Proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions studied with HADES
Phys. Rev. C 102, 024914 (2020) We present an analysis of proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions measured with the High-Acceptance DiElectron Spectrometer (HADES) at GSI. With the help of extensive detector simulations done with IQMD transport model events including...
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| creator | Adamczewski-Musch, J Arnold, O Behnke, C Belyaev, A Berger-Chen, J. C Biernat, J Blanco, A Blume, C Bordalo, P Chernenko, S Deveaux, C Dybczak, A Epple, E Fabbietti, L Fateev, O Filip, P Fonte, P Franco, C Friese, J Fr"ohlich, I Galatyuk, T Garzon, J. A Gernh"auser, R Greifenhagen, R Guber, F Gumberidze, M Harabasz, S Heinz, T Hennino, T Hlavac, S H"ohne, C Holzmann, R Ierusalimov, A Ivashkin, A K"ampfer, B Kardan, B Koenig, I Koenig, W Kolb, B. W Kotte, R Kunz, T Kurilkin, A Kurilkin, P Ladygin, V Lalik, R Lapidus, K Lebedev, A Lopes, L Lorenz, M Maier, L Mangiarotti, A Markert, J Maurus, S Michel, J Morozov, S M"untz, C M"unzer, R Naumann, L Nowakowski, K Palka, M Parpottas, Y Pechenov, V Pechenova, O Petukhov, O Piasecki, K Pietraszko, J Przygoda, W Ramos, S Ramstein, B Reshetin, A Rodriguez-Ramos, P Rosier, P Rost, A Rustamov, A Sadovsky, A Salabura, P Scheib, T Schuldes, H Scozzi, F Seck, F Sellheim, P Selyuzhenkov, I Siebenson, J Silva, L Sobolev, Yu. G Spataro, S Str"obele, H Stroth, J Strzempek, P Sturm, C Tlusty, P Traxler, M Tsertos, H Usenko, E Wagner, V Wendisch, C Wiebusch, M. G Wirth, J Zanevsky, Y Zumbruch, P |
| description | Phys. Rev. C 102, 024914 (2020) We present an analysis of proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4
GeV Au+Au collisions measured with the High-Acceptance DiElectron Spectrometer
(HADES) at GSI. With the help of extensive detector simulations done with IQMD
transport model events including nuclear clusters, various nuisance effects
influencing the observed proton cumulants have been investigated. Acceptance
and efficiency corrections have been applied as a function of fine grained
rapidity and transverse momentum bins, as well as considering local track
density dependencies. Next, the effects of volume changes within particular
centrality selections have been considered and beyond-leading-order corrections
have been applied to the data. The efficiency and volume corrected proton
number moments and cumulants Kn of orders n = 1, . . . , 4 have been obtained
as a function of centrality and phase-space bin, as well as the corresponding
correlators C_n . We find that the observed correlators show a power-law
scaling with the mean number of protons, i.e. $C_n \propto ^n$, indicative
of mostly long-range multi-particle correlations in momentum space. We also
present a comparison of our results with Au+Au collision data obtained at RHIC
at similar centralities, but higher $\sqrt{s_{NN}}$. |
| doi_str_mv | 10.48550/arxiv.2002.08701 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2002_08701</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2002_08701</sourcerecordid><originalsourceid>FETCH-arxiv_primary_2002_087013</originalsourceid><addsrcrecordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjAw0jOwMDcw5GSIDijKL8nPU8grzU1KLVJIyylNLilNLMnMzytWyMxTUIkpLiwqqS6Or_bzq61VUbBVMNIzUXBPDVNwLNV2LFVIzs_JySwGqy4uKU3JTE1RKM8syVDwcHRxDeZhYE1LzClO5YXS3Azybq4hzh66YGfEFxRl5iYWVcaDnBMPdo4xYRUAQjg-1g</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions studied with HADES</title><source>arXiv.org</source><creator>Adamczewski-Musch, J ; Arnold, O ; Behnke, C ; Belyaev, A ; Berger-Chen, J. C ; Biernat, J ; Blanco, A ; Blume, C ; Bordalo, P ; Chernenko, S ; Deveaux, C ; Dybczak, A ; Epple, E ; Fabbietti, L ; Fateev, O ; Filip, P ; Fonte, P ; Franco, C ; Friese, J ; Fr"ohlich, I ; Galatyuk, T ; Garzon, J. A ; Gernh"auser, R ; Greifenhagen, R ; Guber, F ; Gumberidze, M ; Harabasz, S ; Heinz, T ; Hennino, T ; Hlavac, S ; H"ohne, C ; Holzmann, R ; Ierusalimov, A ; Ivashkin, A ; K"ampfer, B ; Kardan, B ; Koenig, I ; Koenig, W ; Kolb, B. W ; Kotte, R ; Kunz, T ; Kurilkin, A ; Kurilkin, P ; Ladygin, V ; Lalik, R ; Lapidus, K ; Lebedev, A ; Lopes, L ; Lorenz, M ; Maier, L ; Mangiarotti, A ; Markert, J ; Maurus, S ; Michel, J ; Morozov, S ; M"untz, C ; M"unzer, R ; Naumann, L ; Nowakowski, K ; Palka, M ; Parpottas, Y ; Pechenov, V ; Pechenova, O ; Petukhov, O ; Piasecki, K ; Pietraszko, J ; Przygoda, W ; Ramos, S ; Ramstein, B ; Reshetin, A ; Rodriguez-Ramos, P ; Rosier, P ; Rost, A ; Rustamov, A ; Sadovsky, A ; Salabura, P ; Scheib, T ; Schuldes, H ; Scozzi, F ; Seck, F ; Sellheim, P ; Selyuzhenkov, I ; Siebenson, J ; Silva, L ; Sobolev, Yu. G ; Spataro, S ; Str"obele, H ; Stroth, J ; Strzempek, P ; Sturm, C ; Tlusty, P ; Traxler, M ; Tsertos, H ; Usenko, E ; Wagner, V ; Wendisch, C ; Wiebusch, M. G ; Wirth, J ; Zanevsky, Y ; Zumbruch, P</creator><creatorcontrib>Adamczewski-Musch, J ; Arnold, O ; Behnke, C ; Belyaev, A ; Berger-Chen, J. C ; Biernat, J ; Blanco, A ; Blume, C ; Bordalo, P ; Chernenko, S ; Deveaux, C ; Dybczak, A ; Epple, E ; Fabbietti, L ; Fateev, O ; Filip, P ; Fonte, P ; Franco, C ; Friese, J ; Fr"ohlich, I ; Galatyuk, T ; Garzon, J. A ; Gernh"auser, R ; Greifenhagen, R ; Guber, F ; Gumberidze, M ; Harabasz, S ; Heinz, T ; Hennino, T ; Hlavac, S ; H"ohne, C ; Holzmann, R ; Ierusalimov, A ; Ivashkin, A ; K"ampfer, B ; Kardan, B ; Koenig, I ; Koenig, W ; Kolb, B. W ; Kotte, R ; Kunz, T ; Kurilkin, A ; Kurilkin, P ; Ladygin, V ; Lalik, R ; Lapidus, K ; Lebedev, A ; Lopes, L ; Lorenz, M ; Maier, L ; Mangiarotti, A ; Markert, J ; Maurus, S ; Michel, J ; Morozov, S ; M"untz, C ; M"unzer, R ; Naumann, L ; Nowakowski, K ; Palka, M ; Parpottas, Y ; Pechenov, V ; Pechenova, O ; Petukhov, O ; Piasecki, K ; Pietraszko, J ; Przygoda, W ; Ramos, S ; Ramstein, B ; Reshetin, A ; Rodriguez-Ramos, P ; Rosier, P ; Rost, A ; Rustamov, A ; Sadovsky, A ; Salabura, P ; Scheib, T ; Schuldes, H ; Scozzi, F ; Seck, F ; Sellheim, P ; Selyuzhenkov, I ; Siebenson, J ; Silva, L ; Sobolev, Yu. G ; Spataro, S ; Str"obele, H ; Stroth, J ; Strzempek, P ; Sturm, C ; Tlusty, P ; Traxler, M ; Tsertos, H ; Usenko, E ; Wagner, V ; Wendisch, C ; Wiebusch, M. G ; Wirth, J ; Zanevsky, Y ; Zumbruch, P</creatorcontrib><description>Phys. Rev. C 102, 024914 (2020) We present an analysis of proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4
GeV Au+Au collisions measured with the High-Acceptance DiElectron Spectrometer
(HADES) at GSI. With the help of extensive detector simulations done with IQMD
transport model events including nuclear clusters, various nuisance effects
influencing the observed proton cumulants have been investigated. Acceptance
and efficiency corrections have been applied as a function of fine grained
rapidity and transverse momentum bins, as well as considering local track
density dependencies. Next, the effects of volume changes within particular
centrality selections have been considered and beyond-leading-order corrections
have been applied to the data. The efficiency and volume corrected proton
number moments and cumulants Kn of orders n = 1, . . . , 4 have been obtained
as a function of centrality and phase-space bin, as well as the corresponding
correlators C_n . We find that the observed correlators show a power-law
scaling with the mean number of protons, i.e. $C_n \propto ^n$, indicative
of mostly long-range multi-particle correlations in momentum space. We also
present a comparison of our results with Au+Au collision data obtained at RHIC
at similar centralities, but higher $\sqrt{s_{NN}}$.</description><identifier>DOI: 10.48550/arxiv.2002.08701</identifier><language>eng</language><subject>Physics - Nuclear Experiment</subject><creationdate>2020-02</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2002.08701$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.1103/PhysRevC.102.024914$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2002.08701$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Adamczewski-Musch, J</creatorcontrib><creatorcontrib>Arnold, O</creatorcontrib><creatorcontrib>Behnke, C</creatorcontrib><creatorcontrib>Belyaev, A</creatorcontrib><creatorcontrib>Berger-Chen, J. 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G</creatorcontrib><creatorcontrib>Spataro, S</creatorcontrib><creatorcontrib>Str"obele, H</creatorcontrib><creatorcontrib>Stroth, J</creatorcontrib><creatorcontrib>Strzempek, P</creatorcontrib><creatorcontrib>Sturm, C</creatorcontrib><creatorcontrib>Tlusty, P</creatorcontrib><creatorcontrib>Traxler, M</creatorcontrib><creatorcontrib>Tsertos, H</creatorcontrib><creatorcontrib>Usenko, E</creatorcontrib><creatorcontrib>Wagner, V</creatorcontrib><creatorcontrib>Wendisch, C</creatorcontrib><creatorcontrib>Wiebusch, M. G</creatorcontrib><creatorcontrib>Wirth, J</creatorcontrib><creatorcontrib>Zanevsky, Y</creatorcontrib><creatorcontrib>Zumbruch, P</creatorcontrib><title>Proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions studied with HADES</title><description>Phys. Rev. C 102, 024914 (2020) We present an analysis of proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4
GeV Au+Au collisions measured with the High-Acceptance DiElectron Spectrometer
(HADES) at GSI. With the help of extensive detector simulations done with IQMD
transport model events including nuclear clusters, various nuisance effects
influencing the observed proton cumulants have been investigated. Acceptance
and efficiency corrections have been applied as a function of fine grained
rapidity and transverse momentum bins, as well as considering local track
density dependencies. Next, the effects of volume changes within particular
centrality selections have been considered and beyond-leading-order corrections
have been applied to the data. The efficiency and volume corrected proton
number moments and cumulants Kn of orders n = 1, . . . , 4 have been obtained
as a function of centrality and phase-space bin, as well as the corresponding
correlators C_n . We find that the observed correlators show a power-law
scaling with the mean number of protons, i.e. $C_n \propto ^n$, indicative
of mostly long-range multi-particle correlations in momentum space. We also
present a comparison of our results with Au+Au collision data obtained at RHIC
at similar centralities, but higher $\sqrt{s_{NN}}$.</description><subject>Physics - Nuclear Experiment</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjAw0jOwMDcw5GSIDijKL8nPU8grzU1KLVJIyylNLilNLMnMzytWyMxTUIkpLiwqqS6Or_bzq61VUbBVMNIzUXBPDVNwLNV2LFVIzs_JySwGqy4uKU3JTE1RKM8syVDwcHRxDeZhYE1LzClO5YXS3Azybq4hzh66YGfEFxRl5iYWVcaDnBMPdo4xYRUAQjg-1g</recordid><startdate>20200220</startdate><enddate>20200220</enddate><creator>Adamczewski-Musch, J</creator><creator>Arnold, O</creator><creator>Behnke, C</creator><creator>Belyaev, A</creator><creator>Berger-Chen, J. 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C</creatorcontrib><creatorcontrib>Biernat, J</creatorcontrib><creatorcontrib>Blanco, A</creatorcontrib><creatorcontrib>Blume, C</creatorcontrib><creatorcontrib>Bordalo, P</creatorcontrib><creatorcontrib>Chernenko, S</creatorcontrib><creatorcontrib>Deveaux, C</creatorcontrib><creatorcontrib>Dybczak, A</creatorcontrib><creatorcontrib>Epple, E</creatorcontrib><creatorcontrib>Fabbietti, L</creatorcontrib><creatorcontrib>Fateev, O</creatorcontrib><creatorcontrib>Filip, P</creatorcontrib><creatorcontrib>Fonte, P</creatorcontrib><creatorcontrib>Franco, C</creatorcontrib><creatorcontrib>Friese, J</creatorcontrib><creatorcontrib>Fr"ohlich, I</creatorcontrib><creatorcontrib>Galatyuk, T</creatorcontrib><creatorcontrib>Garzon, J. A</creatorcontrib><creatorcontrib>Gernh"auser, R</creatorcontrib><creatorcontrib>Greifenhagen, R</creatorcontrib><creatorcontrib>Guber, F</creatorcontrib><creatorcontrib>Gumberidze, M</creatorcontrib><creatorcontrib>Harabasz, S</creatorcontrib><creatorcontrib>Heinz, T</creatorcontrib><creatorcontrib>Hennino, T</creatorcontrib><creatorcontrib>Hlavac, S</creatorcontrib><creatorcontrib>H"ohne, C</creatorcontrib><creatorcontrib>Holzmann, R</creatorcontrib><creatorcontrib>Ierusalimov, A</creatorcontrib><creatorcontrib>Ivashkin, A</creatorcontrib><creatorcontrib>K"ampfer, B</creatorcontrib><creatorcontrib>Kardan, B</creatorcontrib><creatorcontrib>Koenig, I</creatorcontrib><creatorcontrib>Koenig, W</creatorcontrib><creatorcontrib>Kolb, B. W</creatorcontrib><creatorcontrib>Kotte, R</creatorcontrib><creatorcontrib>Kunz, T</creatorcontrib><creatorcontrib>Kurilkin, A</creatorcontrib><creatorcontrib>Kurilkin, P</creatorcontrib><creatorcontrib>Ladygin, V</creatorcontrib><creatorcontrib>Lalik, R</creatorcontrib><creatorcontrib>Lapidus, K</creatorcontrib><creatorcontrib>Lebedev, A</creatorcontrib><creatorcontrib>Lopes, L</creatorcontrib><creatorcontrib>Lorenz, M</creatorcontrib><creatorcontrib>Maier, L</creatorcontrib><creatorcontrib>Mangiarotti, A</creatorcontrib><creatorcontrib>Markert, J</creatorcontrib><creatorcontrib>Maurus, S</creatorcontrib><creatorcontrib>Michel, J</creatorcontrib><creatorcontrib>Morozov, S</creatorcontrib><creatorcontrib>M"untz, C</creatorcontrib><creatorcontrib>M"unzer, R</creatorcontrib><creatorcontrib>Naumann, L</creatorcontrib><creatorcontrib>Nowakowski, K</creatorcontrib><creatorcontrib>Palka, M</creatorcontrib><creatorcontrib>Parpottas, Y</creatorcontrib><creatorcontrib>Pechenov, V</creatorcontrib><creatorcontrib>Pechenova, O</creatorcontrib><creatorcontrib>Petukhov, O</creatorcontrib><creatorcontrib>Piasecki, K</creatorcontrib><creatorcontrib>Pietraszko, J</creatorcontrib><creatorcontrib>Przygoda, W</creatorcontrib><creatorcontrib>Ramos, S</creatorcontrib><creatorcontrib>Ramstein, B</creatorcontrib><creatorcontrib>Reshetin, A</creatorcontrib><creatorcontrib>Rodriguez-Ramos, P</creatorcontrib><creatorcontrib>Rosier, P</creatorcontrib><creatorcontrib>Rost, A</creatorcontrib><creatorcontrib>Rustamov, A</creatorcontrib><creatorcontrib>Sadovsky, A</creatorcontrib><creatorcontrib>Salabura, P</creatorcontrib><creatorcontrib>Scheib, T</creatorcontrib><creatorcontrib>Schuldes, H</creatorcontrib><creatorcontrib>Scozzi, F</creatorcontrib><creatorcontrib>Seck, F</creatorcontrib><creatorcontrib>Sellheim, P</creatorcontrib><creatorcontrib>Selyuzhenkov, I</creatorcontrib><creatorcontrib>Siebenson, J</creatorcontrib><creatorcontrib>Silva, L</creatorcontrib><creatorcontrib>Sobolev, Yu. G</creatorcontrib><creatorcontrib>Spataro, S</creatorcontrib><creatorcontrib>Str"obele, H</creatorcontrib><creatorcontrib>Stroth, J</creatorcontrib><creatorcontrib>Strzempek, P</creatorcontrib><creatorcontrib>Sturm, C</creatorcontrib><creatorcontrib>Tlusty, P</creatorcontrib><creatorcontrib>Traxler, M</creatorcontrib><creatorcontrib>Tsertos, H</creatorcontrib><creatorcontrib>Usenko, E</creatorcontrib><creatorcontrib>Wagner, V</creatorcontrib><creatorcontrib>Wendisch, C</creatorcontrib><creatorcontrib>Wiebusch, M. G</creatorcontrib><creatorcontrib>Wirth, J</creatorcontrib><creatorcontrib>Zanevsky, Y</creatorcontrib><creatorcontrib>Zumbruch, P</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Adamczewski-Musch, J</au><au>Arnold, O</au><au>Behnke, C</au><au>Belyaev, A</au><au>Berger-Chen, J. C</au><au>Biernat, J</au><au>Blanco, A</au><au>Blume, C</au><au>Bordalo, P</au><au>Chernenko, S</au><au>Deveaux, C</au><au>Dybczak, A</au><au>Epple, E</au><au>Fabbietti, L</au><au>Fateev, O</au><au>Filip, P</au><au>Fonte, P</au><au>Franco, C</au><au>Friese, J</au><au>Fr"ohlich, I</au><au>Galatyuk, T</au><au>Garzon, J. A</au><au>Gernh"auser, R</au><au>Greifenhagen, R</au><au>Guber, F</au><au>Gumberidze, M</au><au>Harabasz, S</au><au>Heinz, T</au><au>Hennino, T</au><au>Hlavac, S</au><au>H"ohne, C</au><au>Holzmann, R</au><au>Ierusalimov, A</au><au>Ivashkin, A</au><au>K"ampfer, B</au><au>Kardan, B</au><au>Koenig, I</au><au>Koenig, W</au><au>Kolb, B. W</au><au>Kotte, R</au><au>Kunz, T</au><au>Kurilkin, A</au><au>Kurilkin, P</au><au>Ladygin, V</au><au>Lalik, R</au><au>Lapidus, K</au><au>Lebedev, A</au><au>Lopes, L</au><au>Lorenz, M</au><au>Maier, L</au><au>Mangiarotti, A</au><au>Markert, J</au><au>Maurus, S</au><au>Michel, J</au><au>Morozov, S</au><au>M"untz, C</au><au>M"unzer, R</au><au>Naumann, L</au><au>Nowakowski, K</au><au>Palka, M</au><au>Parpottas, Y</au><au>Pechenov, V</au><au>Pechenova, O</au><au>Petukhov, O</au><au>Piasecki, K</au><au>Pietraszko, J</au><au>Przygoda, W</au><au>Ramos, S</au><au>Ramstein, B</au><au>Reshetin, A</au><au>Rodriguez-Ramos, P</au><au>Rosier, P</au><au>Rost, A</au><au>Rustamov, A</au><au>Sadovsky, A</au><au>Salabura, P</au><au>Scheib, T</au><au>Schuldes, H</au><au>Scozzi, F</au><au>Seck, F</au><au>Sellheim, P</au><au>Selyuzhenkov, I</au><au>Siebenson, J</au><au>Silva, L</au><au>Sobolev, Yu. G</au><au>Spataro, S</au><au>Str"obele, H</au><au>Stroth, J</au><au>Strzempek, P</au><au>Sturm, C</au><au>Tlusty, P</au><au>Traxler, M</au><au>Tsertos, H</au><au>Usenko, E</au><au>Wagner, V</au><au>Wendisch, C</au><au>Wiebusch, M. G</au><au>Wirth, J</au><au>Zanevsky, Y</au><au>Zumbruch, P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions studied with HADES</atitle><date>2020-02-20</date><risdate>2020</risdate><abstract>Phys. Rev. C 102, 024914 (2020) We present an analysis of proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4
GeV Au+Au collisions measured with the High-Acceptance DiElectron Spectrometer
(HADES) at GSI. With the help of extensive detector simulations done with IQMD
transport model events including nuclear clusters, various nuisance effects
influencing the observed proton cumulants have been investigated. Acceptance
and efficiency corrections have been applied as a function of fine grained
rapidity and transverse momentum bins, as well as considering local track
density dependencies. Next, the effects of volume changes within particular
centrality selections have been considered and beyond-leading-order corrections
have been applied to the data. The efficiency and volume corrected proton
number moments and cumulants Kn of orders n = 1, . . . , 4 have been obtained
as a function of centrality and phase-space bin, as well as the corresponding
correlators C_n . We find that the observed correlators show a power-law
scaling with the mean number of protons, i.e. $C_n \propto ^n$, indicative
of mostly long-range multi-particle correlations in momentum space. We also
present a comparison of our results with Au+Au collision data obtained at RHIC
at similar centralities, but higher $\sqrt{s_{NN}}$.</abstract><doi>10.48550/arxiv.2002.08701</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2002.08701 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2002_08701 |
| source | arXiv.org |
| subjects | Physics - Nuclear Experiment |
| title | Proton number fluctuations in $\sqrt{s_{NN}}$ = 2.4 GeV Au+Au collisions studied with HADES |
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