K/π fluctuations at relativistic energies

B.I. Abelev; R.J.M. Snellings; M. van Leeuwen; M.J. Russcher; T. Peitzmann; A. Mischke; F. Benedosso; E Braidot; M.A.J. Botje

K/π fluctuations at relativistic energies

Translated title of the contribution: K/π fluctuations at relativistic energies

B.I. Abelev, R.J.M. Snellings, M. van Leeuwen, M.J. Russcher, T. Peitzmann, A. Mischke, F. Benedosso, E Braidot, M.A.J. Botje

Medical Physics Group

Research output: Contribution to journal › Article › Academic › peer-review

Abstract

We report K/π fluctuations from Au+Au collisions at √sNN=19.6, 62.4, 130, and 200 GeV using the STAR detector at the Relativistic Heavy Ion Collider. K/π fluctuations in central collisions show little dependence on incident energy and are on the same order as those from NA49 at the Super Proton Synchrotron in central Pb+Pb collisions at √sNN=12.3 and 17.3 GeV. We report results for the collision centrality dependence of K/π fluctuations and results for charge-separated fluctuations. We observe that the K/π fluctuations scale with the charged particle multiplicity density.

Translated title of the contribution	K/π fluctuations at relativistic energies
Original language	Undefined/Unknown
Pages (from-to)	092301/1-092301/6
Number of pages	6
Journal	Physical review letters
Volume	103
Issue number	9
Publication status	Published - 2009

Cite this

@article{518e9d1836fc4291a0640f4e005bae6f,

title = "K/π fluctuations at relativistic energies",

abstract = "We report K/π fluctuations from Au+Au collisions at √sNN=19.6, 62.4, 130, and 200 GeV using the STAR detector at the Relativistic Heavy Ion Collider. K/π fluctuations in central collisions show little dependence on incident energy and are on the same order as those from NA49 at the Super Proton Synchrotron in central Pb+Pb collisions at √sNN=12.3 and 17.3 GeV. We report results for the collision centrality dependence of K/π fluctuations and results for charge-separated fluctuations. We observe that the K/π fluctuations scale with the charged particle multiplicity density.",

author = "B.I. Abelev and R.J.M. Snellings and {van Leeuwen}, M. and M.J. Russcher and T. Peitzmann and A. Mischke and F. Benedosso and E Braidot and M.A.J. Botje",

year = "2009",

language = "Undefined/Unknown",

volume = "103",

pages = "092301/1--092301/6",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "9",

}

TY - JOUR

T1 - K/π fluctuations at relativistic energies

AU - Abelev, B.I.

AU - Snellings, R.J.M.

AU - van Leeuwen, M.

AU - Russcher, M.J.

AU - Peitzmann, T.

AU - Mischke, A.

AU - Benedosso, F.

AU - Braidot, E

AU - Botje, M.A.J.

PY - 2009

Y1 - 2009

N2 - We report K/π fluctuations from Au+Au collisions at √sNN=19.6, 62.4, 130, and 200 GeV using the STAR detector at the Relativistic Heavy Ion Collider. K/π fluctuations in central collisions show little dependence on incident energy and are on the same order as those from NA49 at the Super Proton Synchrotron in central Pb+Pb collisions at √sNN=12.3 and 17.3 GeV. We report results for the collision centrality dependence of K/π fluctuations and results for charge-separated fluctuations. We observe that the K/π fluctuations scale with the charged particle multiplicity density.

AB - We report K/π fluctuations from Au+Au collisions at √sNN=19.6, 62.4, 130, and 200 GeV using the STAR detector at the Relativistic Heavy Ion Collider. K/π fluctuations in central collisions show little dependence on incident energy and are on the same order as those from NA49 at the Super Proton Synchrotron in central Pb+Pb collisions at √sNN=12.3 and 17.3 GeV. We report results for the collision centrality dependence of K/π fluctuations and results for charge-separated fluctuations. We observe that the K/π fluctuations scale with the charged particle multiplicity density.

M3 - Article

SN - 0031-9007

VL - 103

SP - 092301/1-092301/6

JO - Physical review letters

JF - Physical review letters

IS - 9

ER -

K/π fluctuations at relativistic energies

Abstract

Fingerprint

Cite this