“…In the coalescence picture, deuteron, helium-3 and tritium are expected to be created by nucleons with the same spread, and the parameter σ should thus be the same for all three particles. In the previous subsection, we saw that the spread is already well determined by antideuteron experiments, which has been confirmed independently by the measurements on the baryon emission volume by the ALICE collaboration [7,29]. Thus, we can allow ourselves to degrade r 3 He rms to a free parameter to better describe the effective ground state of the nucleus.…”
Section: Comment On Helium-3 and Tritium Productionsupporting
confidence: 60%
“…3, where the best fit to the invariant differential yield of antideuterons measured by the ALICE collaboration [28] is plotted using Pythia 8 and QGSJET II. Furthermore, it describes the behaviour of the nontrivial baryon emission volume as measured by the ALICE collaboration [7,29]. This is particularly important as it provides a method of determining the parameter σ independent of an event generator (orange triangle in Fig.…”
Section: Comparison With Experimental Datamentioning
confidence: 99%
“…The WiFunC model without any Lorentz boost gives a similar fit as the standard coalescence model and is shown for comparison (green dashed line). baryon emission volume with increasing transverse momentum [29], is also naturally described by the WiFunC model [7]. Moreover, the hints are irrelevant for astrophysical processes since they are at present only observed at high energies and multiplicities.…”
The production mechanism of light nuclei, such as deuteron, helium-3, tritium and their antiparticles, has recently attracted an increased attention from the astroparticle and heavy ion communities. The expected low astrophysical background of light antinulei makes them ideal probes for exotic astrophysical processes, such as dark matter annihilations. At the same time, they can be used to measure two-nucleon correlations and density fluctuations in heavy ion collisions, which may shed light on the QCD phase diagram. Motivated by the importance of light antinuclei in cosmic ray studies, we developed a new coalescence model for light (anti)nuclei that includes both the size of the formation region, which is process dependent, and momentum correlations in a semiclassical picture. We have employed the model as an afterburner to the event generators Pythia 8 and QGSJET II, and find that the model agrees well with experimental data on antideuteron and antihelium-3 production in e + e − , pp, pBe and pAl collisions at various energies. In this paper, we review this model and update existing fits to experimental data based on new insights.
“…In the coalescence picture, deuteron, helium-3 and tritium are expected to be created by nucleons with the same spread, and the parameter σ should thus be the same for all three particles. In the previous subsection, we saw that the spread is already well determined by antideuteron experiments, which has been confirmed independently by the measurements on the baryon emission volume by the ALICE collaboration [7,29]. Thus, we can allow ourselves to degrade r 3 He rms to a free parameter to better describe the effective ground state of the nucleus.…”
Section: Comment On Helium-3 and Tritium Productionsupporting
confidence: 60%
“…3, where the best fit to the invariant differential yield of antideuterons measured by the ALICE collaboration [28] is plotted using Pythia 8 and QGSJET II. Furthermore, it describes the behaviour of the nontrivial baryon emission volume as measured by the ALICE collaboration [7,29]. This is particularly important as it provides a method of determining the parameter σ independent of an event generator (orange triangle in Fig.…”
Section: Comparison With Experimental Datamentioning
confidence: 99%
“…The WiFunC model without any Lorentz boost gives a similar fit as the standard coalescence model and is shown for comparison (green dashed line). baryon emission volume with increasing transverse momentum [29], is also naturally described by the WiFunC model [7]. Moreover, the hints are irrelevant for astrophysical processes since they are at present only observed at high energies and multiplicities.…”
The production mechanism of light nuclei, such as deuteron, helium-3, tritium and their antiparticles, has recently attracted an increased attention from the astroparticle and heavy ion communities. The expected low astrophysical background of light antinulei makes them ideal probes for exotic astrophysical processes, such as dark matter annihilations. At the same time, they can be used to measure two-nucleon correlations and density fluctuations in heavy ion collisions, which may shed light on the QCD phase diagram. Motivated by the importance of light antinuclei in cosmic ray studies, we developed a new coalescence model for light (anti)nuclei that includes both the size of the formation region, which is process dependent, and momentum correlations in a semiclassical picture. We have employed the model as an afterburner to the event generators Pythia 8 and QGSJET II, and find that the model agrees well with experimental data on antideuteron and antihelium-3 production in e + e − , pp, pBe and pAl collisions at various energies. In this paper, we review this model and update existing fits to experimental data based on new insights.
“…In this work, we argue that neither two-particle correlations nor the source size can be neglected when describing the cluster formation in small interacting systems 2 . Furthermore, we will use this model to describe the production of hadrons and nuclei in high energy pp collisions and compare it to recent experimental data by the ALICE collaboration on the size of the baryon emitting source [48] and on the multiplicity and transverse momentum dependence of the coalescence factor B 2 [45,49,50]. Both data sets have been interpreted as evidence of collective flows, but we will show that the same characteristics are described using QCD inspired event generators, like QGSJET II [51,52] and Pythia 8.2 [53,54].…”
The formation of light nuclei can be described as the coalescence of clusters of nucleons into nuclei. In the case of small interacting systems, such as dark matter and $$e^+e^-$$
e
+
e
-
annihilations or pp collisions, the coalescence condition is often imposed only in momentum space and hence the size of the interaction region is neglected. On the other hand, in most coalescence models used for heavy ion collisions, the coalescence probability is controlled mainly by the size of the interaction region, while two-nucleon momentum correlations are either neglected or treated as collective flow. Recent experimental data from pp collisions at LHC have been interpreted as evidence for such collective behaviour, even in small interacting systems. We argue that these data are naturally explained in the framework of conventional QCD inspired event generators when both two-nucleon momentum correlations and the size of the hadronic emission volume are taken into account. To include both effects, we employ a per-event coalescence model based on the Wigner function representation of the produced nuclei states. This model reproduces well the source size for baryon emission and the coalescence factor $$B_2$$
B
2
measured recently by the ALICE collaboration in pp collisions.
“…If not, then the uncertainty on the assumed value of r 0 would be a source of systematic uncertainty. The values of r 0 are known with good precision for different pairs and collision systems [48,50], therefore we expect such uncertainty to be small. Besides, the assumption of the Gaussian shape of the r * distribution could be a source of systematic uncertainty since other models are considered in the literature.…”
We present a method for the measurement of parameters of elastic and inelastic interactions of charmonium with hadrons. In this technique, we use femtoscopic analysis of charmonium-hadron correlations at low relative momentum and the Lednicky-Lyuboshitz analytical model to extract the interaction parameters. We argue that such a study is already feasible in the LHCb experiment at the LHC, and we discuss the prospects for studies in STAR at RHIC and other experiments at the LHC.
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