Nuclear Physics Consolidated Grant

核物理综合拨款

• 批准号: ST/P005047/1
• 负责人: Lee Barnby
• 金额: $ 2.3万
• 依托单位: University of Derby
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2017
• 资助国家: 英国
• 起止时间: 2017 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FP005047%2F1
• 关键词: Nuclear; Physics; Consolidated; Grant

The majority of the visible mass of the universe is made up of atomic nuclei that lie at the centre of atoms. Nuclear physics seeks to answer fundamental questions such as: "How do the laws of physics work when driven to the extremes? What are the fundamental constituents and fabric of the universe and how do they interact? How did the universe begin and how is it evolving? What is the nature of nuclear and hadronic matter?" The aim of our research is to study the properties of atomic nuclei and to measure the properties of hot nuclear matter in order to answer these questions. No one yet knows how heavy a nucleus can be; in other words, just how many neutrons and protons can be made to bind together. We will study the heaviest nuclei that can be made in the laboratory and determine their properties which will allow better predictions to be made for the "superheavies". For lighter nuclei we will explore in the region of the proton and neutron drip lines, which are the borders between bound and unbound nuclei. We will determine more precisely than ever before the location of these drip lines. Nuclei beyond the proton drip line have so much electrical charge that they are highly unstable and try to achieve greater stability through the process of proton emission. We will investigate how nuclear behaviour is affected when protons become unbound.For these exotic systems we will also explore how the nucleus prefers to rearrange its shape, which can be a sphere, rugby ball, pear, etc. and how it stores its energy among the possible degrees of freedom. We will also investigate how the properties of these nuclei develop as we make them spin faster and faster. We will try to determine the precise nature of ultra high spin states in heavy nuclei, just before the nucleus breaks up due to fission. By violently removing a nucleon from a nucleus in a nuclear reaction at high energies and measuring its properties, we can investigate to what extent the nucleon "feels" the influence of its neighbouring nucleons, whether it is correlated with them. Such information tells us about the nuclear force inside the nucleus at different inter-nucleon distances. Nuclear matter can exist in different phases, analogous to the solid, liquid, gas and plasma phases in ordinary substances. By varying the temperature, density or pressure, nuclear matter can undergo a transition from one phase to another. In extreme conditions of density and temperature (about 100 thousands times more than the temperature at the heart of the sun!), a phase transition should occur and quarks and gluons (of which the protons and neutrons are made of) should exist in a new state of matter called the Quark-Gluon Plasma. By colliding nuclei together at high energies at the Large Hadron Collider at CERN, we will study properties of this new state of matter. Such information is not only important for nuclear physics but also to understand neutron stars and other compact astrophysical objects.This programme of research will employ a large variety of experimental methods to probe many aspects of nuclear structure and the phases of strongly interacting matter, mostly using instrumentation that we have constructed at several world-leading accelerator laboratories. The work will require a series of related experiments at a range of facilities in order for us to gain an insight into the answers to the questions posed above. These experiments will help theorists to refine and test their calculations that have attempted to predict the properties of nuclei and nuclear matter, often with widely differing results. The resolution of this problem will help us to describe complex many-body nuclear systems and better understand conditions in our universe a few fractions of a second after the big bang.

宇宙的大部分可见质量由位于原子中心的原子核组成。核物理学试图回答诸如：“物理定律在极端行驶时如何起作用？宇宙的基本成分和结构是什么？它们如何相互作用？宇宙如何开始？它如何发展？我们研究的目的是研究原子核的特性并测量热核物质的特性，以回答这些问题。还没有人知道核的沉重。换句话说，可以使多少个中子和质子结合在一起。我们将研究可以在实验室中制作的最重的核，并确定其特性，这将使对“超级疾病”做出更好的预测。对于较轻的核，我们将在质子和中子滴注线的区域进行探索，这些区域是结合和未结合核之间的边界。在这些滴水线的位置之前，我们将比以往任何时候都更精确。质子滴水线以外的核具有太多的电荷，以至于它们高度不稳定，并试图通过质子发射过程实现更大的稳定性。我们将研究当质子变得无束缚时如何影响核行为。对于这些外来系统，我们还将探索核如何重新排列其形状，这可以是球体，橄榄球，梨，梨等，以及它如何在可能的自由度之间存储其能量。我们还将研究这些核的性质如何发展，因为它们使它们越来越快，更快。我们将尝试确定核因裂变而分解的重核中超高态的精确性。通过在高能以核反应中的核反应中从核中猛烈地去除核子并测量其性质，我们可以研究核子在多大程度上“感觉到”其相邻核的影响，无论它是否与它们相关。此类信息告诉我们有关不同核间距离内细胞核内部的核力量。核物质可以以不同的阶段存在，类似于普通物质中的固体，液体，气体和血浆相。通过改变温度，密度或压力，核物质可以从一个相到另一个相的过渡。在密度和温度的极端条件下（比太阳中心的温度高约1万倍！），应发生相变，夸克和胶子（质子和中子的制成）应以一种称为夸克 - 胶状质量的新物质状态存在。通过在CERN大型强子对撞机的高能量上将核一起碰撞，我们将研究这种新物质状态的特性。这样的信息不仅对核物理学很重要，而且要了解中子恒星和其他紧凑的天体物理对象。这项研究计划将采用多种实验方法来探测核结构的许多方面以及强烈相互作用的物质的各个阶段，主要是使用我们在几个世界领先的Accelerator Laberatories中构建的仪器。这项工作将需要一系列相关的实验，以便我们深入了解上述问题的答案。这些实验将帮助理论家改进和测试其试图预测核和核物质特性的计算，通常会有很大不同的结果。解决这个问题的解决将有助于我们描述复杂的多体核系统，并更好地理解宇宙中的条件，这是大爆炸之后的几秒钟。

项目成果

Neutron emission in ultraperipheral Pb-Pb collisions at s N N = 5.02 TeV

s N N = 5.02 TeV 超外周 Pb-Pb 碰撞中的中子发射

• DOI: 10.1103/physrevc.107.064902
• 发表时间: 2023
• 期刊: Physical Review C
• 影响因子: 3.1
• 作者: Acharya S

Multiplicity dependence of $$\pi $$, K, and p production in pp collisions at $$\sqrt{s} = 13$$ TeV

• DOI: 10.1140/epjc/s10052-020-8125-1
• 发表时间: 2020-08
• 期刊: The European Physical Journal C
• 作者: S. Acharya;D. Adamová;A. Adler;J. Adolfsson;M. Aggarwal;G. Rinella;M. Agnello;N. Agrawal;Z. Ahammed;S. Ahmad;S. Ahn;A. Akindinov;M. Al-Turany;S. Alam;D. Albuquerque;D. Aleksandrov;B. Alessandro;H. Alfanda;R. A. Molina;B. Ali;Y. Ali;A. Alici;A. Alkin;J. Alme;T. Alt;L. Altenkamper;I. Altsybeev;M. Anaam;C. Andrei;D. Andreou;H. A. Andrews;A. Andronic;M. Angeletti;V. Anguelov;C. Anson;T. Antičić;F. Antinori;P. Antonioli;N. Apadula;L. Aphecetche;H. Appelshäuser;S. Arcelli;R. Arnaldi;M. Arratia;I. Arsene;M. Arslandok;A. Augustinus;R. Averbeck;S. Aziz;M. D. Azmi;A. Badalà;Y. Baek;S. Bagnasco;X. Bai;R. Bailhache;R. Bala;A. Balbino;A. Baldisseri;M. Ball;S. Balouza;D. Banerjee;R. Barbera;L. Barioglio;G. G. Barnaföldi-G.;L. Barnby;V. Barret;P. Bartalini;K. Barth;E. Bartsch;F. Baruffaldi;N. Bastid;S. Basu;G. Batigne;B. Batyunya;D. Bauri;J. L. Alba;I. Bearden;C. Beattie;C. Bedda;N. Behera;I. Belikov;A. B. Hechavarria;F. Bellini;R. Bellwied;V. Belyaev;G. Bencédi;S. Beole;A. Bercuci;Y. Berdnikov;D. Berényi;R. Bertens;D. Berzano;M. Besoiu;L. Betev;A. Bhasin;I. R. Bhat;M. A. Bhat;H. Bhatt;B. Bhattacharjee;A. Bianchi;L. Bianchi;N. Bianchi;J. Bielcik;J. Bielčíková;A. Bilandzic;G. Bíró;R. Biswas;S. Biswas;J. Blair;D. Blau;C. Blume;G. Boca;F. Bock;F. Bock;A. Bogdanov;S. Boi;L. Boldizsár;A. Bolozdynya;M. Bombara;G. Bonomi;H. Borel;A. Borissov;H. Bossi;E. Botta;L. Bratrud;P. Braun-Munzinger;M. Bregant;M. Broz;E. Bruna;G. Bruno;M. Buckland;D. Budnikov;H. Buesching;S. Bufalino;O. Bugnon;P. Buhler;P. Buncic;Z. Buthelezi;Z. Buthelezi;J. Butt;J. Buxton;S. Bysiak;D. Caffarri;A. Caliva;E. C. Villar;R. S. Camacho;P. Camerini;A. Capon;F. Carnesecchi;R. Caron;J. Castellanos;A. Castro;E. Casula;F. Catalano;C. C. Sanchez-C.;P. Chakraborty;S. Chandra;W. Chang;S. Chapeland;M. Chartier;S. Chattopadhyay;A. Chauvin;C. Cheshkov;B. Cheynis;V. Barroso;D. Chinellato;Soyeon Cho;P. Chochula;T. Chowdhury;P. Christakoglou;C. H. Christensen;P. Christiansen;T. Chujo;C. Cicalò;L. Cifarelli;F. Cindolo;G. Clai;J. Cleymans;F. Colamaria;D. Colella;A. Collu;M. Colocci;M. Concas;G. C. Balbastre;Z. C. Valle;G. Contin;J. G. Contreras;T. Cormier;Y. C. Morales;P. Cortese;M. R. Cosentino;F. Costa;S. Costanza;P. Crochet;E. Cuautle;P. Cui;L. Cunqueiro;D. Dabrowski;T. Dahms;A. Dainese;F. Damas;F. Damas;M. C. Danisch;A. Danu;D. Das;I. Das;P. Das;Shankar P. Das;A. Dash;S. Dash;S. De;A. Caro;G. Cataldo;J. Cuveland;A. Falco;D. Gruttola;N. Marco;S. Pasquale;S. Deb;H. F. Degenhardt;K. Deja;A. Deloff;S. Delsanto;W. Deng;D. Devetak;P. Dhankher;D. Bari;A. Mauro;R. Diaz;T. Dietel;P. Dillenseger;Yanchun Ding;R. Divià;D. Dixit;O. Djuvsland;U. Dmitrieva;A. Dobrin;B. Donigus;O. Dordic;A. Dubey;A. Dubla;S. Dudi;M. Dukhishyam;P. Dupieux;R. Ehlers;R. Ehlers;V. Eikeland;D. Elia;E. Epple;B. Erazmus;F. Erhardt;A. Erokhin;M. R. Ersdal;B. Espagnon;G. Eulisse;D. Evans;S. Evdokimov;L. Fabbietti;M. Faggin;J. Faivre;F. Fan;A. Fantoni;M. Fasel;P. Fecchio;A. Feliciello;G. Feofilov;A. F. Tellez;A. Ferrero;A. Ferretti;A. Festanti;V. Feuillard;J. Figiel;S. Filchagin;D. Finogeev;F. Fionda;G. Fiorenza;Fernando Antonio Flor;S. Foertsch;P. Foka;S. Fokin;E. Fragiacomo;U. Frankenfeld;U. Fuchs;C. Furget;A. Furs;M. Girard;J. Gaardhøje;M. Gagliardi;A. Gago;A. Gal;C. D. Galván;P. Ganoti;C. Garabatos;E. Garcia-Solis;K. Garg;C. Gargiulo;A. Garibli;K. Garner;P. Gasik;E. Gauger;M. Germain;J. Ghosh;M. Giacalone;P. Ghosh;S. Ghosh;P. Gianotti;P. Giubellino;P. Giubilato;P. Glassel;A. Ramírez;V. Gonzalez;L. González-Trueba;S. Gorbunov;L. Gorlich;A. Goswami;S. Gotovac;V. Grabski;L. Graczykowski;K. Graham;L. Greiner;A. Grelli;C. Grigoras;V. Grigoriev;A. Grigoryan;S. Grigoryan;O. Groettvik;F. Grosa;J. Grosse-Oetringhaus;R. Grosso;R. Guernane;M. Guittiere;K. Gulbrandsen;T. Gunji;A. Gupta;Ramni Gupta;I. B. Guzman;R. Haake;M. Habib;C. Hadjidakis;H. Hamagaki;G. Hamar;M. Hamid;R. Hannigan;M. R. Haque;M. R. Haque;A. Harlenderova;J. Harris;A. Harton;J. Hasenbichler;H. Hassan;D. Hatzifotiadou;P. Hauer;S. Hayashi;S. Heckel;S. Heckel;E. Hellbar;H. Helstrup;A. Herghelegiu;T. Herman;E. G. Hernández;G. H. Corral;F. Herrmann;K. Hetland;H. Hillemanns;C. Hills;B. Hippolyte;B. Hohlweger;J. Honermann;D. Hořák;A. Hornung;S. Hornung;R. Hosokawa;P. Hristov;Chun-lu Huang;C. Hughes;P. Huhn;T. Humanic;H. Hushnud;L. A. Husova;N. Hussain;S. Hussain;D. Hutter;J. P. Iddon;J. P. Iddon;R. Ilkaev;H. Ilyas;M. Inaba;G. Innocenti;M. Ippolitov;A. Isakov;M. S. Islam;M. Ivanov;V. Ivanov;V. Izucheev;B. Jacak;N. Jacazio;P. Jacobs;S. Jadlovska;J. Jadlovský;S. Jaelani;C. Jahnke;M. Jakubowska;M. Janik;T. Janson;M. Jercic;O. Jevons;M. Jin;F. Jonas;P. G. Jones;Jerome Jung;M. Jung;A. Jusko;P. Kalinak;A. Kalweit;V. Kaplin;S. Kar;A. Uysal;O. Karavichev;T. Karavicheva;P. Karczmarczyk;E. Karpechev;U. Kebschull;R. Keidel;M. Keil;B. Ketzer;Z. Khabanova;A. M. Khan;Shaista Khan;S. Khan;A. Khanzadeev;Y. Kharlov;A. Khatun;A. Khuntia;B. Kileng;Beomkyu Kim;D. Kim;D. Kim;E. Kim;H. Kim;H. Kim;Jinsook Kim;J. Kim;Minjung Kim;Se Yong Kim;T. Kim;S. Kirsch;I. Kisel;S. Kiselev;A. Kisiel;J. Klay;C. Klein;J. Klein;S. Klein;C. Klein-Bösing;M. Kleiner;A. Kluge;M. L. Knichel;A. Knospe;C. Kobdaj;M. Kohler;T. Kollegger;A. Kondratyev;N. Kondratyeva;E. Kondratyuk;J. Konig;P. Konopka;L. Koska;O. Kovalenko;V. Kovalenko;M. Kowalski;I. Králik;A. Kravčáková;L. Kreis;M. Krivda;M. Krivda;F. Krizek;K. Gajdosova;M. Kruger;E. Kryshen;M. Krzewicki;A. Kubera;V. Kučera;V. Kučera;C. Kuhn;P. Kuijer;L. Kumar;S. Kundu;P. Kurashvili;A. Kurepin;A. Kurepin;A. Kuryakin;S. Kushpil;J. Kvapil;M. Kweon;J. Kwon;Y. Kwon;S. L. Pointe;P. Rocca;Y. S. Lai;R. Langoy;K. Lapidus;A. Lardeux;P. Larionov;E. Laudi;R. Lávička;T. Lazareva;R. Lea;L. Leardini;Joonil Lee;S. Lee;F. Lehas;S. Lehner;J. Lehrbach;R. Lemmon;I. Monzón;E. Lesser;M. Lettrich;P. Lévai;Xiang Li;X. Li;J. Lien;R. Lietava;B. Lim;V. Lindenstruth;S. Lindsay;C. Lippmann;M. Lisa;A. Liu;Suyuan Liu;W. Llope;I. Lofnes;V. Loginov;C. Loizides;P. Loncar;J. Lopez;X. Lopez;E. L. Torres;J. R. Luhder;M. Lunardon;G. Luparello;Y. Ma;A. Maevskaya;M. Mager;S. Mahmood;T. Mahmoud;A. Maire;R. Majka;M. Malaev;Q. W. Malik;L. Malinina;D. Mal’Kevich;P. Malzacher;G. Mandaglio;V. Manko;F. Manso;V. Manzari;Y. Mao;M. Marchisone;J. Mareš;G. Margagliotti;A. Margotti;J. Margutti;A. Marín;C. Markert;M. Marquard;C. Martin;N. Martin;P. Martinengo;M. Martínez;G. García;S. Masciocchi;M. Masera;A. Masoni;L. Massacrier;E. Masson;A. Mastroserio;A. Mathis;O. Matonoha;P. Matuoka;A. Matyja;C. Mayer;F. Mazzaschi;M. Mazzilli;M. Mazzoni;A. Mechler;F. Meddi;Y. Melikyan;A. Menchaca-Rocha;C. Mengke;E. Meninno;M. Meres;S. Mhlanga;Y. Miake;L. Micheletti;D. Mihaylov;K. Mikhaylov;K. Mikhaylov;A. N. Mishra;D. Miśkowiec;A. Modak;N. Mohammadi;A. Mohanty;B. Mohanty;M. M. Khan-M.;Z. Moravcova;C. Mordasini;D. Godoy;L. Moreno;I. Morozov;A. Morsch;T. Mrnjavac;V. Muccifora;E. Mudnić;D. Muhlheim;S. Muhuri;J. Mulligan;M. Munhoz;R. Munzer;H. Murakami;S. Murray;L. Musa;J. Musinsky;C. Myers;J. Myrcha;B. Naik;R. Nair;B. Nandi;R. Nania;E. Nappi;M. U. Naru;A. Nassirpour;C. Nattrass;R. Nayak;T. Nayak;S. Nazarenko;A. Neagu;R. A. Oliveira;L. Nellen;S. V. Nesbø;G. Neskovic;D. Nesterov;L. Neumann;B. Nielsen;S. Nikolaev;S. Nikulin;V. Nikulin;F. Noferini;P. Nomokonov;J. Norman;J. Norman;N. Novitzky;P. Nowakowski;A. Nyanin;J. Nystrand;M. Ogino;A. Ohlson;A. Ohlson;J. Oleniacz;A. C. O. D. Silva;M. Oliver;C. Oppedisano;A. O. Velasquez;A. Oskarsson;J. Otwinowski;K. Oyama;Y. Pachmayer;V. Pacik;D. Pagano;G. Paic;J. Pan;S. Panebianco;P. Pareek;P. Pareek;Jongha Park;J. Parkkila;S. Parmar;S. Pathak;B. Paul;H. Pei;T. Peitzmann;X. Peng;L. G. Pereira;H. P. D. Costa;D. Peresunko;G. Perez;Y. Pestov;V. Petráček;M. Petrovici;R. P. Pezzi;S. Piano;M. Pikna;P. Pillot;O. Pinazza;L. Pinsky;C. Pinto;S. Pisano;D. Pistone;M. Płoskoń;M. Planinić;F. Pliquett;S. Pochybova;M. Poghosyan;B. Polichtchouk;N. Poljak;A. Pop;S. Porteboeuf-Houssais;V. Pozdniakov;S. Prasad;R. Preghenella;F. Prino;C. Pruneau;I. Pshenichnov;M. Puccio;J. Putschke;L. Quaglia;R. Quishpe;S. Ragoni;S. Raha;S. Rajput;J. Rak;A. Rakotozafindrabe;L. Ramello;F. Rami;S. Ramirez;R. Raniwala;S. Raniwala;S. Räsänen;R. Rath;V. Ratza;I. Ravasenga;K. Read;K. Read;A. Redelbach;K. Redlich;A. Rehman;P. Reichelt;F. Reidt;X. Ren;R. Renfordt;Z. Rescakova;K. Reygers;V. Riabov;T. Richert;T. Richert;M. Richter;P. Riedler;W. Riegler;F. Riggi;C. Ristea;S. P. Rode;M. R. Cahuantzi;K. Røed;R. Rogalev;E. Rogochaya;D. Rohr;D. Røhrich;P. Rokita;F. Ronchetti;E. Rosas;K. Rosłon;A. Rossi;A. Rotondi;A. Roy;P. Roy;O. V. Rueda;R. Rui;B. Rumyantsev;A. Rustamov;E. Ryabinkin;Y. Ryabov;A. Rybicki;H. Rytkonen;O. Saarimaki;S. Sadhu;S. Sadovsky;K. Šafařík;S. Saha;B. Sahoo;P. Sahoo;R. Sahoo;S. Sahoo;P. Sahu;J. Saini;S. Sakai;S. Sambyal;V. Samsonov;D. Sarkar;N. Sarkar;P. Sarma;V. Sarti;M. Sas;E. Scapparone;J. Schambach;H. S. Scheid;C. Schiaua;R. Schicker;A. Schmah;C. Schmidt;H. Schmidt;M. Schmidt;M. Schmidt;N. Schmidt;N. Schmidt;A. Schmier;J. Schukraft;Y. Schutz;Y. Schutz;K. Schwarz;K. Schweda;G. Scioli;E. Scomparin;M. Šefčík;J. Seger;Y. Sekiguchi;D. Sekihata;I. Selyuzhenkov;S. Senyukov;D. Serebryakov;E. Serradilla;A. Sevcenco;A. Shabanov;A. Shabetai;R. Shahoyan;W. Shaikh;A. Shangaraev;A. Sharma;H. Sharma;M. Sharma;N. Sharma;S. Sharma;A. I. Sheikh;K. Shigaki;M. Shimomura;S. Shirinkin;Q. Shou;Y. Sibiriak;S. Siddhanta;T. Siemiarczuk;D. Silvermyr;G. Simatović;G. Simonetti;B. Singh;R. Singh;V. Singh;V. Singhal;T. Sinha;B. Sitar;M. Sitta;T. B. Skaali;M. Slupecki;N. Smirnov;R. Snellings;C. Soncco;Jihye Song;A. Songmoolnak;F. Soramel;S. Sorensen;I. Sputowska;J. Stachel;I. Stan;P. Stankus;P. Steffanic;E. Stenlund;D. Stocco;M. Storetvedt;L. Stritto;A. Suaide;T. Sugitate;C. Suire;M. Suleymanov;M. Šuljić;R. Sultanov;M. Šumbera;V. Sumberia;S. Sumowidagdo;S. Swain;A. Szabo;I. Szarka;U. Tabassam;S. F. Taghavi;G. Taillepied;J. Takahashi;G. Tambave;S. Tang;S. Tang;M. Tarhini;M. Tarzila;A. Tauro;G. T. Muñoz;A. Telesca;L. Terlizzi;C. Terrevoli;D. Thakur;S. Thakur;D. Thomas;F. Thoresen;R. Tieulent;A. Tikhonov;A. Timmins;A. Toia;N. Topilskaya;M. Toppi;F. Torales-Acosta;S. R. Torres;S. R. Torres;A. Trifirò;S. Tripathy;S. Tripathy;T. Tripathy;S. Trogolo;G. Trombetta;L. Tropp;V. Trubnikov;W. Trzaska;T. Trzciński;B. Trzeciak;B. Trzeciak;T. Tsuji;A. Tumkin;R. Turrisi;T. Tveter;K. Ullaland;Ejiro Naomi Umaka;A. Uras;G. Usai;M. Vala;N. Valle;S. Vallero;N. Kolk;L. Doremalen;M. Leeuwen;P. Vyvre;D. Varga;Z. Varga;M. Varga-Kofarago;A. Vargas;M. Vasileiou;A. Vasiliev;O. Doce;V. Vechernin;E. Vercellin;S. Limon;L. Vermunt;R. Vernet;R. Vértesi;L. Vicković;Z. Vilakazi;O. Baillie;G. Vino;A. Vinogradov;T. Virgili;V. Vislavicius;A. Vodopyanov;B. Volkel;M. Volkl;K. Voloshin;S. Voloshin;G. Volpe;B. Haller;I. Vorobyev;D. Vošček;J. Vrláková;B. Wagner;M. Weber;A. Wegrzynek;S. Wenzel;J. Wessels;J. Wiechula;J. Wikne;G. Wilk;J. Wilkinson;G. Willems;E. Willsher;B. Windelband;M. Winn;W. Witt;Y. Wu;R. Xu;S. Yalcin;Y. Yamaguchi;K. Yamakawa;Shiming Yang;S. Yano;Z. Yin;H. Yokoyama;I. Yoo;J. Yoon;S. Yuan;A. Yuncu;V. Yurchenko;V. Zaccolo;A. Zaman;C. Zampolli;H. Zanoli;N. Zardoshti;A. Zarochentsev;P. Zavada;N. Zaviyalov;H. Zbroszczyk;M. Zhalov;Song Zhang;Xiaoming Zhang;Z. Zhang;V. Zherebchevskii;D. Zhou;You Zhou;Zhuo Zhou;J. Zhu;Ya Zhu;A. Zichichi;G. Zinovjev;N. Zurlo

Probing the Effects of Strong Electromagnetic Fields with Charge-Dependent Directed Flow in Pb-Pb Collisions at the LHC.

利用电荷相关定向流探索 LHC 中 Pb-Pb 碰撞中强电磁场的影响。

• DOI: 10.1103/physrevlett.125.022301
• 发表时间: 2020
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: Acharya S