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  1. Article ; Online: Scaling of charged particle production and centrality determination in p-Pb collisions at √sNN = 5.02 TeV at ALICE

    Oppedisano C.

    EPJ Web of Conferences, Vol 95, p

    2015  Volume 04047

    Abstract: Proton-nucleus collisions are studied in order to disentangle initial state effects, already present in cold nuclear matter, from final state effects, that are associated to the hot and strongly interacting medium created in A-A collisions. However, ... ...

    Abstract Proton-nucleus collisions are studied in order to disentangle initial state effects, already present in cold nuclear matter, from final state effects, that are associated to the hot and strongly interacting medium created in A-A collisions. However, after the 2013 p-Pb data taking at LHC, the importance of p-A collisions on their own has been acknowledged. Several measurements clearly showed that p-A collisions cannot simply be explained by an incoherent superposition of proton-nucleon collisions, but indicate the presence of coherent and collective effects, with a strong dependence on the collision geometry. These measurements pointed out the need for a detailed characterization of the collision geometry. Typically, parameters such as the number of binary collisions Ncoll or the number of participating nucleons Npart are used to characterize the centrality. In nucleus-nucleus interactions the centrality is usually estimated by measuring the charged particle multiplicity. However, in contrast to A-A, in p-A collisions the large fluctuations in a much reduced multiplicity environment generate a dynamical bias in centrality classes based on particle multiplicity measurement. The centrality determination is critically addressed and a different approach to extract the average Ncoll values, needed to compare p-A to pp data, is presented. The centrality dependence of primary charged-particle production and of transverse momentum distributions in p-A collisions at √sNN = 5.02 TeV measured by ALICE are presented.
    Keywords Science ; Q ; Physics ; QC1-999
    Subject code 530
    Language English
    Publishing date 2015-01-01T00:00:00Z
    Publisher EDP Sciences
    Document type Article ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  2. Article ; Online: Scaling of charged particle production and centrality determination in p-Pb collisions at √sNN = 5.02 TeV at ALICE

    Oppedisano C.

    EPJ Web of Conferences, Vol 95, p

    2015  Volume 04047

    Abstract: Proton-nucleus collisions are studied in order to disentangle initial state effects, already present in cold nuclear matter, from final state effects, that are associated to the hot and strongly interacting medium created in A-A collisions. However, ... ...

    Abstract Proton-nucleus collisions are studied in order to disentangle initial state effects, already present in cold nuclear matter, from final state effects, that are associated to the hot and strongly interacting medium created in A-A collisions. However, after the 2013 p-Pb data taking at LHC, the importance of p-A collisions on their own has been acknowledged. Several measurements clearly showed that p-A collisions cannot simply be explained by an incoherent superposition of proton-nucleon collisions, but indicate the presence of coherent and collective effects, with a strong dependence on the collision geometry. These measurements pointed out the need for a detailed characterization of the collision geometry. Typically, parameters such as the number of binary collisions Ncoll or the number of participating nucleons Npart are used to characterize the centrality. In nucleus-nucleus interactions the centrality is usually estimated by measuring the charged particle multiplicity. However, in contrast to A-A, in p-A collisions the large fluctuations in a much reduced multiplicity environment generate a dynamical bias in centrality classes based on particle multiplicity measurement. The centrality determination is critically addressed and a different approach to extract the average Ncoll values, needed to compare p-A to pp data, is presented. The centrality dependence of primary charged-particle production and of transverse momentum distributions in p-A collisions at √sNN = 5.02 TeV measured by ALICE are presented.
    Keywords Science ; Q ; Physics ; QC1-999
    Subject code 530
    Language English
    Publishing date 2015-01-01T00:00:00Z
    Publisher EDP Sciences
    Document type Article ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  3. Article ; Online: X-ray polarization evidence for a 200-year-old flare of Sgr A

    Marin, Frédéric / Churazov, Eugene / Khabibullin, Ildar / Ferrazzoli, Riccardo / Di Gesu, Laura / Barnouin, Thibault / Di Marco, Alessandro / Middei, Riccardo / Vikhlinin, Alexey / Costa, Enrico / Soffitta, Paolo / Muleri, Fabio / Sunyaev, Rashid / Forman, William / Kraft, Ralph / Bianchi, Stefano / Donnarumma, Immacolata / Petrucci, Pierre-Olivier / Enoto, Teruaki /
    Agudo, Iván / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Chen, Chien-Ting / Ciprini, Stefano / De Rosa, Alessandra / Del Monte, Ettore / Di Lalla, Niccolò / Doroshenko, Victor / Dovčiak, Michal / Ehlert, Steven R / Evangelista, Yuri / Fabiani, Sergio / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Ingram, Adam / Iwakiri, Wataru / Jorstad, Svetlana G / Kaaret, Philip / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / Krawczynski, Henric / La Monaca, Fabio / Latronico, Luca / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Massaro, Francesco / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Negro, Michela / Ng, C-Y / O'Dell, Stephen L / Omodei, Nicola / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Rankin, John / Ratheesh, Ajay / Roberts, Oliver J / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Spandre, Gloria / Swartz, Doug / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicholas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey S / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Nature

    2023  Volume 619, Issue 7968, Page(s) 41–45

    Abstract: The centre of the Milky Way Galaxy hosts a black hole with a solar mass of about 4 million (Sagittarius ... ...

    Abstract The centre of the Milky Way Galaxy hosts a black hole with a solar mass of about 4 million (Sagittarius A
    Language English
    Publishing date 2023-06-21
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-023-06064-x
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  4. Article ; Online: Vela pulsar wind nebula X-rays are polarized to near the synchrotron limit.

    Xie, Fei / Di Marco, Alessandro / La Monaca, Fabio / Liu, Kuan / Muleri, Fabio / Bucciantini, Niccolò / Romani, Roger W / Costa, Enrico / Rankin, John / Soffitta, Paolo / Bachetti, Matteo / Di Lalla, Niccolò / Fabiani, Sergio / Ferrazzoli, Riccardo / Gunji, Shuichi / Latronico, Luca / Negro, Michela / Omodei, Nicola / Pilia, Maura /
    Trois, Alessio / Watanabe, Eri / Agudo, Iván / Antonelli, Lucio A / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Donnarumma, Immacolata / Doroshenko, Victor / Dovčiak, Michal / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Garcia, Javier A / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / Krawczynski, Henric / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marin, Frédéric / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Massaro, Francesco / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Ng, C-Y / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Petrucci, Pierre-Olivier / Possenti, Andrea / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Ratheesh, Ajay / Sgró, Carmelo / Slane, Patrick / Spandre, Gloria / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicolas E / Tombesi, Francesco / Tsygankov, Sergey S / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Zane, Silvia

    Nature

    2022  Volume 612, Issue 7941, Page(s) 658–660

    Abstract: Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years) ...

    Abstract Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar wind nebula is powered by a young pulsar (B0833-45, aged 11,000 years)
    Language English
    Publishing date 2022-12-21
    Publishing country England
    Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-022-05476-5
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  5. Article ; Online: Polarized x-rays from a magnetar.

    Taverna, Roberto / Turolla, Roberto / Muleri, Fabio / Heyl, Jeremy / Zane, Silvia / Baldini, Luca / González-Caniulef, Denis / Bachetti, Matteo / Rankin, John / Caiazzo, Ilaria / Di Lalla, Niccolò / Doroshenko, Victor / Errando, Manel / Gau, Ephraim / Kırmızıbayrak, Demet / Krawczynski, Henric / Negro, Michela / Ng, Mason / Omodei, Nicola /
    Possenti, Andrea / Tamagawa, Toru / Uchiyama, Keisuke / Weisskopf, Martin C / Agudo, Ivan / Antonelli, Lucio A / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Capitanio, Fiamma / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Di Marco, Alessandro / Donnarumma, Immacolata / Dovčiak, Michal / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Fabiani, Sergio / Ferrazzoli, Riccardo / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / La Monaca, Fabio / Latronico, Luca / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marin, Frédéric / Marinucci, Andrea / Marscher, Alan P / Marshall, Herman L / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Ng, Stephen C-Y / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Poutanen, Juri / Puccetti, Simonetta / Ramsey, Brian D / Ratheesh, Ajay / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Soffitta, Paolo / Spandre, Gloria / Tavecchio, Fabrizio / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicholas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey S / Vink, Jacco / Wu, Kinwah / Xie, Fei

    Science (New York, N.Y.)

    2022  Volume 378, Issue 6620, Page(s) 646–650

    Abstract: Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 ... ...

    Abstract Magnetars are neutron stars with ultrastrong magnetic fields, which can be observed in x-rays. Polarization measurements could provide information on their magnetic fields and surface properties. We observed polarized x-rays from the magnetar 4U 0142+61 using the Imaging X-ray Polarimetry Explorer and found a linear polarization degree of 13.5 ± 0.8% averaged over the 2- to 8-kilo-electron volt band. The polarization changes with energy: The degree is 15.0 ± 1.0% at 2 to 4 kilo-electron volts, drops below the instrumental sensitivity ~4 to 5 kilo-electron volts, and rises to 35.2 ± 7.1% at 5.5 to 8 kilo-electron volts. The polarization angle also changes by 90° at ~4 to 5 kilo-electron volts. These results are consistent with a model in which thermal radiation from the magnetar surface is reprocessed by scattering off charged particles in the magnetosphere.
    Language English
    Publishing date 2022-11-03
    Publishing country United States
    Document type Journal Article ; Research Support, Non-U.S. Gov't ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.add0080
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  6. Article ; Online: Polarized blazar X-rays imply particle acceleration in shocks.

    Liodakis, Ioannis / Marscher, Alan P / Agudo, Iván / Berdyugin, Andrei V / Bernardos, Maria I / Bonnoli, Giacomo / Borman, George A / Casadio, Carolina / Casanova, Vı Ctor / Cavazzuti, Elisabetta / Rodriguez Cavero, Nicole / Di Gesu, Laura / Di Lalla, Niccoló / Donnarumma, Immacolata / Ehlert, Steven R / Errando, Manel / Escudero, Juan / Garcı A-Comas, Maya / Agı S-González, Beatriz /
    Husillos, César / Jormanainen, Jenni / Jorstad, Svetlana G / Kagitani, Masato / Kopatskaya, Evgenia N / Kravtsov, Vadim / Krawczynski, Henric / Lindfors, Elina / Larionova, Elena G / Madejski, Grzegorz M / Marin, Frédéric / Marchini, Alessandro / Marshall, Herman L / Morozova, Daria A / Massaro, Francesco / Masiero, Joseph R / Mawet, Dimitri / Middei, Riccardo / Millar-Blanchaer, Maxwell A / Myserlis, Ioannis / Negro, Michela / Nilsson, Kari / O'Dell, Stephen L / Omodei, Nicola / Pacciani, Luigi / Paggi, Alessandro / Panopoulou, Georgia V / Peirson, Abel L / Perri, Matteo / Petrucci, Pierre-Olivier / Poutanen, Juri / Puccetti, Simonetta / Romani, Roger W / Sakanoi, Takeshi / Savchenko, Sergey S / Sota, Alfredo / Tavecchio, Fabrizio / Tinyanont, Samaporn / Vasilyev, Andrey A / Weaver, Zachary R / Zhovtan, Alexey V / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bianchi, Stefano / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccoló / Capitanio, Fiamma / Castellano, Simone / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Marco, Alessandro / Doroshenko, Victor / Dovčiak, Michal / Enoto, Teruaki / Evangelista, Yuri / Fabiani, Sergio / Ferrazzoli, Riccardo / Garcia, Javier A / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Karas, Vladimir / Kitaguchi, Takao / Kolodziejczak, Jeffery J / La Monaca, Fabio / Latronico, Luca / Maldera, Simone / Manfreda, Alberto / Marinucci, Andrea / Matt, Giorgio / Mitsuishi, Ikuyuki / Mizuno, Tsunefumi / Muleri, Fabio / Ng, Stephen C-Y / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Ramsey, Brian D / Rankin, John / Ratheesh, Ajay / Sgró, Carmelo / Slane, Patrick / Soffitta, Paolo / Spandre, Gloria / Tamagawa, Toru / Taverna, Roberto / Tawara, Yuzuru / Tennant, Allyn F / Thomas, Nicolas E / Tombesi, Francesco / Trois, Alessio / Tsygankov, Sergey / Turolla, Roberto / Vink, Jacco / Weisskopf, Martin C / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Nature

    2022  Volume 611, Issue 7937, Page(s) 677–681

    Abstract: Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a ... ...

    Abstract Most of the light from blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of sight, is produced by high-energy particles, up to around 1 TeV. Although the jets are known to be ultimately powered by a supermassive black hole, how the particles are accelerated to such high energies has been an unanswered question. The process must be related to the magnetic field, which can be probed by observations of the polarization of light from the jets. Measurements of the radio to optical polarization-the only range available until now-probe extended regions of the jet containing particles that left the acceleration site days to years earlier
    Language English
    Publishing date 2022-11-23
    Publishing country England
    Document type Journal Article
    ZDB-ID 120714-3
    ISSN 1476-4687 ; 0028-0836
    ISSN (online) 1476-4687
    ISSN 0028-0836
    DOI 10.1038/s41586-022-05338-0
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  7. Article ; Online: Polarized x-rays constrain the disk-jet geometry in the black hole x-ray binary Cygnus X-1.

    Krawczynski, Henric / Muleri, Fabio / Dovčiak, Michal / Veledina, Alexandra / Rodriguez Cavero, Nicole / Svoboda, Jiri / Ingram, Adam / Matt, Giorgio / Garcia, Javier A / Loktev, Vladislav / Negro, Michela / Poutanen, Juri / Kitaguchi, Takao / Podgorný, Jakub / Rankin, John / Zhang, Wenda / Berdyugin, Andrei / Berdyugina, Svetlana V / Bianchi, Stefano /
    Blinov, Dmitry / Capitanio, Fiamma / Di Lalla, Niccolò / Draghis, Paul / Fabiani, Sergio / Kagitani, Masato / Kravtsov, Vadim / Kiehlmann, Sebastian / Latronico, Luca / Lutovinov, Alexander A / Mandarakas, Nikos / Marin, Frédéric / Marinucci, Andrea / Miller, Jon M / Mizuno, Tsunefumi / Molkov, Sergey V / Omodei, Nicola / Petrucci, Pierre-Olivier / Ratheesh, Ajay / Sakanoi, Takeshi / Semena, Andrei N / Skalidis, Raphael / Soffitta, Paolo / Tennant, Allyn F / Thalhammer, Phillipp / Tombesi, Francesco / Weisskopf, Martin C / Wilms, Joern / Zhang, Sixuan / Agudo, Iván / Antonelli, Lucio A / Bachetti, Matteo / Baldini, Luca / Baumgartner, Wayne H / Bellazzini, Ronaldo / Bongiorno, Stephen D / Bonino, Raffaella / Brez, Alessandro / Bucciantini, Niccolò / Castellano, Simone / Cavazzuti, Elisabetta / Ciprini, Stefano / Costa, Enrico / De Rosa, Alessandra / Del Monte, Ettore / Di Gesu, Laura / Di Marco, Alessandro / Donnarumma, Immacolata / Doroshenko, Victor / Ehlert, Steven R / Enoto, Teruaki / Evangelista, Yuri / Ferrazzoli, Riccardo / Gunji, Shuichi / Hayashida, Kiyoshi / Heyl, Jeremy / Iwakiri, Wataru / Jorstad, Svetlana G / Karas, Vladimir / Kolodziejczak, Jeffery J / La Monaca, Fabio / Liodakis, Ioannis / Maldera, Simone / Manfreda, Alberto / Marscher, Alan P / Marshall, Herman L / Mitsuishi, Ikuyuki / Ng, Chi-Yung / O'Dell, Stephen L / Oppedisano, Chiara / Papitto, Alessandro / Pavlov, George G / Peirson, Abel L / Perri, Matteo / Pesce-Rollins, Melissa / Pilia, Maura / Possenti, Andrea / Puccetti, Simonetta / Ramsey, Brian D / Romani, Roger W / Sgrò, Carmelo / Slane, Patrick / Spandre, Gloria / Tamagawa, Toru / Tavecchio, Fabrizio / Taverna, Roberto / Tawara, Yuzuru / Thomas, Nicholas E / Trois, Alessio / Tsygankov, Sergey / Turolla, Roberto / Vink, Jacco / Wu, Kinwah / Xie, Fei / Zane, Silvia

    Science (New York, N.Y.)

    2022  Volume 378, Issue 6620, Page(s) 650–654

    Abstract: A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray ... ...

    Abstract A black hole x-ray binary (XRB) system forms when gas is stripped from a normal star and accretes onto a black hole, which heats the gas sufficiently to emit x-rays. We report a polarimetric observation of the XRB Cygnus X-1 using the Imaging X-ray Polarimetry Explorer. The electric field position angle aligns with the outflowing jet, indicating that the jet is launched from the inner x-ray-emitting region. The polarization degree is 4.01 ± 0.20% at 2 to 8 kiloelectronvolts, implying that the accretion disk is viewed closer to edge-on than the binary orbit. These observations reveal that hot x-ray-emitting plasma is spatially extended in a plane perpendicular to, not parallel to, the jet axis.
    Language English
    Publishing date 2022-11-03
    Publishing country United States
    Document type Journal Article ; Research Support, U.S. Gov't, Non-P.H.S.
    ZDB-ID 128410-1
    ISSN 1095-9203 ; 0036-8075
    ISSN (online) 1095-9203
    ISSN 0036-8075
    DOI 10.1126/science.add5399
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  8. Article: First results on angular distributions of thermal dileptons in nuclear collisions.

    Arnaldi, R / Banicz, K / Castor, J / Chaurand, B / Cicalò, C / Colla, A / Cortese, P / Damjanovic, S / David, A / de Falco, A / Devaux, A / Ducroux, L / En'yo, H / Fargeix, J / Ferretti, A / Floris, M / Förster, A / Force, P / Guettet, N /
    Guichard, A / Gulkanian, H / Heuser, J M / Keil, M / Kluberg, L / Lourenço, C / Lozano, J / Manso, F / Martins, P / Masoni, A / Neves, A / Ohnishi, H / Oppedisano, C / Parracho, P / Pillot, P / Poghosyan, T / Puddu, G / Radermacher, E / Ramalhete, P / Rosinsky, P / Scomparin, E / Seixas, J / Serci, S / Shahoyan, R / Sonderegger, P / Specht, H J / Tieulent, R / Usai, G / Veenhof, R / Wöhri, H K

    Physical review letters

    2009  Volume 102, Issue 22, Page(s) 222301

    Abstract: The NA60 experiment at the CERN Super Proton Synchrotron has studied dimuon production in 158A GeV In-In collisions. The strong excess of pairs above the known sources found in the complete mass region 0.2

    Abstract The NA60 experiment at the CERN Super Proton Synchrotron has studied dimuon production in 158A GeV In-In collisions. The strong excess of pairs above the known sources found in the complete mass region 0.2<M<2.6 GeV has previously been interpreted as thermal radiation. We now present first results on the associated angular distributions. Using the Collins-Soper reference frame, the structure function parameters lambda, mu, and nu are measured to be zero, and the projected distributions in polar and azimuth angles are found to be uniform. The absence of any polarization is consistent with the interpretation of the excess dimuons as thermal radiation from a randomized system.<br />
    Language English
    Publishing date 2009-06-05
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.102.222301
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  9. Article: Evidence for radial flow of thermal dileptons in high-energy nuclear collisions.

    Arnaldi, R / Banicz, K / Castor, J / Chaurand, B / Cicalò, C / Colla, A / Cortese, P / Damjanovic, S / David, A / de Falco, A / Devaux, A / Ducroux, L / En'yo, H / Fargeix, J / Ferretti, A / Floris, M / Förster, A / Force, P / Guettet, N /
    Guichard, A / Gulkanian, H / Heuser, J M / Keil, M / Kluberg, L / Lourenço, C / Lozano, J / Manso, F / Martins, P / Masoni, A / Neves, A / Ohnishi, H / Oppedisano, C / Parracho, P / Pillot, P / Poghosyan, T / Puddu, G / Radermacher, E / Ramalhete, P / Rosinsky, P / Scomparin, E / Seixas, J / Serci, S / Shahoyan, R / Sonderegger, P / Specht, H J / Tieulent, R / Usai, G / Veenhof, R / Wöhri, H K

    Physical review letters

    2008  Volume 100, Issue 2, Page(s) 22302

    Abstract: The NA60 experiment at the CERN SPS has studied low-mass dimuon production in 158A GeV In-In collisions. An excess of pairs above the known meson decays has been reported before. We now present precision results on the associated transverse momentum ... ...

    Abstract The NA60 experiment at the CERN SPS has studied low-mass dimuon production in 158A GeV In-In collisions. An excess of pairs above the known meson decays has been reported before. We now present precision results on the associated transverse momentum spectra. The slope parameter Teff extracted from the spectra rises with dimuon mass up to the rho, followed by a sudden decline above. While the initial rise is consistent with the expectations for radial flow of a hadronic decay source, the decline signals a transition to an emission source with much smaller flow. This may well represent the first direct evidence for thermal radiation of partonic origin in nuclear collisions.
    Language English
    Publishing date 2008-01-18
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.100.022302
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  10. Article: J/psi production in Indium-Indium collisions at 158 GeV/nucleon.

    Arnaldi, R / Banicz, K / Castor, J / Chaurand, B / Cicalò, C / Colla, A / Cortese, P / Damjanovic, S / David, A / de Falco, A / Devaux, A / Ducroux, L / En'yo, H / Fargeix, J / Ferretti, A / Floris, M / Förster, A / Force, P / Guettet, N /
    Guichard, A / Gulkanian, H / Heuser, J M / Keil, M / Kluberg, L / Lourenço, C / Lozano, J / Manso, F / Martins, P / Masoni, A / Neves, A / Ohnishi, H / Oppedisano, C / Parracho, P / Pillot, P / Poghosyan, T / Puddu, G / Radermacher, E / Ramalhete, P / Rosinsky, P / Scomparin, E / Seixas, J / Serci, S / Shahoyan, R / Sonderegger, P / Specht, H J / Tieulent, R / Usai, G / Veenhof, R / Wöhri, H K

    Physical review letters

    2007  Volume 99, Issue 13, Page(s) 132302

    Abstract: The NA60 experiment studies muon pair production at the CERN Super Proton Synchrotron. In this Letter we report on a precision measurement of J/psi in In-In collisions. We have studied the J/psi centrality distribution, and we have compared it with the ... ...

    Abstract The NA60 experiment studies muon pair production at the CERN Super Proton Synchrotron. In this Letter we report on a precision measurement of J/psi in In-In collisions. We have studied the J/psi centrality distribution, and we have compared it with the one expected if absorption in cold nuclear matter were the only active suppression mechanism. For collisions involving more than approximately 80 participant nucleons, we find that an extra suppression is present. This result is in qualitative agreement with previous Pb-Pb measurements by the NA50 experiment, but no theoretical explanation is presently able to coherently describe both results.
    Language English
    Publishing date 2007-09-28
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.99.132302
    Database MEDical Literature Analysis and Retrieval System OnLINE

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