REVIEW 3 major objections 4 minor 74 references
A holographic soft-wall model predicts that J/ψ mesons in a rotating quark-gluon plasma acquire a spin-rotation splitting of their spectral peaks, with the pattern depending on whether the meson momentum is parallel or perpendicular to the
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-04 00:57 UTC pith:MZIG7GDQ
load-bearing objection A genuinely new local-frame method and a clean parallel-axis result, but the transverse momentum claims rest on an uncontrolled quasi-classical approximation. the 3 major comments →
Spectral Functions of J/psi Meson in Rotating Thermal Background from Holography
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The vector field in a rotating AdS-like bulk, when projected onto spin eigenstates in a local inertial frame, yields retarded Green functions whose imaginary parts show three distinct invariant-mass peaks for J/ψ at T = 150 MeV. For momentum along the rotation axis, the peak masses obey ω(Ω) = ω(0) − ΩS_z (with orbital L_z = 0), so the λ = +1, 0, −1 states split linearly in Ω and the widths change by less than 1% up to Ω = 0.1 GeV. For momentum transverse to the axis, the fixed-momentum states are not eigenstates of total angular momentum; the projected Green function becomes non-diagonal, the extracted spectral functions for λ = +1 and λ = −1 develop multi-peak structures and negative regio
What carries the argument
The central object is the soft-wall holographic action for a bulk U(1) gauge field in a rotating AdS metric, combined with a local vielbein frame (e^a_M) that carries the rotation terms and allows spin to be defined at the boundary. The proof mechanism is the near-horizon incoming-wave expansion: analytically solving the equations of motion to next-to-leading order in (ζ/ζ_h − 1), numerically propagating to the boundary, and using the holographic dictionary to extract the retarded Green function; the spin projection onto circular polarizations then isolates the spectral functions ϱ_λ. The −ΩJ_z energy shift enters through the near-horizon frequency redefinition ω̃ = ω + (L_z + λ)Ω.
Load-bearing premise
The calculation freezes the transverse location (x, y) of the meson, treating it as a point particle on macroscopic scales while a plane wave microscopically; if Ωx or Ωy are not small compared with the inverse wavelength, the neglected mixing of Fourier modes would change the spectral functions.
What would settle it
Compute the same spectral functions by solving the bulk equations with the full coordinate-dependent rotating metric, without the classical-location freezing, and check whether the −ΩJ_z splitting and direction-dependent multi-peak structure survive; any sizable deviation would falsify the paper's central prediction.
If this is right
- For momentum along the rotation axis, the three spin peaks split linearly with Ω and widths stay within about 1%, so rotation acts essentially as a shift without distorting the line shape.
- For transverse momentum, the model predicts non-trivial interference: λ = ±1 spectral functions acquire multi-peak structure and negative values at large Ω, signalling that fixed-momentum spin projections are not angular-momentum eigenstates.
- The triplet splitting pattern provides a holographic benchmark for spin-dependent J/ψ properties in a vortical plasma, and the same framework with different dilaton parameters extends to φ and bottomonium.
- The predicted splittings are tied to the near-horizon condition ω̃ ≈ ω + (L_z + λ)Ω, giving a direct geometric origin for the rotational energy shift.
Where Pith is reading between the lines
- If the direction-dependent splitting holds, the relative heights and shifts of the three spin peaks in the J/ψ invariant-mass spectrum could serve as a vorticity probe in heavy-ion collisions, since the pattern encodes both the magnitude and the orientation of Ω relative to the meson momentum.
- The negative spectral regions at large transverse momentum suggest that single-particle spectral interpretation fails there; an editor-level extension is to compute the off-diagonal projected Green function to quantify the mixing angle between fixed-momentum and fixed-J_z bases as a function of q and Ω.
- The quasi-classical decoupling assumption should be tested by a solution retaining the full x, y dependence of the metric; if the Ωx, Ωy corrections matter at moderate Ω, the predicted triplet splitting may be a lower-order artifact rather than a stable signature.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper computes the invariant-mass spectral functions of the J/psi meson in a rotating thermal plasma using a soft-wall AdS/QCD model. Global rotation is implemented by a metric with off-diagonal terms proportional to Omega, and a local inertial frame is introduced so that spin projections lambda=0,+1,-1 are well defined. The equations of motion for the bulk vector field are solved with an incoming-wave boundary condition near the horizon, and the retarded Green function is projected onto polarization vectors. For momentum parallel to the rotation axis, the extracted peak masses follow the expected -Omega J_z shift and the widths are nearly Omega-independent. For perpendicular momentum, the spectral functions of spin-+1 and spin--1 states deviate from a single-peak form and can become negative at large Omega and transverse momentum; these features are attributed to off-diagonal mixing in the projected Green function.
Significance. If the perpendicular-momentum results are robust, the paper provides a concrete holographic prediction for spin-rotation splitting of quarkonium spectral functions, which is potentially relevant for spin-alignment measurements in heavy-ion collisions. The framework is presented clearly, the near-horizon analysis is explicit, and the paper includes a data-availability statement. However, the central perpendicular-momentum claim rests on an uncontrolled quasi-classical approximation, and the numerical evidence at the onset of the claimed effect is not yet sufficient. The parallel-axis result is a useful consistency check of the formalism, but it is not an independent prediction in the present form.
major comments (3)
- [Sec. II, Eqs. (14)–(16); Appendix A] The 'plane-wave/point-particle' approximation is not systematically controlled for the transverse-momentum case. The stated condition (15), Omega << omega,|q|, bounds the derivative of the metric (∂_x g ~ Omega) against the inverse wavelength, but the coefficient matrices T3 in Eq. (A1) retain terms of order Omega L_z and Omega^2 L_z^2. For the parameters of Sec. V.B (L_z=2.54, Omega=0.05–0.1 GeV), Omega L_z is 0.13–0.25 GeV; for q_y=2 GeV in Fig. 8 it reaches approximately 0.5 GeV, comparable to |q|. Thus the regime in which the paper reports deviations from -Omega J_z and negative spectral functions is precisely where the expansion parameter Omega L_z/|q| is O(0.25–1), not small. In the exact theory, a term like Omega y A_x becomes Omega ∂_{q_y} A_x, so fixing (x,y) neglects coupling between Fourier modes separated by Omega in q_y; replacing i∂_{q_y} by x is an uncontrolled stationary-
- [Sec. V.B, Figs. 4–8] The numerical support for the perpendicular-momentum claims is incomplete. The Breit-Wigner fit (58) fails exactly in the region where Omega L_z/|q| is not tiny (q_y=1 GeV, Omega > 0.07 GeV), and the lambda=+1 points are omitted from Figs. 5(b) and 6(b). The spectral functions in Figs. 7 and 8 contain visible oscillations attributed to 'numerical noise', but no convergence tests are reported (grid spacing, near-horizon starting point, order of the near-horizon expansion) and no error estimates are given for the extracted masses and widths. Because the negative values and multi-peak structure are the paper’s main new effect, it is essential to demonstrate that these features are not numerical artifacts and that the fit failures do not simply mark the breakdown of the approximation discussed above. A concrete robustness test would be to vary the near-horizon matching point and the radial g
- [Eq. (57) and Eq. (35)] The excellent agreement in Fig. 2 between the holographic masses and Eq. (57) is, at least in part, a consistency check rather than an independent confirmation. The near-horizon consistency condition (35) already yields omega_tilde = omega + (L_z + lambda) Omega, and the incoming-wave ansatz (25) is built with omega_tilde. The paper should clarify that the comparison verifies that the self-consistent near-horizon analysis and the boundary spectral extraction are compatible with the expected -Omega J_z shift, and should make explicit which parts of the shift are derived from the equations of motion rather than inserted by hand. Without this clarification, the abstract’s first main result could be read as tautological.
minor comments (4)
- [Sec. II, after Eq. (15)] Typo: 'allowing us to choice a classical transverse location' should be 'choose'.
- [Eq. (58)] The fit function has a dimensionful parameter a and an exponent b; please specify the dimensions explicitly so that the GeV^4 normalization on the right-hand side is unambiguous.
- [Sec. V.A, Fig. 2] The relation (57) is written for the energy omega, but the figure shows invariant mass M. Please state the conversion used to plot the solid lines, especially for nonzero q_z, so that the reader can reproduce the comparison.
- [Sec. V.B, Figs. 7 and 8] The captions mention 'small oscillations originate from numerical noise'. Please specify the numerical scheme, the grid resolution, and the tolerance used for the ODE integration; otherwise the reader cannot judge the significance of features that are of similar size to the noise.
Circularity Check
No significant circularity: the −ΩJ_z shift is an output of the near-horizon boundary-value problem, not a fitted parameter, and the quasi-classical (x,y)-freezing is an explicit approximation rather than a self-referential reduction.
full rationale
The central derivation is not circular. The peak shift −ΩJ_z is obtained from the near-horizon consistency condition: the ansatz (25), E = e^{-i\tilde\omega r_*}\psi, is a standard normal form, and the value \tilde\omega_\lambda \simeq \omega+(L_z+\lambda)\Omega is solved from the leading-order matrix condition (32) and displayed in Eq. (35). It is not a parameter fitted to the spectral functions; the full spectral functions are then obtained by numerical integration from the horizon to the boundary with the near-horizon initial data (38). Thus the masses and widths are outputs of the boundary-value problem. The only calibrated parameter is the soft-wall dilaton constant c=m_{J/\psi}^2/4, which fixes the zero-rotation mass but does not determine the Ω-dependence, the q_⊥ behavior, or the widths; consequently no fitted input is renamed as a prediction. The paper explicitly introduces the quasi-classical point-particle truncation in Sec. II (Eqs. (14)–(16)): the metric inhomogeneity is replaced by a fixed transverse location (x,y). This is an uncontrolled approximation when ΩL_z becomes comparable to |q|, as the skeptical review notes, and the paper itself acknowledges the resulting non-diagonal projected Green function and negative spectral weights (Sec. V.B, Figs. 7–8). But an uncontrolled or limited approximation is a correctness/robustness issue, not a circularity: the equations used to produce the shifts are not equivalent by construction to the result being claimed. Self-citations [63,64] are used for standard spectral-function methodology and comparison, not as load-bearing uniqueness or ansatz justification. No step in the paper reduces to its own input by definition, and no external benchmark is manufactured by fitting. Therefore the circularity score is 0.
Axiom & Free-Parameter Ledger
free parameters (2)
- soft-wall dilaton parameter c =
≈2.40 GeV^2 (m_J/ψ^2/4)
- Breit-Wigner fit parameters a, b in Eq. (58) =
fitted per configuration
axioms (6)
- domain assumption AdS/CFT correspondence: boundary current correlator is dual to bulk U(1) gauge field action (Sec. I, Eq. (1)).
- domain assumption Soft-wall model with dilaton Φ=cζ^2 and generalized Maxwell action describes J/ψ meson (Sec. II, Eq. (2)).
- domain assumption Global rotation is represented by the rotating-coordinate AdS-Schwarzschild metric (6) and a local inertial frame via vielbein (10).
- ad hoc to paper Quasi-classical plane-wave/point-particle approximation (Eqs. (14)–(15)) freezes the transverse location (x,y) and decouples Fourier modes.
- standard math Incoming-wave condition near the horizon selects the retarded Green function; outgoing modes are neglected (Sec. III).
- domain assumption Projecting the retarded Green function onto fixed-spin polarization vectors (51)–(53) yields meaningful spectral functions even when J_z and transverse momentum do not commute.
read the original abstract
We investigate the spectral functions of the $J/\psi$ meson in a rotating thermal background within the soft-wall holographic model. The global rotation is implemented through a rotating AdS-like metric, while a local inertial frame is introduced in which the vector field can be decomposed into different spin states. We solve the equations of motion of the vector field in the bulk with incoming wave condition near the horizon and compute the retarded Green function, from which we extract the invariant-mass spectral functions for $J/\psi$. When the momentum is parallel to the rotation axis, the peak energies shift by $-\Omega J_z$, as expected by a coupling between rotation and angular momentum, while the widths are nearly independent to $\Omega$. When the momentum is in perpendicular direction, the spectral functions for spin-$\pm1$ states deviate significantly from the single-peak behavior and the energy shifts depart from $-\Omega J_z$. The resulting triplet splittings of the spectral functions provides a holographic perspective on spin-dependent vector meson properties in rotating systems.
Figures
Reference graph
Works this paper leans on
-
[1]
In this paper, we quantify the bulk behavior of a quasi- classical vector meson with momentumqµ and located at (x, y)on the transverse plane. We will show later that such a meson has an energy shift of−(x×q+s)·Ωdue to the coupling between its total angular momentum and the global rotation, as predicted by classical theories. III. SOLUTION NEAR HORIZON Sim...
-
[2]
D. H. Rischke, Prog. Part. Nucl. Phys.52, 197 (2004), arXiv:nucl-th/0305030
Pith/arXiv arXiv 2004
-
[3]
M. Gyulassy and L. McLerran, Nucl. Phys. A750, 30 (2005), arXiv:nucl-th/0405013. 10
Pith/arXiv arXiv 2005
-
[4]
E. V. Shuryak, Nucl. Phys. A750, 64 (2005), arXiv:hep- ph/0405066
arXiv 2005
-
[5]
S. A. Voloshin, (2004), arXiv:nucl-th/0410089
Pith/arXiv arXiv 2004
-
[6]
Z.-T. Liang and X.-N. Wang, Phys. Lett. B629, 20 (2005), arXiv:nucl-th/0411101
Pith/arXiv arXiv 2005
-
[7]
Z.-T. Liang and X.-N. Wang, Phys. Rev. Lett.94, 102301 (2005), [Erratum: Phys.Rev.Lett. 96, 039901 (2006)], arXiv:nucl-th/0410079
Pith/arXiv arXiv 2005
-
[8]
N. Banerjee, J. Bhattacharya, S. Bhattacharyya, S. Dutta, R. Loganayagam, and P. Surowka, JHEP01, 094 (2011), arXiv:0809.2596 [hep-th]
Pith/arXiv arXiv 2011
-
[9]
M. Torabian and H.-U. Yee, JHEP08, 020 (2009), arXiv:0903.4894 [hep-th]
Pith/arXiv arXiv 2009
-
[10]
D. T. Son and P. Surowka, Phys. Rev. Lett.103, 191601 (2009), arXiv:0906.5044 [hep-th]
Pith/arXiv arXiv 2009
-
[11]
D. E. Kharzeev, J. Liao, S. A. Voloshin, and G. Wang, Prog. Part. Nucl. Phys.88, 1 (2016), arXiv:1511.04050 [hep-ph]
Pith/arXiv arXiv 2016
-
[12]
X.-G. Huang, K. Nishimura, and N. Yamamoto, JHEP 02, 069 (2018), arXiv:1711.02190 [hep-ph]
Pith/arXiv arXiv 2018
-
[13]
Y. Jiang, X.-G. Huang, and J. Liao, Phys. Rev. D92, 071501 (2015), arXiv:1504.03201 [hep-ph]
Pith/arXiv arXiv 2015
-
[14]
B. I. Abelevet al.(STAR), Phys. Rev. C76, 024915 (2007), [Erratum: Phys.Rev.C 95, 039906 (2017)], arXiv:0705.1691 [nucl-ex]
Pith/arXiv arXiv 2007
-
[15]
Adamczyket al.(STAR), Nature548, 62 (2017), arXiv:1701.06657 [nucl-ex]
L. Adamczyket al.(STAR), Nature548, 62 (2017), arXiv:1701.06657 [nucl-ex]
Pith/arXiv arXiv 2017
-
[16]
M. S. Abdallahet al.(STAR), Phys. Rev. C104, L061901 (2021), arXiv:2108.00044 [nucl-ex]
arXiv 2021
-
[17]
I. Karpenko and F. Becattini, Eur. Phys. J. C77, 213 (2017), arXiv:1610.04717 [nucl-th]
Pith/arXiv arXiv 2017
-
[18]
H. Li, L.-G. Pang, Q. Wang, and X.-L. Xia, Phys. Rev. C96, 054908 (2017), arXiv:1704.01507 [nucl-th]
Pith/arXiv arXiv 2017
-
[19]
Y. Guo, J. Liao, E. Wang, H. Xing, and H. Zhang, Phys. Rev. C104, L041902 (2021), arXiv:2105.13481 [nucl-th]
Pith/arXiv arXiv 2021
-
[20]
Y. Sun and C. M. Ko, Phys. Rev. C96, 024906 (2017), arXiv:1706.09467 [nucl-th]
Pith/arXiv arXiv 2017
-
[21]
F. Becattini, M. Buzzegoli, T. Niida, S. Pu, A.-H. Tang, and Q. Wang, Int. J. Mod. Phys. E33, 2430006 (2024), arXiv:2402.04540 [nucl-th]
Pith/arXiv arXiv 2024
-
[22]
M. S. Abdallahet al.(STAR), Nature614, 244 (2023), arXiv:2204.02302 [hep-ph]
arXiv 2023
-
[23]
Y.-G. Yang, R.-H. Fang, Q. Wang, and X.-N. Wang, Phys. Rev. C97, 034917 (2018), arXiv:1711.06008 [nucl- th]
Pith/arXiv arXiv 2018
-
[24]
X.-L. Sheng, L. Oliva, and Q. Wang, Phys. Rev. D 101, 096005 (2020), [Erratum: Phys.Rev.D 105, 099903 (2022)], arXiv:1910.13684 [nucl-th]
Pith/arXiv arXiv 2020
-
[25]
X.-L. Sheng, L. Oliva, Z.-T. Liang, Q. Wang, and X.-N. Wang, Phys. Rev. Lett.131, 042304 (2023), arXiv:2205.15689 [nucl-th]
Pith/arXiv arXiv 2023
-
[26]
X.-L. Sheng, S. Pu, and Q. Wang, Phys. Rev. C108, 054902 (2023), arXiv:2308.14038 [nucl-th]
Pith/arXiv arXiv 2023
-
[27]
J.-H. Chen, Z.-T. Liang, Y.-G. Ma, X.-L. Sheng, and Q. Wang, Sci. China Phys. Mech. Astron.68, 211001 (2025), arXiv:2407.06480 [hep-ph]
Pith/arXiv arXiv 2025
-
[28]
J. M. Maldacena, Adv. Theor. Math. Phys.2, 231 (1998), arXiv:hep-th/9711200
Pith/arXiv arXiv 1998
-
[29]
E. Witten, Adv. Theor. Math. Phys.2, 505 (1998), arXiv:hep-th/9803131
Pith/arXiv arXiv 1998
-
[30]
E. Witten, Adv. Theor. Math. Phys.2, 253 (1998), arXiv:hep-th/9802150
Pith/arXiv arXiv 1998
-
[31]
O. Aharony, S. S. Gubser, J. M. Maldacena, H. Ooguri, and Y. Oz, Phys. Rept.323, 183 (2000), arXiv:hep- th/9905111
arXiv 2000
- [32]
-
[33]
T. Sakai and S. Sugimoto, Prog. Theor. Phys.113, 843 (2005), arXiv:hep-th/0412141
Pith/arXiv arXiv 2005
-
[34]
T. Sakai and S. Sugimoto, Prog. Theor. Phys.114, 1083 (2005), arXiv:hep-th/0507073
Pith/arXiv arXiv 2005
-
[35]
A. Karch, E. Katz, D. T. Son, and M. A. Stephanov, Phys. Rev. D74, 015005 (2006), arXiv:hep-ph/0602229
Pith/arXiv arXiv 2006
-
[36]
T. Gherghetta, J. I. Kapusta, and T. M. Kelley, Phys. Rev. D79, 076003 (2009), arXiv:0902.1998 [hep-ph]
Pith/arXiv arXiv 2009
-
[37]
M. Fujita, K. Fukushima, T. Misumi, and M. Murata, Phys. Rev. D80, 035001 (2009), arXiv:0903.2316 [hep- ph]
Pith/arXiv arXiv 2009
-
[38]
L. A. H. Mamani, A. S. Miranda, H. Boschi-Filho, and N. R. F. Braga, JHEP2014, 1 (2014), arXiv:1312.3815 [hep-th]
Pith/arXiv arXiv 2014
-
[39]
N. R. F. Braga, L. F. Ferreira, and A. Vega, Phys. Lett. B774, 476 (2017), arXiv:1709.05326 [hep-ph]
Pith/arXiv arXiv 2017
- [40]
-
[41]
C. P. Herzog, Phys. Rev. Lett.98, 091601 (2007), arXiv:hep-th/0608151
Pith/arXiv arXiv 2007
-
[42]
O. Andreev, Phys. Rev. Lett.102, 212001 (2009), arXiv:0903.4375 [hep-ph]
Pith/arXiv arXiv 2009
-
[43]
O. Andreev and V. I. Zakharov, JHEP04, 100 (2007), arXiv:hep-ph/0611304
Pith/arXiv arXiv 2007
-
[44]
N. R. F. Braga, L. F. Faulhaber, and O. C. Junqueira, Phys. Rev. D105, 106003 (2022), arXiv:2201.05581 [hep- th]
Pith/arXiv arXiv 2022
-
[45]
X. Chen, L. Zhang, D. Li, D. Hou, and M. Huang, JHEP 07, 132 (2021), arXiv:2010.14478 [hep-ph]
Pith/arXiv arXiv 2021
-
[46]
J.-H. Wang and S.-Q. Feng, Phys. Rev. D109, 066019 (2024), arXiv:2403.01814 [hep-ph]
Pith/arXiv arXiv 2024
-
[47]
Y.-Q. Zhao, S. He, D. Hou, L. Li, and Z. Li, JHEP04, 115 (2023), arXiv:2212.14662 [hep-ph]
Pith/arXiv arXiv 2023
-
[48]
J.-X. Chen, S. Wang, D. Hou, and H.-C. Ren, Phys. Rev. D111, 026020 (2025), arXiv:2410.04763 [hep-ph]
Pith/arXiv arXiv 2025
-
[49]
S.-J. Rey, S. Theisen, and J.-T. Yee, Nucl. Phys. B527, 171 (1998), arXiv:hep-th/9803135
Pith/arXiv arXiv 1998
-
[50]
A. Brandhuber, N. Itzhaki, J. Sonnenschein, and S. Yankielowicz, Phys. Lett. B434, 36 (1998), arXiv:hep- th/9803137
arXiv 1998
-
[51]
R. Rougemont, R. Critelli, and J. Noronha, Phys. Rev. D91, 066001 (2015), arXiv:1409.0556 [hep-th]
Pith/arXiv arXiv 2015
-
[52]
Z.-q. Zhang, D.-f. Hou, and G. Chen, Eur. Phys. J. A 52, 357 (2016), arXiv:1607.03985 [hep-ph]
Pith/arXiv arXiv 2016
-
[53]
J.-X. Chen and D.-F. Hou, Eur. Phys. J. C84, 447 (2024), arXiv:2202.00888 [hep-ph]
Pith/arXiv arXiv 2024
-
[54]
H. Liu, K. Rajagopal, and U. A. Wiedemann, Phys. Rev. Lett.97, 182301 (2006), arXiv:hep-ph/0605178
Pith/arXiv arXiv 2006
-
[55]
C. P. Herzog, A. Karch, P. Kovtun, C. Kozcaz, and L. G. Yaffe, JHEP07, 013 (2006), arXiv:hep-th/0605158
Pith/arXiv arXiv 2006
-
[56]
D. Hou, M. Atashi, K. Bitaghsir Fadafan, and Z.-q. Zhang, Phys. Lett. B817, 136279 (2021)
2021
-
[57]
J.-X. Chen, D.-F. Hou, and H.-C. Ren, JHEP03, 171 (2024), arXiv:2308.08126 [hep-ph]
Pith/arXiv arXiv 2024
-
[58]
Z.-R. Zhu, J.-X. Chen, X.-M. Liu, and D. Hou, Eur. Phys. J. C82, 560 (2022), arXiv:2109.02366 [hep-ph]
Pith/arXiv arXiv 2022
-
[59]
D. T. Son and A. O. Starinets, JHEP09, 042 (2002), arXiv:hep-th/0205051
Pith/arXiv arXiv 2002
-
[60]
G. Policastro, D. T. Son, and A. O. Starinets, JHEP09, 043 (2002), arXiv:hep-th/0205052. 11
Pith/arXiv arXiv 2002
-
[61]
Kim, J.-P
Y. Kim, J.-P. Lee, and S. H. Lee, Physical Review D75, 114008 (2007)
2007
-
[62]
M. A. Martin Contreras, A. Vega, and S. Diles, Physical Review D103, 086008 (2021)
2021
-
[63]
Fujita, T
M. Fujita, T. Kikuchi, K. Fukushima, T. Misumi, and M. Murata, Physical Review D81, 065024 (2010)
2010
-
[64]
X.-L. Sheng, Y.-Q. Zhao, S.-W. Li, F. Becattini, and D. Hou, Phys. Rev. D110, 056047 (2024), arXiv:2403.07522 [hep-ph]
Pith/arXiv arXiv 2024
-
[65]
Y.-Q. Zhao, X.-L. Sheng, S.-W. Li, and D. Hou, JHEP 08, 070 (2024), arXiv:2403.07468 [hep-ph]
Pith/arXiv arXiv 2024
-
[66]
N. R. F. Braga and Y. F. Ferreira, Phys. Rev. D108, 094017 (2023), arXiv:2309.11643 [hep-ph]
Pith/arXiv arXiv 2023
-
[67]
Y.-Q. Zhao and D. Hou, Eur. Phys. J. C83, 1076 (2023), arXiv:2306.04318 [hep-ph]
Pith/arXiv arXiv 2023
-
[68]
Z.-R. Zhu, M. Sun, R. Zhou, Z. Ma, and J. Han, Eur. Phys. J. C84, 1252 (2024), arXiv:2406.19661 [hep-ph]
Pith/arXiv arXiv 2024
-
[69]
X.-L. Wang and S.-Q. Feng, Phys. Rev. D110, 086018 (2024), arXiv:2407.00627 [hep-ph]
Pith/arXiv arXiv 2024
-
[70]
Zhao and G
Z. Zhao and G. Yuan-xing, Chinese Astronomy and As- trophysics7, 201 (1983)
1983
-
[71]
Mashhoon, Physical review letters61, 2639 (1988)
B. Mashhoon, Physical review letters61, 2639 (1988)
1988
-
[72]
Mashhoon, R
B. Mashhoon, R. Neutze, M. Hannam, and G. E. Sted- man, Physics Letters A249, 161 (1998)
1998
-
[73]
F. W. Hehl and W.-T. Ni, Physical Review D42, 2045 (1990)
2045
-
[74]
Dataset for
X.-l. Sheng, J.-X. Chen, D. Hou, and H.-c. Ren, “Dataset for "spectral functions of$j/ψ$meson in rotating ther- mal background from holography",” (2026). Appendix A: Explicit expressions In this appendix, we collect explicit expressions of coefficient matrices appearing in Sec. III. The matricesT1,2,3 in Eq. (21) are given by T1 = ζ 4Q(ζ) L4 −1 0 0 0...
2026
discussion (0)
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