Nuclear Theory·nucl-th

Friday·September 9, 2022

12 papers—5 primary·7 cross-listed

06
[Submitted on 7 Sept 2022] (cross-list from gr-qc)
Neutron stars as extreme laboratories for gravity tests
Lijing Shao🇨🇳 · Kent Yagi🇺🇸
Neutron stars are versatile in their application to studying various important aspects of fundamental physics, in particular strong-field gravity tests and the equation of state for super-dense nuclear matter at low temperatures. However, in many cases these two objectives are degenerate to each other. We discuss how pulsar timing and gravitational waves provide accurate measurements of neutron star systems and how to effectively break the degeneracy using tools like universal relations. We also present perspectives on future opportunities and challenges in the field of neutron star physics.
Comments:
5 pages, 2 figures; accepted by Science Bulletin
Subjects:
General Relativity and Quantum Cosmology (gr-qc); High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
arXiv:
2209.03351 [pdf]
Sci.Bull.(2022)·30 citations
07
[Submitted on 7 Sept 2022] (cross-list from nucl-ex)
Search for the Chiral Magnetic Effect in Au+Au collisions at $s_{_{NN}} = 27$ GeV with the STAR forward Event Plane Detectors
STAR Collaboration: B. E. Aboona🇺🇸 · J. Adam🇨🇿 · L. Adamczyk🇵🇱 · J. R. Adams · I. Aggarwal🇮🇳 · M. M. Aggarwal🇮🇳 · Z. Ahammed · D. M. Anderson🇺🇸 · E. C. Aschenauer🇺🇸 · J. Atchison🇺🇸 · V. Bairathi🇨🇱 · W. Baker🇺🇸 and 359 other authors
A decisive experimental test of the Chiral Magnetic Effect (CME) is considered one of the major scientific goals at the Relativistic Heavy-Ion Collider (RHIC) towards understanding the nontrivial topological fluctuations of the Quantum Chromodynamics vacuum. In heavy-ion collisions, the CME is expected to result in a charge separation phenomenon across the reaction plane, whose strength could be strongly energy dependent. The previous CME searches have been focused on top RHIC energy collisions. In this Letter, we present a low energy search for the CME in Au+Au collisions at $s_{_{NN}} = 27$ GeV. We measure elliptic flow scaled charge-dependent correlators relative to the event planes that are defined at both mid-rapidity $∣ η ∣ < 1.0$ and at forward rapidity $2.1 < ∣ η ∣ < 5.1$ . We compare the results based on the directed flow plane ( $Ψ_{1}$ ) at forward rapidity and the elliptic flow plane ( $Ψ_{2}$ ) at both central and forward rapidity. The CME scenario is expected to result in a larger correlation relative to $Ψ_{1}$ than to $Ψ_{2}$ , while a flow driven background scenario would lead to a consistent result for both event planes. In 10-50\% centrality, results using three different event planes are found to be consistent within experimental uncertainties, suggesting a flow driven background scenario dominating the measurement. We obtain an upper limit on the deviation from a flow driven background scenario at the 95\% confidence level. This work opens up a possible road map towards future CME search with the high statistics data from the RHIC Beam Energy Scan Phase-II.
Comments:
main: 16 pages, 5 figures; supplementary material: 2 pages, 1 figure
Subjects:
Nuclear Experiment (nucl-ex); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2209.03467 [pdf]
PLB(2023)·29 citations
08
[Submitted on 8 Sept 2022] (cross-list from astro-ph.HE)
Light Curves and Event Rates of Axion Instability Supernovae
Kanji Mori🇯🇵 · Takashi J. Moriya🇯🇵 · Tomoya Takiwaki🇯🇵 · Kei Kotake🇯🇵 · Shunsaku Horiuchi🇺🇸 · Sergei I. Blinnikov🇯🇵
It was recently proposed that exotic particles can trigger a new stellar instability which is analogous to the e-e+ pair instability if they are produced and reach equilibrium in the stellar plasma. In this study, we construct axion instability supernova (AISN) models caused by the new instability to predict their observational signatures. We focus on heavy axion-like particles (ALPs) with masses of ~400 keV--2 MeV and coupling with photons of g_{ag}~10^{-5} GeV^{-1}. It is found that the 56Ni mass and the explosion energy are significantly increased by ALPs for a fixed stellar mass. As a result, the peak times of the light curves of AISNe occur earlier than those of standard pair-instability supernovae by 10--20 days when the ALP mass is equal to the electron mass. Also, the event rate of AISNe is 1.7--2.6 times higher than that of pair-instability supernovae, depending on the high mass cutoff of the initial mass function.
Comments:
10 pages, 6 figures, 1 table, accepted for publication in ApJ
Subjects:
High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2209.03517 [pdf]
ApJ(2023)·7 citations
09
[Submitted on 8 Sept 2022] (cross-list from hep-ph)
T-odd Leading-Twist Quark TMDs at Small $x$
Yuri V. Kovchegov🇺🇸 · M. Gabriel Santiago🇺🇸
We study the small- $x$ asymptotics of the flavor non-singlet T-odd leading-twist quark transverse momentum dependent parton distributions (TMDs), the Sivers and Boer-Mulders functions. While the leading eikonal small- $x$ asymptotics of the quark Sivers function is given by the spin-dependent odderon, we are interested in revisiting the sub-eikonal correction considered by us earlier. We first simplify the expressions for both TMDs at small Bjorken $x$ and then construct small- $x$ evolution equations for the resulting operators in the large- $N_{c}$ limit, with $N_{c}$ the number of quark colors. For both TMDs, the evolution equations resum all powers of the double-logarithmic parameter $α_{s} ln^{2} (1/ x)$ , where $α_{s}$ is the strong coupling constant, which is assumed to be small. Solving these evolution equations numerically (for the Sivers function) and analytically (for the Boer-Mulders function) we arrive at the following leading small- $x$ asymptotics of these TMDs at large $N_{c}$ : \begin{align} f_{1 \: T}^{\perp \: NS} (x \ll 1 ,k_T^2) & = C_O (x, k_T^2) \, \frac{1}{x} + C_1 (x, k_T^2) \, \left( \frac{1}{x} \right)^{3.4 \, \sqrt{\frac{\alpha_s \, N_c}{4 \pi}}} , \notag \\ h_1^{\perp \, \textrm{NS}} (x \ll 1, k_T^2) & = C (x, k_T^2) \left( \frac{1}{x} \right)^{-1}. \notag \end{align} The functions $C_{O} (x, k_{T}^{2})$ , $C_{1} (x, k_{T}^{2})$ , and $C (x, k_{T}^{2})$ can be readily obtained in our formalism: they are mildly $x$ -dependent and do not strongly affect the power-of- $x$ asymptotics shown above. The function $C_{O}$ , along with the $1/ x$ factor, arises from the odderon exchange. For the sub-eikonal contribution to the quark Sivers function (the term with $C_{1}$ ), our result shown above supersedes the one obtained in our previous work due to the new contributions identified recently.
Comments:
50 pages, 5 figures
Subjects:
High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Experiment (hep-ex); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2209.03538 [pdf]
JHEP(2022)·42 citations
10
[Submitted on 8 Sept 2022] (cross-list from hep-ex)
Spin polarization measurements in relativistic heavy-ion collisions
Debojit Sarkar🇺🇸
The hot and dense matter formed in relativistic heavy-ion collisions at Relativistic Heavy Ion Collider (RHIC) and Large Hadron Collider (LHC) is termed quark-gluon plasma (QGP). The evolution of the medium is characterized by non-trivial velocity and vorticity fields, resulting in the polarization of the produced particles. The spin polarization, being sensitive to the hydrothermal (flow velocity and temperature) gradients, is unique compared to conventional observables that are sensitive to the hydrothermal fields only. Hence, the recent measurements of global and local hyperon spin polarization and vector meson spin alignment by the LHC and STAR collaborations provide a unique opportunity to probe the QGP substructure with finer details.
Comments:
Presented at Quark Matter 2022 (Krakow, Poland, Plenary Session VII)-- https://indico.cern.ch/event/895086/contributions/4615144/
Subjects:
High Energy Physics — Experiment (hep-ex); High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th); Data Analysis, Statistics and Probability (physics.data-an)
arXiv:
2209.03689 [pdf]
Acta Phys.Polon.Supp.(2023)·0 citations
11
[Submitted on 8 Sept 2022] (cross-list from nucl-ex)
Exploring the neutron skin by hyperon-antihyperon production in antiproton-nucleus interactions
Martin Christiansen🇩🇪 · Falk Schupp🇩🇪 · Patrick Achenbach🇩🇪 · Michael Bölting🇩🇪 · Josef Pochodzalla🇩🇪 · Marcell Steinen🇩🇪
In this work we propose a new method to measure the evolution of the neutron skin thickness between different isotopes. We consider antiproton-nucleus interactions close to the production threshold of $Λ Λ$ and $Σ Λ$ pairs. At low energies, $Λ Λ$ pairs are produced in p + p collisions, while $Σ Λ$ pairs can only be produced in p + n interactions. Measuring these cross sections provides information on the neutron skin thickness
Comments:
4 pages, 3 figures, 14th International Conference on Hypernuclear and Strange Particle Physics - HYP2022
Subjects:
Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2209.03875 [pdf]
EPJ Web Conf.(2022)·2 citations
12
[Submitted on 8 Sept 2022] (cross-list from hep-ph)
Random statistical analysis of transverse momentum spectra of strange particles and dependence of related parameters on centrality in high energy collisions at the LHC
Xu-Hong Zhang🇨🇳 · Fu-Hu Liu🇨🇳 · Khusniddin K. Olimov🇺🇿 · Airton Deppman🇧🇷
We have studied the transverse momentum ( $p_{T}$ ) spectra of the final-state strange particles, including $K^{\pm}$ , $ϕ$ , $Ξ$ , and $Ω$ , produced in high energy lead-lead (Pb-Pb), proton-lead ( $p$ -Pb), xenon-xenon (Xe-Xe) collisions at the Large Hadron Collider (LHC). Taking into account the contribution of multi-quark composition, whose probability density distribution is described by the modified Tsallis-Pareto-type function, we simulate the $p_{T}$ spectra of the final-state strange particles by a Monte Carlo method, which is shown to be in good agreement with the experimental data in most the cases. The kinetic freeze-out parameters are obtained. The present method provides a new tool for studying the spectra of various particles produced in high energy collisions, reflecting more realistically the collision process, which is of great significance to study the formation and properties of the produced particles.
Comments:
19 pages, 9 figures. Advances in High Energy Physics, Accepted
Subjects:
High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Experiment (hep-ex); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2209.03894 [pdf]
Adv.High Energy Phys.(2022)·2 citations

Affiliations

first authorsco-authorsvia INSPIRE

Neutron stars as extreme laboratories for gravity tests

Search for the Chiral Magnetic Effect in Au+Au collisions at sNN​​​=27 GeV with the STAR forward Event Plane Detectors

Light Curves and Event Rates of Axion Instability Supernovae

T-odd Leading-Twist Quark TMDs at Small x

Spin polarization measurements in relativistic heavy-ion collisions

Exploring the neutron skin by hyperon-antihyperon production in antiproton-nucleus interactions

Random statistical analysis of transverse momentum spectra of strange particles and dependence of related parameters on centrality in high energy collisions at the LHC

Affiliations

Search for the Chiral Magnetic Effect in Au+Au collisions at $s_{_{NN}} = 27$ GeV with the STAR forward Event Plane Detectors

T-odd Leading-Twist Quark TMDs at Small $x$