej<\/li>\n<\/ul>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div><div class=\"container\"><div class=\"separator\" style=\"background-color: #EBEBEB\"><\/div><\/div>\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><p><strong>Opis projektu<\/strong><\/p>\n<p>U\u017cyty w tytule powab oznacza jedn\u0105 z cech hadron\u00f3w &#8211; silnie oddzia\u0142uj\u0105cych cz\u0105stek elementarnych. Hadrony s\u0105 zbudowane z parton\u00f3w &#8211; kwark\u00f3w i gluon\u00f3w, b\u0119d\u0105cych swoistymi cz\u0105stkami suplementarnymi. Partony posiadaj\u0105 specyficzny dla siebie \u0142adunek, zwany kolorem, umownie przybieraj\u0105cy podstawowe warto\u015bci: czerwone, zielone i niebieskie. To w\u0142a\u015bnie \u00a0kolor odpowiada za silne oddzia\u0142ywania sk\u0142adaj\u0105ce partony w nukleony &#8211; protony i neutrony &#8211; a te z kolei &#8211; w j\u0105dra atomowe. Teori\u0105 silnych oddzia\u0142ywa\u0144\u00ab jest Chromodynamika Kwantowa (QCD). Hadrony s\u0105 zbudowane z parton\u00f3w tak, \u017ce same s\u0105 bezkolorowe. Kolory parton\u00f3w nie s\u0105 wi\u0119c dziedziczone przez hadrony. Inaczej jest z innymi \u0142adunkami parton\u00f3w &#8211; \u0142adunkiem elektrycznym, izospinem i smakiem. \u0141adunki smak\u00f3w to dziwno\u015b\u0107 posiadana przez kwark s, powab posiadany przez kwark c, prawda przenoszona przez kwark t i pi\u0119kno przenoszone przez kwark b. Kwarki s; c; t; b, uporz\u0105dkowane tu wed\u0142ug swych rosn\u0105cych mas, s\u0105 w tej hierarchii poprzedzane przez najl\u017cejsze kwarki u i d maj\u0105ce jednakowe masy, ale r\u00f3\u017cni\u0105ce si\u0119 trzeci\u00a1 sk\u0142adow\u0105 izospinu. Gluony s\u0105 bez masowe i wyst\u0119puj\u0105\u00a1 w o\u015bmiu stanach wielokolorowych. Ka\u017cdy kwark q ma swego antykwarka \u00a0q \u00a0o tej samej masie, ale z przeciwnymi \u0142adunkami. Wszystkie hadrony mog\u0105 by\u00a2 rozmieszczone w strukturach zbudowanych z par kwark-antykwark qq (mezony) lub trzech kwark\u00f3w qqq (bariony) &#8211; z kwarkami sklejanymi przez gluony. Prawie wszystkie hadrony Wszech\u015bwiata to kwarki u i d. Ci\u0119\u017csze smaki s; c; t; b pojawiaj\u00a1 si\u0119<\/p>\n<p>w szczeg\u00f3lnych warunkach, gdy &#8222;zwykle&#8221; hadrony zderzaj\u0105 si\u0119 ze sob\u0105 nader energicznie. Energia wzbudzenia objawia si\u0119 \u00a0produkcj\u0105\u00a1 nowych cz\u0105stek, a jej zwi\u0119kszanie generuje hadrony wy\u017cszych smak\u00f3w, zbudowanych z kwark\u00f3w ci\u0119\u017cszych od najl\u017cejszych u i d. Podobnie by\u0142o gdy Wielki Wybuch inicjowa\u0142 Wszech\u015bwiat, podobnie jest we wn\u0119trzu gwiazd i wtedy gdy strumie\u0144 cz\u0105stek z akceleratora zderza si\u0119 z tarcz\u0105 (eksperyment z nieruchom\u00a1 tarcz\u0105) lub tez zderza si\u0119 inn\u0105, przeciwnie skierowan\u0105 wi\u0105zk\u0105\u00a1 cz\u0105stek (eksperyment zderzeniowy). Takie eksperymenty s\u0105 okazj\u0105 odtworzenia zjawisk i si\u0142 dzia\u0142aj\u0105cych na najbardziej podstawowym, partonowym poziomie, odtworzenia warunk\u00f3w z wn\u0119trza gwiazd, nie wy\u0142\u0105czaj\u0105c nawet niekt\u00f3rych ze zdarze\u0144 z Wielkiego Wybuchu. Wyj\u0105tkowo ciekawe s\u0105 sytuacje gdy zderzaj\u0105cymi si\u0119 obiektami b\u0119d\u0105 nie pojedyncze cz\u0105stki, ale j\u0105dra. Zgodnie z teoretycznymi przewidywaniami opartymi na QCD, przy takich zderzeniach mo\u017ce pojawi\u00a2 si\u0119 nowa posta\u0107 materii, rodzaj gor\u0105cej i g\u0119stej zupy partonowej, zwanej Plazm\u00a1 Kwarkowo- Gluonowa (QGP). &#8222;Gor\u0105ca&#8221; oznacza tu temperatur\u0119 rz\u0119du 10<sup>12<\/sup> K, a &#8222;g\u0119sta&#8221; znaczy 3-15 razy wi\u0119cej ni\u017c g\u0119sto\u015b\u0107 \u00a0j\u0105dra atomowego. G\u0142\u00f3wnym przy tym problemem, niezale\u017cnie od skomplikowania technicznego takiego eksperymentu, jest znalezienie oznak pojawienia si\u00a6 stanu QGP. Plazma ta, sk\u0142adaj\u0105ca si\u0119 z &#8222;uwolnionych&#8221; kwark\u00f3w i gluon\u00f3w sch\u0142adza si\u0119 w czasie 10<sup>-14<\/sup>s, partony przechodz\u0105 w stan hadronowego &#8222;uwi\u0119zienia&#8221;, a powsta\u0142e przy tym hadrony trafiaj\u0105 do detektor\u00f3w. W takim g\u0105szczu danych do\u015bwiadczalnych trzeba teraz odnale\u017a\u0107 ewentualne sygna\u0142y \u015bwiadcz\u0105ce o obecno\u015bci QGP.<\/p>\n<p>Eksperyment NA61\/SHINE, prowadzony na supersynchrotronie CERN SPS, jest ci\u0119\u017ckojonowym eksperymentem ze stacjonarn\u0105 tarcz\u0105. J\u0105dra, od Be+Be po Pb+Pb zderzaj\u0105 si\u0119 tam przy r\u00f3\u017cnych energiach w konfiguracjach wi\u0105zka-tarcza. G\u0142\u00f3wnym celem projektu realizowanego przez Polsko-Norweskie Konsorcjum uczestniczce w eksperymencie jest rozbudowa podstawowej cz\u0119\u015bci detektora \u2013 Kom\u00f3r Czasu Przelotu (TPC). Rozbudowa ta umo\u017cliwi rejestracje powabnych mezon\u00f3w D o sk\u0142adzie kwarkowym typu kwark powabny\/niepowabny. Od dawna istnieje dobrze uzasadniona teoretycznie hipoteza, \u017ce oznak\u0105 \u00a0pojawienia si\u0119 QGP by\u0142oby t\u0142umienie produkcji niepowabnych mezon\u00f3w w por\u00f3wnaniu z produkcj\u0105 w tym\u017ce \u015brodowisku powabnych mezon\u00f3w D. Wci\u0105\u017c bowiem brak jednoznacznych dowod\u00f3w na powstawanie plamy QGP spe\u0142niaj\u0105cej teoretyczne oczekiwania, mimo mnogo\u015bci danych do\u015bwiadczalnych z ci\u0119\u017ckojonowych zderzeniowych do\u015bwiadcze\u0144 na akceleratorach RHIC i LHC. &#8222;Powabny&#8221; program badawczy NA61\/SHINE, b\u0119d\u0105cy naturalnym rozwini\u0119ciem bada\u0144 dotycz\u0105cych przej\u015bcia do stanu QGP, wymaga zdziesi\u0119ciokrotnienia wydajno\u015bci detektor\u00f3w. Wi\u0105\u017ce si\u0119 z pytaniami zwi\u0105zanymi z u\u017cywaniem obecnych statystycznych i dynamicznych modeli w rozszerzonym zakresie mas kwarkowych. Bezpo\u015brednim celem badawczym jest otrzymanie unikalnych wynik\u00f3w do\u015bwiadczalnych o liczebno\u015bci powstaj\u0105cych par cc, mierzonych w pe\u0142nej przestrzeni fazowej. Ponadto, zostan\u0105 otrzymane unikalne wyniki dotycz\u0105ce wp\u0142ywu energii zderze\u0144 oraz wielko\u015bci system\u00f3w na procesy zderzeniowe ci\u0119\u017ckich jon\u00f3w. Powinno to pom\u00f3c odpowiedzie\u0107 na wci\u0105\u017c aktualne istotne pytania:<\/p>\n<ul>\n<li>Jaki jest mechanizm produkcji &#8222;otwartego&#8221; powabu?<\/li>\n<li>Jak uwalnianie si\u0119 parton\u00f3w wp\u0142ywa na pojawienie si\u0119 stan\u00f3w otwartego powabu?<\/li>\n<li>Jak tworzenie si\u0119 QGP wp\u0142ywa na pojawienie si\u0119 mezon\u00f3w J\/psi?<\/li>\n<\/ul>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>[\/vc_column][vc_column][\/vc_column][\/vc_row][vc_row][vc_column]<div class=\"container\"><div class=\"separator\" style=\"background-color: #EBEBEB\"><\/div><\/div>[\/vc_column][\/vc_row][vc_row][vc_column]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><\/p>\n<h1>Podmioty realizuj\u0105ce:<\/h1>\n<ol>\n<li><span id=\"entityListForm:j_idt394_data_table:0:institutionNamePl\">Uniwersytet \u015al\u0105ski w Katowicach<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:1:institutionNamePl\">University of Oslo<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:3:institutionNamePl\">University of Bergen<\/span><\/li>\n<li>Western Norway University of Applied Sciences<\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:2:institutionNamePl\">Politechnika Warszawska<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:5:institutionNamePl\">Uniw<\/span><span id=\"entityListForm:j_idt394_data_table:5:institutionNamePl\">ersytet Jagiello\u0144ski<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:6:institutionNamePl\">Uniwersytet Jana Kochanowskiego w Kielcach<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:7:institutionNamePl\">Uniwersytet Wroc\u0142awski<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:8:institutionNamePl\">Uniwersytet Warszawski<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:9:institutionNamePl\">Narodowe Centrum Bada\u0144 J\u0105drowych<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:10:institutionNamePl\">Instytut Fizyki J\u0105drowej im. Henryka Niewodnicza\u0144skiego Polskiej Akademii Nauk<\/span><\/li>\n<li><span id=\"entityListForm:j_idt394_data_table:11:institutionNamePl\">Akademia G\u00f3rniczo-Hutnicza im. Stanis\u0142awa Staszica w Krakowie<\/span><\/li>\n<\/ol>\n<p>\n<\/div>\r\n                    <\/div>\r\n                <\/div>[vc_single_image image=&#8221;2681&#8243; img_size=&#8221;large&#8221; alignment=&#8221;center&#8221; style=&#8221;vc_box_shadow_border&#8221;]\r\n                <div class=\"text-modules\">\r\n                    <div class=\"container\">\r\n                        \r\n                        <div class=\"text-modules__content\"><p><b>Spotkanie inicjuj\u0105ce projekt<\/b><\/p>\n<p><a href=\"https:\/\/indico.cern.ch\/event\/892056\/\">Strona www spotkania<\/a><\/p>\n<p>Prezentacje podczas spotkania:<\/p>\n<ul>\n<li><a href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/IArsene_NA61CollabMeeting_2020Sep23-3.pdf\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize3,43MB\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize3,43MB\">Phenomenology of open charm production in heavy-ion collisions<\/a>, \u00a0<span class=\"\">Ionut Arsene Arsene<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Oslo)<\/span><\/span><\/span><\/li>\n<li><a href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/cmos_23Sept2020..pdf\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize2,00MB\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize2,00MB\">Open charm measurements in NA61\/SHINE<\/a> Pawel Piotr Staszel<span class=\"affiliation\">\u00a0<span class=\"text\">(Jagiellonian University)<\/span><\/span><\/li>\n<li><a href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/2019\/11\/upgrade_PS.pdf\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize12,37MB\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize12,37MB\">Overview of NA61\/SHINE detector upgrade<\/a>, \u00a0<span class=\"\">Piotr Podlaski<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Warsaw)<\/span><\/span><\/span><\/li>\n<li><a href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/Nieprzypisane\/GRIEG_call_for_Polish-Norwegian_research_projects.pdf\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize347,45kB\" class=\"mtli_attachment mtli_pdf\" data-mtli=\"mtli_filesize347,45kB\">Grieg grant for funding of the NA61\/SHINE detector upgrade<\/a>, Seweryn Kowalski<span class=\"affiliation\">\u00a0<span class=\"text\">(University of Silesia)<\/span><\/span><\/li>\n<\/ul>\n<h2>G\u0142\u00f3wne zadania i dzia\u0142ania projektu w latach 2020 i 2021:<\/h2>\n<h3>Modernizacja kom\u00f3r projekcji czasowej<\/h3>\n<p>Znaczna modyfikacja spektrometru NA61\/SHINE by\u0142a planowana na lata 2019 &#8211; 2022. Modernizacja by\u0142a motywowana programem dotycz\u0105cym kwarku powabnego, kt\u00f3ry wymaga dziesi\u0119ciokrotnego zwi\u0119kszenia szybko\u015bci zbierania danych do oko\u0142o 1 kHz &#8211; g\u0142\u00f3wny temat zwi\u0105zany z t\u0105 modernizacj\u0105 i obj\u0119ty tym projektem to modernizacja kom\u00f3r TPC. Nast\u0119puj\u0105ce zadania obejmuj\u0105 ten temat:<\/p>\n<ul>\n<li>Opracowanie modelu 3D detektor\u00f3w z elektronik\u0105, systemem ch\u0142odzenia i elementami wsparcia mechanicznego<\/li>\n<li>Projektowanie, produkcja i monta\u017c mechanicznego wsparcia elektroniki i element\u00f3w ch\u0142odz\u0105cych<\/li>\n<li>Projektowanie i monta\u017c systemu niskonapi\u0119ciowego<\/li>\n<li>Projektowanie, budowa i konserwacja \u0142a\u0144cucha odczytu<\/li>\n<li>Konserwacja i dalszy rozw\u00f3j systemu kontroli detektor\u00f3w<\/li>\n<li>Konserwacja i modernizacja systemu gazowego<\/li>\n<li>Test detektora<\/li>\n<\/ul>\n<p>Przed testem na wi\u0105zce, FEC zosta\u0142 przetestowany w celu sprawdzenia ka\u017cdego elementu odczytu pod k\u0105tem szum\u00f3w i \u0142\u0105czno\u015bci. \u0141\u0105czno\u015b\u0107 z komorami odczytu zosta\u0142a przetestowana przy u\u017cyciu systemu kalibracyjnego pulsatora. System LV (Wiener PS) w swojej finalnej konfiguracji by\u0142 u\u017cywany do test\u00f3w opisanych powy\u017cej. Ponadto por\u00f3wnano poziom szum\u00f3w do tego zmierzonego wcze\u015bniej przez ALICE (gdzie dzia\u0142a\u0142a ta elektronika). Poziom szum\u00f3w jest og\u00f3lnie wy\u017cszy ni\u017c w ALICE, poniewa\u017c obwody ochronne i d\u0142ugo\u015b\u0107 \u015bcie\u017cek na p\u0142ytkach adapter\u00f3w wprowadzaj\u0105 dodatkowe szumy.<\/p>\n<p>TPC zosta\u0142 przetestowany na wi\u0105zce jesieni\u0105 2021 roku z w\u0142\u0105czonym polem magnetycznym, i zaobserwowano pierwsze \u015blady. Analiza danych zebranych podczas testu pozwala na dostrojenie parametr\u00f3w detektora.<\/p>\n<h3>Oprogramowanie<\/h3>\n<p>Przygotowano nowy system Trigger and Data Acquisition (TDAQ). Wszystkie kluczowe komponenty oprogramowania przep\u0142ywu danych zosta\u0142y opracowane i przetestowane. Obecnie jeste\u015bmy na etapie dostrajania konfiguracji. Ponadto dodawane s\u0105 nowe funkcje, takie jak interfejs u\u017cytkownika oparty na sieci i dodatkowe monitorowanie. Z punktu widzenia oprogramowania kalibracyjnego i analitycznego, wdro\u017cono nowe oprogramowanie do kalibracji straty energii (dE\/dx) w TPC. Przeprowadzono wst\u0119pn\u0105 walidacj\u0119 na danych p+Pb przy 158 GeV\/c i zbudowano system automatyzacji, aby u\u0142atwi\u0107 bezobs\u0142ugowe wykonywanie wielu etap\u00f3w kalibracji. Dodatkowo przeprowadzono szczeg\u00f3\u0142ow\u0105 inspekcj\u0119 zmienno\u015bci wzmocnienia w TPC za pomoc\u0105 map wzmocnienia pad\u00f3w dla ka\u017cdego sektora TPC, uzyskanych z widm \u0142adunku na padzie wynikaj\u0105cych z wtrysku i p\u00f3\u017aniejszego rozpadu izotopu 83Kr w komorach. Zmodernizowana elektronika TPC dostarcza dane w nowym formacie surowych danych, a odpowiednia infrastruktura do dekodowania i analizowania danych musi by\u0107 dost\u0119pna w ramach SHINE Offline Framework. Podczas testowania elektroniki TPC napisano parser surowych danych detektora, kt\u00f3ry by\u0142 u\u017cywany do oceny jako\u015bci surowych danych TPC. Ten parser zostanie przeniesiony do bibliotek I\/O w Offline Framework. Drugi parser zosta\u0142 napisany w celu przet\u0142umaczenia surowych kana\u0142\u00f3w elektroniki front-end TPC na fizyczne obiekty pad\u00f3w TPC, co jest kluczowym krokiem w kierunku rekonstrukcji danych. Prace zwi\u0105zane z symulacjami Monte Carlo by\u0142y g\u0142\u00f3wnie po\u015bwi\u0119cone wdro\u017ceniu nowej wersji GEANT 4.0, narz\u0119dzia do symulacji przej\u015bcia cz\u0105stek przez materi\u0119, oraz wdro\u017ceniu algorytmu \u015bledzenia opartego na filtrze Kalmana.<\/p>\n<p>Najwa\u017cniejszym osi\u0105gni\u0119ciem w zakresie utrzymania zasob\u00f3w IT by\u0142a przej\u015bcie z Jenkins do GitLab CI. To zapewni\u0142o wersjonowanie konfiguracji CI, testowanego oprogramowania, automatyczne sprawdzanie wszystkich ga\u0142\u0119zi oraz podzia\u0142 pipeline&#8217;\u00f3w na etapy. Dostarczono cztery wersje oprogramowania, wspieraj\u0105ce rozw\u00f3j nowego oprogramowania rekonstrukcyjnego, ulepszenia w Monte Carlo oraz liczne poprawki b\u0142\u0119d\u00f3w i optymalizacje.<\/p>\n<h3>Fizyka kwarku powabnego<\/h3>\n<p>G\u0142\u00f3wne dzia\u0142ania by\u0142y zwi\u0105zane z analiz\u0105 danych pilota\u017cowych zebranych przed modernizacj\u0105 TPC. Ponadto przeprowadzono analiz\u0119 w celu uzyskania wydajno\u015bci produkcji otwartego powabu, danych pilota\u017cowych przy u\u017cyciu r\u00f3\u017cnych modeli statystycznych i strunowych oraz wcze\u015bniejszych pomiar\u00f3w (eksperyment NA60\/NA50). Prace s\u0105 nadal w toku.<\/p>\n<h2>G\u0142\u00f3wne zadania i dzia\u0142ania projektu w 2023 roku: Modernizacja kom\u00f3r projekcji czasowej<\/h2>\n<p>Modernizacja detektora LS2 zosta\u0142a zako\u0144czona. Nowe i zmodernizowane detektory zosta\u0142y uruchomione za pomoc\u0105 wi\u0105zek hadron\u00f3w wiosn\u0105 2022 roku. Uruchomienie z wi\u0105zk\u0105 Pb przy 150A GeV\/c oraz pierwsze zbieranie danych dotycz\u0105cych produkcji otwartego powabu w zderzeniach Pb+Pb mia\u0142o miejsce w listopadzie 2022 roku.<\/p>\n<p>Przebieg eksperymentu dowi\u00f3d\u0142, \u017ce g\u0142\u00f3wny cel modernizacji zosta\u0142 osi\u0105gni\u0119ty. Maksymalna szybko\u015b\u0107 zbierania danych osi\u0105gn\u0119\u0142a 1,6 kHz, znacznie wy\u017csz\u0105 ni\u017c zak\u0142adane 1 kHz. Modernizacja elektroniki TPC wp\u0142yn\u0119\u0142a na jako\u015b\u0107 zebranych danych, co pokazano na poni\u017cszym rysunku:<\/p>\n<p><img class=\"aligncenter\" src=\"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-content\/uploads\/sites\/39\/Bez-kategorii\/Picture1-1.png\" \/><\/p>\n<p>Znaczny wysi\u0142ek, jaki uczestnicy w\u0142o\u017cyli w modernizacj\u0119 detektora, otwiera nowe mo\u017cliwo\u015bci dla pomiar\u00f3w fizycznych i zapewnia dzia\u0142anie eksperymentu na nast\u0119pne kilka lat.<\/p>\n<h3>Oprogramowanie<\/h3>\n<p>Oprogramowanie do rekonstrukcji i kalibracji jest stale utrzymywane i rozwijane. Znaczny wysi\u0142ek zosta\u0142 po\u015bwi\u0119cony opracowaniu oprogramowania dla zmodernizowanego detektora. Pozwoli\u0142o to na efektywne monitorowanie online i offline podczas zbierania danych fizycznych w 2022 roku, a tak\u017ce kalibracj\u0119 Kr zmodernizowanych Kom\u00f3r Projekcji Czasowej.<\/p>\n<h3>Fizyka kwarku powabnego<\/h3>\n<p>W 2023 roku wi\u0105zka Pb o momencie 150A GeV\/c zosta\u0142a dostarczona do eksperymentu NA61\/SHINE 16 listopada. Po tygodniu konfiguracji rozpocz\u0119to zbieranie danych produkcyjnych z 3 mm o\u0142owianym celem, zapewniaj\u0105cym 6% prawdopodobie\u0144stwo interakcji. Dane by\u0142y zbierane z u\u017cyciem bezstronnego wyzwalacza interakcji T2 (zidentyfikowana interakcja) oraz wyzwalacza wi\u0105zki T1 (zidentyfikowana wi\u0105zka) zredugowanego o czynnik 100. Ca\u0142kowita liczba zdarze\u0144 wyzwalaj\u0105cych interakcj\u0119 zebranych podczas tygodnia zbierania danych produkcyjnych wynosi 50 milion\u00f3w. Obejmuje to oko\u0142o 30 milion\u00f3w zderze\u0144 Pb+Pb. By\u0142 to pierwszy pomiar NA61\/SHINE z wi\u0105zk\u0105 jon\u00f3w o\u0142owiu wykonany po modernizacji sprz\u0119tu podczas Drugiego D\u0142ugiego Wy\u0142\u0105czenia (Long Shutdown 2).<\/p>\n<p>Spotkanie projektowe (spotkanie \u015bredniej wielko\u015bci)<\/p>\n<p><a href=\"https:\/\/indico.cern.ch\/event\/1241273\/\">https:\/\/indico.cern.ch\/event\/1241273\/<\/a><\/p>\n<p>&nbsp;<\/p>\n<p>\n<style type=\"text\/css\">a[data-mtli~=\"mtli_filesize3,43MB\"]:after {content:\" (3,43 MB)\"}a[data-mtli~=\"mtli_filesize2,00MB\"]:after {content:\" (2,00 MB)\"}a[data-mtli~=\"mtli_filesize12,37MB\"]:after {content:\" (12,37 MB)\"}a[data-mtli~=\"mtli_filesize347,45kB\"]:after {content:\" (347,45 kB)\"}<\/style><\/div>\r\n                    <\/div>\r\n                <\/div>[\/vc_column][\/vc_row][vc_row][vc_column][\/vc_column][\/vc_row]<\/p>\n<style type=\"text\/css\">a[data-mtli~=\"mtli_filesize3,43MB\"]:after {content:\" (3,43 MB)\"}a[data-mtli~=\"mtli_filesize2,00MB\"]:after {content:\" (2,00 MB)\"}a[data-mtli~=\"mtli_filesize12,37MB\"]:after {content:\" (12,37 MB)\"}a[data-mtli~=\"mtli_filesize347,45kB\"]:after {content:\" (347,45 kB)\"}<\/style>","protected":false},"excerpt":{"rendered":"<p>[vc_row][vc_column][vc_single_image image=&#8221;2725&#8243; img_size=&#8221;medium&#8221; alignment=&#8221;center&#8221;][\/vc_column][\/vc_row][vc_row][vc_column][\/vc_column][\/vc_row][vc_row][vc_column][vc_single_image image=&#8221;2726&#8243; img_size=&#8221;large&#8221; alignment=&#8221;center&#8221;][\/vc_column][\/vc_row][vc_row][vc_column][\/vc_column][\/vc_row] &nbsp; [vc_row][vc_column][vc_single_image image=&#8221;2636&#8243; alignment=&#8221;center&#8221;][\/vc_column][vc_column][\/vc_column][\/vc_row][vc_row][vc_column][\/vc_column][\/vc_row][vc_row][vc_column][vc_single_image image=&#8221;2681&#8243; img_size=&#8221;large&#8221; alignment=&#8221;center&#8221; style=&#8221;vc_box_shadow_border&#8221;][\/vc_column][\/vc_row][vc_row][vc_column][\/vc_column][\/vc_row] [&#8230;]<\/p>\n<p><a class=\"btn btn-secondary understrap-read-more-link\" href=\"https:\/\/us.edu.pl\/instytut\/ifiz\/badanie-produkcji-powabu-w-zderzeniach-ciezkich-jonow\/\">Read More&#8230;<\/a><\/p>\n","protected":false},"author":104,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_expiration-date-status":"saved","_expiration-date":0,"_expiration-date-type":"","_expiration-date-categories":[],"_expiration-date-options":[]},"acf":[],"_links":{"self":[{"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/pages\/2337"}],"collection":[{"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/users\/104"}],"replies":[{"embeddable":true,"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/comments?post=2337"}],"version-history":[{"count":0,"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/pages\/2337\/revisions"}],"wp:attachment":[{"href":"https:\/\/us.edu.pl\/instytut\/ifiz\/wp-json\/wp\/v2\/media?parent=2337"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}