429 research outputs found

    The Effect of Quantum Fluctuations in Compact Star Observables

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    Astrophysical measurements regarding compact stars are just ahead of a big evolution jump, since the NICER experiment deployed on ISS on 14 June 2017. This will soon provide data that would enable the determination of compact star radius with less than 10% error. This poses new challenges for nuclear models aiming to explain the structure of super dense nuclear matter found in neutron stars. Detailed studies of the QCD phase diagram shows the importance of bosonic quantum fluctuations in the cold dense matter equation of state. Here, we using a demonstrative model to show the effect of bosonic quantum fluctuations on compact star observables such as mass, radius, and compactness. We have also calculated the difference in the value of compressibility which is caused by quantum fluctuations. The above mentioned quantities are calculated in mean field, one-loop and in high order many-loop approximation. The results show that the magnitude of these effects is ~5%, which place it into the region where forthcoming high-accuracy measurements may detect it.Comment: 6 pages 4 figues, minor corrections were adde

    Nuclear effects in dAu collisions from recent RHIC data

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    Neutral pion (pi(0)) production is calculated in a leading order (LO) perturbative QCD-based model in pp and dAu collisions at root s = 200 AGeV at midrapidity. The model includes transverse component of the initial parton distribution. We compare our results for pp collision to experimental data at RHIC energy. We repeat our calculation for the dAu collision and investigate the interplay between shadowing and multiple scattering. In central dAu collisions the influence of possible jet energy loss in cold nuclear matter in discussed and numerical results are presented

    Application of the non-extensive statistical approach to high energy particle collisions

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    In high-energy collisions the number of the created particles is far less than the thermodynamic limit, especially in small colliding systems (e.g. proton-proton). Therefore final-state effects and fluctuations in the one-particle energy distribution are appreciable. As a consequence the characterization of identified hadron spectra with the Boltzmann\,--\,Gibbs thermodynamical approach is insufficient. Instead particle spectra measured in high-energy collisions can be described very well with Tsallis\,--\,Pareto distributions, derived from non-extensive thermodynamics. Using the Tsallis q-entropy formula, a generalization of the Boltzmann\,--\,Gibbs entropy, we interpret the microscopical physics by analysing the Tsallis qq and TT parameters. In this paper we give a quick overview on these parameters, analyzing identified hadron spectra from recent years in a wide center of mass energy range. We demonstrate that the fitted Tsallis-parameters show dependency on this energy and on the particle species. Our findings are described well by a QCD inspired evolution ansatz

    Where does the energy loss lose strength?

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    Nuclear modification factors for pion production in AuAu and CuCu collisions are analyzed at very high transverse momenta. At p(T) greater than or similar to 10 GeV/c, the RAA(pT) is determined mostly by the initial-state nuclear modifications (e. g. the EMC effect) and the non-Abelian jet energy loss in the final state. At high momenta these effects together are strong enough to suppress RAA(p(T)) to below 1 at RHIC energies. We display results using HKN shadowing in our pQCD-improved parton model. Result of a similar calculation at LHC energies for PbPb collisions is also displayed. Based on dN/dy estimates, a larger opacity value, L/lambda(g) approximate to 10 +/- 2, is used for the produced partonic matter in central collisions at the LHC

    Systematic analysis of the non-extensive statistical approach in high energy particle collisions-experiment vs. theory

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    The analysis of high-energy particle collisions is an excellent testbed for the non-extensive statistical approach. In these reactions we are far from the thermodynamical limit. In small colliding systems, such as electron-positron or nuclear collisions, the number of particles is several orders of magnitude smaller than the Avogadro number; therefore, finite-size and fluctuation effects strongly influence the final-state one-particle energy distributions. Due to the simple characterization, the description of the identified hadron spectra with the Boltzmann-Gibbs thermodynamical approach is insufficient. These spectra can be described very well with Tsallis-Pareto distributions instead, derived from non-extensive thermodynamics. Using the qq-entropy formula, we interpret the microscopic physics in terms of the Tsallis qq and TT parameters. In this paper we give a view on these parameters, analyzing identified hadron spectra from recent years in a wide center-of-mass energy range. We demonstrate that the fitted Tsallis-parameters show dependency on the center-of-mass energy and particle species (mass). Our findings are described well by a QCD (Quantum Chromodynamics) inspired parton evolution ansatz. Based on this comprehensive study, apart from the evolution, both mesonic and baryonic components found to be non-extensive (q>1q>1), besides the mass ordered hierarchy observed in the parameter TT. We also study and compare in details the theory-obtained parameters for the case of PYTHIA8 Monte Carlo Generator, perturbative QCD and quark coalescence models.Comment: 21 pages, 12 figures. This is an extended version of our paper at the 36th International Workshop on Bayesian Inference and Maximum Entropy Methods in Science and Engineering (MaxEnt 2016), 10-15 July 2016, Ghent, Belgiu

    High pT pion and kaon production in relativistic nuclear collisions

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    High-p(T) pion and kaon production is studied in relativistic proton-proton, proton-nucleus, and nucleus-nucleus collisions in a wide energy range. Cross sections are calculated based on perturbative QCD, augmented by a phenomenological transverse- momentum distribution of partons ("intrinsic k(T)"). An energy dependent width of the transverse-momentum distribution is extracted from pion and charged hadron production data in proton-proton/proton-antiproton collisions. Effects of multiscattering and shadowing in the strongly interacting medium are taken into account. Enhancement of the transverse-momentum width is introduced and parameterized to explain the Cronin effect. In collisions between heavy nuclei, the model overpredicts central pion production cross sections (more significantly at higher energies), hinting at the presence of jet quenching. Predictions are made for proton-nucleus and nucleus-nucleus collisions at relativistic heavy ion collider energies

    Does the Cronin Peak Disappear at LHC Energies

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    In this work we compare the nuclear modification factors in proton (deuteron) - nucleus collisions at CERN SPS, FNAL and RHIC energies in a wide PT range. In these experiments the nuclear modification factor has shown an enhancement at p(T) approximate to 4 GeV/c. The height of this "Cronin peak" depends on the c.m. energy of the collision, as it is subject to stronger shadowing at higher energies. One of the aims of this contribution is to analyze the shadowing phenomenon at lower (2GeV/c less than or similar to p(T) less than or similar to 4 GeV/c) and intermediate (4 GeV/c less than or similar to p(T) less than or similar to 8 GeV/c) transverse momentum. Different shadowing parametrizations are considered and the obtained Cronin peaks are investigated at RHIC and LHC energies
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