Nuclear Theory·nucl-th

Friday·September 4, 2020

18 papers—7 primary·11 cross-listed

01
[Submitted on 2 Sept 2020]
Alternate Solution of the $α$ -Potential Mystery
Vlad Avrigeanu · Marilena Avrigeanu
A consistent set of statistical-model input parameters, validated by analysis of various independent data, makes possible the assessment of an $α$ -particle optical model potential [Phys. Rev. C {\bf 90}, 044612 (2014)] also for nucleon-induced $α$ -emission within $A$ $\sim$ 60 mass-number range. The advantage of recent data for low-lying states feeding is taken as well. Consideration of additional reaction channels leading to increase of the $α$ -emission beyond the statistical predictions has concerned the pickup direct interaction and Giant Quadrupole Resonance similar features.
Comments:
5+28 pages, 5+24 figures
Subjects:
Nuclear Theory (nucl-th); Nuclear Experiment (nucl-ex)
arXiv:
2009.01361 [pdf]
0 citations
02
[Submitted on 3 Sept 2020]
Utility of antiproton-nucleus scattering for probing nuclear surface density distributions
K. Makiguchi · W. Horiuchi · A. Kohama
Antiproton-nucleon ( $p ˉ N$ ) total cross sections are typically 3-4 times larger than the $N N$ ones at incident energies from a few hundreds to thousands MeV. We investigate antiproton-nucleus scattering as it could work as a probe of the nuclear structure giving the sensitivity differently from a proton probe. High-energy antiproton-nucleus reactions are reasonably described by the Glauber model with a minimal profile function that reproduces the $p ˉ N$ and $p ˉ$ - $^{12}$ C cross section data. In contrast to the proton-nucleus scattering, we find that the complete absorption occurs even beyond the nuclear radius due to the large $p ˉ N$ elementary cross sections, which shows stronger sensitivity to the nuclear density distribution in the tail region. This sensitivity is quantified in the total reaction cross sections with various density profiles for future measurement including neutron-rich unstable nuclei.
Comments:
9 pages, 9 figures, to appear in Phys. Rev. C
Subjects:
Nuclear Theory (nucl-th)
arXiv:
2009.01413 [pdf]
PRC(2020)·4 citations
03
[Submitted on 3 Sept 2020]
Jet quenching in the hadron gas: An exploratory study
Hannah Elfner🇳🇴 · Philipp Dorau🇩🇪 · Jean-Bernard Rose🇩🇪 · Daniel Pablos🇳🇴
In most calculations of hard particle suppression in heavy-ion reactions the hadronic stage has been neglected due to formation time arguments. Most of the hard particle shower exits the hot and dense medium before the system enters the hadronic evolution. In this contribution, a first assessment within the hadronic transport approach SMASH (Simulating Many Accelerated Strongly-interacting Hadrons) of rescattering effects on hard particles is presented. In particular, it is shown that the hadronic energy loss depends on the particle species as well as the energy of the probe. A parametrization for the $⟨ q ~ ⟩$ parameter as a function of temperature and particle energy is given for pions. Overall, major effects of the hadronic stage are expected in the transverse momentum range from 2-10 GeV and therefore jet sub-structure analysis and (hard-soft) correlation observables might be affected.
Comments:
5 pages, 4 figures, Proceedings for HardProbes2020, 1-6 June 2020, Austin, Texas (virtual)
Subjects:
Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)
arXiv:
2009.01736 [pdf]
PoS(2021)·2 citations
04
[Submitted on 3 Sept 2020]
Electron capture in stars
Karlheinz Langanke · Gabriel Martínez-Pinedo · Remco Zegers
Electron captures on nuclei play an essential role for the dynamics of several astrophysical objects. The capture rate can be derived in perturbation theory where allowed nuclear transitions (Gamow-Teller transitions) dominate, except at the higher temperatures achieved in core-collapse supernovae where also forbidden transitions contribute significantly to the rates. There has been decisive progress in recent years in measuring Gamow-Teller (GT) strength distributions using novel experimental techniques based on charge-exchange reactions. These measurements provide not only data for the GT distributions of ground states for many relevant nuclei, but also serve as valuable constraints for nuclear models which are needed to derive the capture rates for the many nuclei, for which no data exist yet. In particular models are needed to evaluate the stellar capture rates at finite temperatures, where the capture can also occur on excited nuclear states. There has also been significant progress in recent years in the modelling of stellar capture rates. This has been made possible by advances in nuclear many-body models as well as in computer soft- and hardware. Specifically to derive reliable capture rates for core-collapse supernovae a dedicated strategy has been developed based on a hierarchy of nuclear models specifically adapted to the abundant nuclei and astrophysically conditions present at the various collapse conditions. This manuscript reviews the experimental and theoretical progress achieved recently in deriving stellar electron capture rates. It also discusses the impact these improved rates have on the various astrophysical objects. (Abridged)
Comments:
64 pages, 24 figures, Review article submitted to Reports on Progress in Physics
Subjects:
Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Experiment (nucl-ex)
arXiv:
2009.01750 [pdf]
Rept.Prog.Phys.(2021)·59 citations
05
[Submitted on 3 Sept 2020]
Coulomb sum rule for $^{4}$ He and $^{16}$ O from coupled-cluster theory
J. E. Sobczyk🇩🇪 · B. Acharya🇩🇪 · S. Bacca🇩🇪 · G. Hagen🇺🇸
We demonstrate the capability of coupled-cluster theory to compute the Coulomb sum rule for the $^{4}$ He and $^{16}$ O nuclei using interactions from chiral effective field theory. We perform several checks, including a few-body benchmark for $^{4}$ He. We provide an analysis of the center-of-mass contaminations, which we are able to safely remove. We then compare with other theoretical results and experimental data available in the literature, obtaining a fair agreement. This is a first and necessary step towards initiating a program for computing neutrino-nucleus interactions from first principles and supporting the experimental long-baseline neutrino program with a state-of-the-art theory that can reach medium-mass nuclei.
Comments:
10 pages, 5 figures
Subjects:
Nuclear Theory (nucl-th); High Energy Physics — Experiment (hep-ex); Nuclear Experiment (nucl-ex)
arXiv:
2009.01761 [pdf]
PRC(2020)·19 citations
06
[Submitted on 3 Sept 2020]
The importance of charged particle reactions in the r-process on supernovae and neutron stars
Pedro V. Guillaumon · Iuda D. Goldman
We propose a $(p, x n)$ mechanism with dynamic production as a new set of nuclear reactions that could produce high density neutrons and explain the r- and rp-elements. We calculate the rate of thorium and uranium produced by our proposed mechanism and show that it is compatible with different stellar conditions found in explosive events at an initial temperature of $T \geq 3 \times 1 0^{9} K$ with a "freeze-out" by a neutrino-driven wind. We show that charged particle reactions could explain the discrepancies in the abundances of $^{232} T h$ and $^{235, 238} U$ nucleochronometers. We extend the endpoint of the rapid proton (rp) process far beyond the previous work by showing that $(p, x n)$ reactions could contribute to the nucleosynthesis of heavy stable neutron deficient nuclides, like $^{190} P t$ , $^{184} O s$ , $^{180} W$ and $^{174}$ Hf. This implies in a broader definition of the rp-process and has important consequences for the nucleosynthesis of heavy elements. We show that we did not need to assume an extreme condition for the drip line of super neutron-rich nuclei.
Subjects:
Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR)
arXiv:
2009.01814 [pdf]
1 citation
07
[Submitted on 3 Sept 2020]
Moving away from singly-magic nuclei with Gorkov Green's function theory
Vittorio Somà🇫🇷 · Carlo Barbieri🇬🇧 · Thomas Duguet🇫🇷 · Petr Navrátil🇨🇦
Ab initio calculations of bulk nuclear properties (ground-state energies, root mean square charge radii and charge density distributions) are presented for seven complete isotopic chains around calcium, from argon to chromium. Calculations are performed within the Gorkov self-consistent Green's function approach at second order and make use of two state-of-the-art two- plus three-nucleon Hamiltonians, $N N$ + $3 N (lnl)$ and NNLO $_{sat}$ . An overall good agreement with available experimental data is found, in particular for differential energies (charge radii) when the former (latter) interaction is employed. Remarkably, neutron magic numbers $N = 28, 32, 34$ emerge and evolve following experimental trends. In contrast, pairing gaps are systematically underestimated. General features of the isotopic dependence of charge radii are also reproduced, as well as charge density distributions. A deterioration of the theoretical description is observed for certain nuclei and ascribed to the inefficient account of (static) quadrupole correlation in the present many-body truncation scheme. In order to resolve these limitations, we advocate the extension of the formalism towards incorporating breaking of rotational symmetry or, alternatively, performing a stochastic sampling of the self-energy.
Comments:
17 pages, 14 figures
Subjects:
Nuclear Theory (nucl-th); Nuclear Experiment (nucl-ex)
arXiv:
2009.01829 [pdf]
EPJA(2021)·42 citations
08
[Submitted on 1 Sept 2020] (cross-list from hep-th)
The cosmological constant and the use of cutoffs
John F. Donoghue🇺🇸
Of the contributions to the cosmological constant, zero-point energy and self energy contributions scale as $Λ^{4}$ where $Λ$ is an ultraviolet cutoff used to regulate the calculations. I show that such contributions vanish when calculated in perturbation theory. This demonstration uses a little-known modification to perturbation theory found by Honerkamp and Meetz and by Gerstein, Jackiw, Lee and Weinberg which comes into play when using cutoffs and interactions with multiple derivatives, as found in chiral theories and gravity. In a path integral treatment, the new interaction arises from the path integral measure. This reduces the sensitivity of the cosmological constant to the high energy cutoff significantly, although it does not resolve the cosmological constant problem. The feature removes one of the common motivations for supersymmetry. It also calls into question some of the results of the Asymptotic Safety program. Covariance and quadratic cutoff dependence are also briefly discussed.
Comments:
9 pages, 1 figure Reference to Fradkin - Vilkovisky added, as well as some clarifying comments
Subjects:
High Energy Physics — Theory (hep-th); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2009.00728 [pdf]
PRD(2021)·42 citations
09
[Submitted on 3 Sept 2020] (cross-list from nucl-ex)
Status of CME Search Before Isobar Collisions and Methods of Blind Analysis From STAR
Prithwish Tribedy (for the STAR Collaboration)🇺🇸
The STAR collaboration is currently pursuing the blind analysis of the data for isobar collisions that was performed at RHIC in the year 2018 to make a decisive test of the Chiral Magnetic Effect (CME). Why is it so difficult to detect signals of CME in the experiment? Do we really understand different sources of background? Why observing similar charge separation between p/d+A and A+A does not stop us from pursuing the search for CME? In this contribution, I attempt to address some of these questions and briefly outline a few recent STAR analyses based on new methods and observables to isolate the possible CME-driven signal and non-CME background contributions at the top RHIC energy. Finally, I describe the procedure for the blind analysis of the isobar data. An outstanding question remains -- what happens if we go down in energy? I address this by discussing how the new event-plane detector (EPD) upgrade provides a new capability at STAR towards CME search using the data from the RHIC BES-II program.
Comments:
Part of Proceedings, 36th Winter Workshop on Nuclear Dynamics (WWND 2020) and STAR Note SN0755
Subjects:
Nuclear Experiment (nucl-ex); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2009.01230 [pdf]
J.Phys.Conf.Ser.(2020)·4 citations
10
[Submitted on 2 Sept 2020] (cross-list from hep-ph)
Left-right symmetry and leading contributions to neutrinoless double beta decay
Gang Li🇺🇸 · Michael Ramsey-Musolf🇨🇳 · Juan Carlos Vasquez🇺🇸
We study the impact of the mixing (LR mixing) between the standard model $W$ boson and its hypothetical, heavier right-handed parter $W_{R}$ on the neutrinoless double beta decay ( $0 ν β β$ -decay) rate. Our study is done in the minimal left-right symmetric model assuming type-II dominance scenario with charge conjugation as the left-right symmetry. We then show that the $0 ν β β$ -decay rate may be dominated by the contribution proportional to this LR mixing, which at the hadronic level induces the leading-order contribution to the interaction between two pions and two charged leptons. The resulting long-range pion exchange contribution can significantly enhance the decay rate compared to previously considered short-range contributions. Finally, we find that even if future cosmological experiments rule out the inverted hierarchy for neutrino masses, there are still good prospects for a positive signal in the next generation of $0 ν β β$ -decay experiments.
Comments:
6 pages, 3 figures
Subjects:
High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2009.01257 [pdf]
PRL(2021)·46 citations
11
[Submitted on 2 Sept 2020] (cross-list from hep-ph)
Proton spin after 30 years: what we know and what we don't?
Xiangdong Ji🇺🇸 · Feng Yuan🇺🇸 · Yong Zhao🇺🇸
More than three decades has passed since the European Muon Collaboration published the first surprising result on the spin structure of the proton. Much theoretical and experimental progress has been made in understanding the origins of the proton spin. In this review, we will discuss what we have learned so far, what are still missing, and what we shall expect to learn from the upcoming experiments including JLab 12 GeV and Electron-Ion Collider. In particular, we focus on first principles calculations and experimental measurements of the total gluon helicity $Δ G$ , and quark and gluon orbital angular momenta.
Comments:
17 pages, 4 figures, to appear in Nature Review
Subjects:
High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Experiment (hep-ex); High Energy Physics — Lattice (hep-lat); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2009.01291 [pdf]
Nature Rev.Phys.(2021)·137 citations
12
[Submitted on 2 Sept 2020] (cross-list from hep-ph)
Jet fragmentation function in heavy-ion collisions
Paul Caucal🇫🇷 · Edmond Iancu🇫🇷 · Alfred H. Mueller🇺🇸 · Gregory Soyez🇫🇷
We study the fragmentation function of jets propagating through a dense quark-gluon plasma within perturbative QCD. Our results for its nuclear modification factor are in qualitative agreement with the experimental data in Pb+Pb collisions at the LHC. In particular, we reproduce the enhancements seen in the data at both relatively soft and relatively large transverse momenta, with clear physical interpretations. The perturbative predictions however are quite sensitive to the value of the infrared cutoff mimicking the confinement scale, due to the fact that the fragmentation function is not an infrared safe quantity. To remedy this, we propose a new observable -- the (primary) subjet fragmentation function -- which is infrared safe and has features similar to the fragmentation function. We provide predictions for this observable in the vacuum and in heavy-ion collisions that could be tested against the experimental data.
Comments:
4 pages, 4 figures; 10th International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions
Subjects:
High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2009.01350 [pdf]
PoS(2021)·2 citations
13
[Submitted on 3 Sept 2020] (cross-list from hep-ph)
Brownian motion of neutrinos in the Sun [On the distribution of collisions of a neutrino with nucleons of the Sun]
L.M. Slad🇷🇺
When solving the solar neutrino problem on the basis of the hypothesis of the existence of a new interaction between electron neutrinos and nucleons, carried by a massless pseudoscalar boson, it becomes necessary to find the consequences of the short-term Brownian motion of neutrinos in the Sun. Earlier, we transmitted these consequences by the effective number of collisions of a neutrino with nucleons of the Sun, assuming the equality of fluxes near the Earth of left- and right-handed solar neutrinos. In this paper, we analyze the transfer of the mentioned consequences by a test geometric distribution of collisions with one free parameter. This distribution provides good agreement between theoretical and experimental results for all five observed processes with solar neutrinos, while it gives the ratio of fluxes near the Earth of left- and right-handed neutrinos equal to 0.516:0.484. With such a ratio, the acceptability of the method of the effective number of collisions of a neutrino with nucleons is again confirmed.
Comments:
6 pages. Journal version
Subjects:
High Energy Physics — Phenomenology (hep-ph); Solar and Stellar Astrophysics (astro-ph.SR); High Energy Physics — Experiment (hep-ex); Nuclear Theory (nucl-th)
arXiv:
2009.01528 [pdf]
Nucl. Phys. A 1021 (2022) 122425·0 citations
14
[Submitted on 3 Sept 2020] (cross-list from hep-ph)
A fast centrality-meter for heavy-ion collisions at the CBM experiment
Manjunath Omana Kuttan🇩🇪 · Jan Steinheimer🇩🇪 · Kai Zhou🇩🇪 · Andreas Redelbach🇩🇪 · Horst Stoecker🇩🇪
A new method of event characterization based on Deep Learning is presented. The PointNet models can be used for fast, online event-by-event impact parameter determination at the CBM experiment. For this study, UrQMD and the CBM detector simulation are used to generate Au+Au collision events at 10 AGeV which are then used to train and evaluate PointNet based architectures. The models can be trained on features like the hit position of particles in the CBM detector planes, tracks reconstructed from the hits or combinations thereof. The Deep Learning models reconstruct impact parameters from 2-14 fm with a mean error varying from -0.33 to 0.22 fm. For impact parameters in the range of 5-14 fm, a model which uses the combination of hit and track information of particles has a relative precision of 4-9 % and a mean error of -0.33 to 0.13 fm. In the same range of impact parameters, a model with only track information has a relative precision of 4-10 % and a mean error of -0.18 to 0.22 fm. This new method of event-classification is shown to be more accurate and less model dependent than conventional methods and can utilize the performance boost of modern GPU processor units.
Comments:
Replaced with version accepted for publication. 10 pages, 8 figures
Subjects:
High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
arXiv:
2009.01584 [pdf]
PLB(2020)·46 citations
15
[Submitted on 1 Sept 2020] (cross-list from math.AP)
Local well-posedness in Sobolev spaces for first-order barotropic causal relativistic viscous hydrodynamics
Fabio S. Bemfica · Marcelo M. Disconzi · P. Jameson Graber
We study the theory of relativistic viscous hydrodynamics introduced in arXiv:1109.0985 and arXiv:1907.12695, which provided a causal and stable first-order theory of relativistic fluids with viscosity in the case of barotropic fluids. The local well-posedness of its equations of motion has been previously established in Gevrey spaces. Here, we improve this result by proving local well-posedness in Sobolev spaces.
Comments:
arXiv admin note: text overlap with arXiv:1911.02504
Subjects:
math.AP (math.AP); Nuclear Theory (nucl-th)
arXiv:
2009.01621 [pdf]
4 citations
16
[Submitted on 3 Sept 2020] (cross-list from hep-ph)
Role of the conserved charges in the chiral symmetry restoration phase transition
Pedro Costa🇵🇹 · Renan Câmara Pereira🇵🇹 · Constança Providência🇵🇹
The effect of conserved baryon, isospin and strangeness charges on the behavior of phase transitions in dense matter is studied. Baryonic matter is described within the three-flavor Polyakov $-$ Nambu $-$ Jona-Lasinio model and several charge fractions $Y_{Q}$ are considered. The role of the vector interaction, which can be important to describe dense systems, is discussed. Special attention is given to the case with charge fraction $Y_{Q} = 0.4$ , due to its importance in heavy-ion collisions and core-collapse supernova matter. It is shown that the possible formation of chiral-symmetric quark matter in the laboratory will be favored in asymmetric matter. Besides, the inclusion of the vector interaction reinforces the formation of quark matter at lower densities.
Comments:
8 pages, 4 figures
Subjects:
High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
arXiv:
2009.01781 [pdf]
PRD(2020)·12 citations
17
[Submitted on 3 Sept 2020] (cross-list from hep-ph)
Operator Counting and Soft Blocks in Chiral Perturbation Theory
Lin Dai🇺🇸 · Ian Low🇺🇸 · Thomas Mehen🇺🇸 · Abhishek Mohapatra🇺🇸
Chiral perturbation theory (ChPT) is a low-energy effective field theory of QCD and also a nonlinear sigma model based on the symmetry breaking pattern $SU (N_{f}) \times SU (N_{f}) \to SU (N_{f})$ . In the limit of massless $N_{f}$ quarks, we enumerate the independent operators without external sources in ChPT using an on-shell method, by counting and presenting the soft blocks at each order in the derivative expansion, up to $O (p^{10})$ . Given the massless on-shell condition and total momentum conservation, soft blocks are homogeneous polynomials of kinematic invariants exhibiting the Adler's zero when any external momentum becomes soft and vanishing. In addition, soft blocks are seeds for recursively generating all tree amplitudes of Nambu-Goldstone bosons without recourse to ChPT, and in one-to-one correspondence with the "low energy constants" which are the Wilson coefficients. Relations among operators, such as those arising from equations of motion, integration-by-parts, hermiticity, and symmetry structure, manifest themselves in the soft blocks in simple ways. We find agreements with the existing results up to NNNLO, and make a prediction at N $^{4}$ LO.
Comments:
31 pages, 2 figures and 6 tables. Mathematica codes added as ancillary files
Subjects:
High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Theory (hep-th); Nuclear Theory (nucl-th)
arXiv:
2009.01819 [pdf]
PRD(2020)·22 citations
18
[Submitted on 3 Sept 2020] (cross-list from hep-ph)
Regularization of the Nambu-Jona Lasinio model under a uniform magnetic field and the role of the anomalous magnetic moments
R. M. Aguirre🇦🇷
The vacuum contribution to quark matter under a uniform magnetic field within the SU(3) version of the Nambu and Jona-Lasinio model is studied. The standard regularization procedure is examined and a new prescription is proposed. For this purpose analytic regularization and a subtraction scheme are used to deal with divergencies depending on the magnetic intensity. This scheme is combined with the standard three momentum cutoff recipe, and reduces to it for vanishing magnetic intensity. Furthermore, the effects of a direct coupling between the anomalous magnetic moments of the quarks and the magnetic field is considered. Single particle properties as well as bulk thermodynamical quantities are studied for a configuration of matter found in neutron stars. A wide range of baryonic densities and magnetic intensities are examined at zero temperature.
Comments:
Major revision
Subjects:
High Energy Physics — Phenomenology (hep-ph); High Energy Astrophysical Phenomena (astro-ph.HE); Nuclear Theory (nucl-th)
arXiv:
2009.01828 [pdf]
PRD(2020)·21 citations

Affiliations

first authorsco-authorsvia INSPIRE