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Constraining the colored cc¯ energy loss from J/ψ production in p-A collisions

NUCLEAR PHYSICS AND INTERDISCIPLINARY RESEARCH

Constraining the colored cc¯ energy loss from J/ψ production in p-A collisions

Li-Hua Song
Lin-Wan Yan
Ying Liu
Nuclear Science and TechniquesVol.29, No.11Article number 159Published in print 01 Nov 2018Available online 27 Sep 2018
52000

Considering the volatility of the propagation path for charmonium passing across the nuclear target in J/ψ formation from p-A collisions, the charmonium energy loss is investigated using Salgado-Wiedemann quenching weights. A successful description regarding J/ψ suppression of RW(Fe)/Be(xF) from the E866 experiment for 0.2 < xF < 0.65 gives the transport coefficient q^=0.29±0.07 GeV2/fm for the colored cc¯ energy loss. The calculated result indicates that radiative energy loss of a parton should be independent of its mass at high energy. The calculations are further compared to LHC and RHIC measurements.

J/ψproductionenergy losscharm quarkgluon

1 Introduction

A wide range of phenomena observed from experiments on ultra-relativistic heavy-ion collisions suggests that the Quark-Gluon Plasma (QGP) has been founded [1, 2]. The suppression of J/ψ production as a result of Debye screening about heavy-quark potential at a finite temperature is a striking observable phenomenon from heavy-ion collisions which was expected as the signature of QGP formation [3, 4]. However, there are several other effects that can suppress the J/ψ yields from heavy-ion collisions for high energy [5, 6]. Among them, the energy loss effect from the particles when they go through a medium and experience collisions and eradiating gluons have received much attention. For quantifying of the properties of the QGP, it is necessary to constrain the values about the transport characteristic parameters for the cold nuclear medium by means of J/ψ formation from p-A collisions.

It is generally recognized that the process of J/ψ production from proton-nucleus collisions can be separated into three stages. As discussed in Ref. [7], the first is the perturbative (gluon fusion) production stage which leads to a colored cc¯ pair, which is followed by the emission or absorption of a further gluon, thereby inducing color neutrality and establishing the quarkonia produced as color singlets. In the final step, the nascent J/ψ evolves into a fully grown physical charmonium resonance. The nuclear effects responsible for the suppression of J/ψ formation generally contain the modifications of the nuclear parton densities, the energy loss experienced by the incoming proton or colored cc¯ pair when they traverse the nuclear medium, and the nuclear absorption about a cc¯ pair or resonances. Experiments involving a wide collision energy range from NA3 [8], E772 [9], E866 [10, 11], NA50 [12], HEAR-B [13], LHC [14, 15] and RHIC [16] have revealed the drastic nuclear suppression effects.

The conventional nuclear suppression mechanism is still an open question because of the existence of many competitive effects. There are several phenomenological models proposed separately on the basis of the nuclear absorption effect of the cc¯ pair [17, 18], the parton energy loss induced by parton multiple scattering in a nuclear medium [19-21], and a decrease of the overlap with the J/ψ wave function caused by the increase of the invariant mass for the cc¯ pair with multiple soft rescatterings when they traverse the nucleus [22]. It is generally recognized that when J/ψ formation occurs outside of the nuclear target, the cc¯ will maintain color for the entire path in the target nucleus. In this case, the color octet cc¯ loses energy due to the medium-induced gluon radiation when traversing the target nucleus. This induces a suppression of J/ψ formation.

It was determined from our previous work that the associated medium-induced energy loss is the main effect which leads to the J/ψ suppression for J/ψ formation which occurs outside the nuclear target [20, 21]. In this investigation, our aim is to extract the transport coefficient for charm quarks by fitting the acquired experimental data to J/ψ hadronization which arises outside the nucleus. The main improvements over previous works are twofold: using Salgado-Wiedemann (SW) quenching weights [23], our calculations include the probability that a charmonium can radiate an additional energy fraction ε in a cold nuclear medium due to scattering. In addition, we consider the volatility of the propagation path L of the charmonium passing across the nuclear target by averaging over the nuclear geometry. In view of the deviation between the modification of the parton distribution functions of the different sets, we consider the uncertainty that our calculated results originate from the nuclear parton densities by analyzing the uncertainties of the nuclear parton distribution functions.

We organization of this report is as follows: in Sect. 2, we will emphasize the introduction of the method adopted in this work for calculating the J/ψ formation cross-section from p-A collisions modified due to the charmonium energy loss. A presentation of the results obtained and discussion is provided in Sect. 3. Finally, we will end with a brief summary in Sect. 4.

2 The modification for charmonium energy loss

As discussed in our earlier articles [20, 21], when the distance L0 that the cc¯ peregrinates within the appropriate color neutralization time τ0 exceeds its passing length LA in the target nucleus, it will be colored for the whole path in the target nucleus. The cc¯ energy loss plays the main role in J/ψ suppression for the case that J/ψ formation occurs outside the nucleus. If a color octet cc¯ pair loses energy ε because of multiple scattering and gluon radiation, the energy loss ε will cause the rescaling of xF:

xF(E)xF(E+ε),xF=xF+ε/Ep. (1)

The distribution function D(ε) about the probability that a parton loses energy ε determines the nuclear modification induced by the colored cc¯ energy loss. According to Ref. [23], if we assume that the gluon emissions are independent, the probability distribution D(ε) can be expressed as:

D(ε)=n=01n![i=1ndωidI(ωi)dω]δ(εi=1nωi)exp[0+dωdI(ω)dω], (2)

Where dI(ω)/dω represents the spectrum of the medium-induced gluon and n is the gluon number radiated by the hard parton. The probability distribution D(ε) with a discrete and a continuous part is expressed as [24]:

D(ε)=p0δ(ε)+p(ε). (3)

Its normalization is unity.

The color evaporation model (CEM) [25] and non-relativistic QCD (NRQCD) are two successful formalisms [26] with incorporate the features of the process for J/ψ formation. Due to the formalism about NRQCD including more free parameters than CEM [27-31], we express the cross-section about J/ψ formation from p-A collisions based on the CEM formalism. With the probability ρJ/ψ of a cc¯ pair developing into a J/ψ state and the parton densities fi(x1,m2) (fi(x2,m2)) in proton (nucleon), dσp-A/dxF can be written as [32]:

dσpAdxF(xF)=ρJ/ψ2mc2mDdm2mxF2s+4m2×[fg(x1,m2)fg(x2,m2)σgg(mc2)+q=u,d,s{fq(x1,m2)fq¯(x2,m2)+fq¯(x1,m2)fq(x2,m2)}σqq¯(mc2)]. (4)

As expressed in Ref. [20, 21], the leading order cross-section about the cc¯ partonic production formed by the amalgamation of gluons or the annihilation of quark-antiquark is respectively σgg or σqq¯.

Considering the modification due to cc¯ energy loss with the probability D(ε), the J/ψ formation cross-section thus becomes

dσ'pAdxF(xF)=0εmaxdεD(ε)dσpAdxF(xF). (5)

In the previous formula, x1,2=12[xF2(1τ)2+4τ±xF(1τ)] (τ=m2s) takes place x1,2 in equation 4, respectively. In our calculations, the integral over ε is bounded by εmax = min(Ep-E, E), and we use the Salgado-Wiedemann (SW) quenching weights for the probability distribution D(ε), which are obtained based on multiple soft and single hard scattering approximations and available as a FORTRAN routine [33].

The SW quenching weight returns results for a quark with m/E traversing a medium with transport coefficient q^ (it determines the transport properties of the so-called cold nuclear matter) and length L. In view of the fluctuations of the path length L traveled by the cc¯ through the target nucleus, we consider the geometry of J/ψ formation in this process. As displayed in Fig.1, we suppose that the target nucleus is located at (0,0), and at (b,y) the cc¯ pair is formed. Thus, the path length L that the cc¯ pair propagates along in accordance with the direction of the impact parameter b can be expressed as L=RA2b2y (RA=1.12A1/3, where y represents the coordinate along direction of the cc¯.) [34]. It is worth mentioning that the collisions of the nucleons are not polarized, and do not rely on the direction. As such, the expression of the path length L does not depend on the direction of the cc¯ pair. The J/ψ formation cross-section dσp-A/dxF which contains the modification of the nuclear geometry effect, can be expressed as:

Fig. 1.
Demonstration of the geometry of J/ψ formation from p-A collisions.
pic
dσpAdxF(xF)=d2bdyρA(b,y)dσpAdxF(xF). (6)

In the preceding formula, the y is from RA2b2 to RA2b2, and the nuclear density distribution ρA(b,y) is normalized to unity (ρA(b2+y2)=(ρ0/A)Θ(RAb2+y2)) [35-37].

The effect of the incident proton can decrease the center-mass system energy of the nucleon-nucleon collision for producing the cc¯. As such, the momentum fraction becomes xF rescaled again [38]:

xF=rsxF=rs(xF+ε/Ep), (7)

with rs=s/s, s=s(n1)s, and n denoting the number of collisions for the incident proton with the nucleons in the nuclear target. Based on the Glauber model [39], the J/ψ formation cross section for p-A collisions is ultimately:

dσpAdxF=n=1AP(n)dσpA(n)dxF(xF). (8)

In the preceding formula, dσpA(n)dxF(xF)=dσpAdxF(xF) denotes the J/ψ production cross-section in the nth collision, and the probability P(n) of the projectile proton scattering inelastically on the nuclear target for possessing n collisions with nucleons is given as:

P(n)=dbP(n,b)n=1AdbP(n,b), (9)

with P(n,b)=A!n!(An)![T(b)σin]n[1T(b)σin]An. According to Ref. [40], for A ≤ 32 the thickness function T(b)=12πβA2exp(b2/2βA2), T(b)=32πRA3RA2b2θ(RA|b|) for A > 32. See details in Ref. [20, 21].

3 Results and discussion

In order to facilitate the theoretical investigation of the parton energy loss in cold nuclear matter, the extraction of the value of the transport coefficient q^ about the charmonium energy loss by means of J/ψ formation experimental data is necessary. The transport coefficient q^ determines the amount about the medium-induced gluon radiation and the J/ψ suppression strength. In view of Ref. [41], if an appropriate color neutralization time τ0=0.25 fm is assumed, then L0>LA for xF > 0 with s=40 GeV. This indicates that the cc¯ will be colored along its entire path at E866 energy for xF>0. Therefore, the E866 experimental data for J/ψ production provides a reliable approach for investigating the colored cc¯ energy loss. To constrain the transport coefficient q^ about the colored cc¯ energy loss, we perform the calculation about the J/ψ formation cross-section ratios RW(Fe)/Be(xF):

RW(Fe)/Be(xF)=dσpW(Fe)dxF/dσpBedxF (10)

at E866 energy.

Using the CERN subroutine MINUIT [42], based on the minimization of the function of χ2, the transport coefficient q^ for cc¯ energy loss is extracted. Table 1 shows the values of the transport coefficient q^ and corresponding χ2/ndf obtained from the data of the E866 experiment on J/ψ production in different xF intervals. With an increase of χ2 by 1 unit from its minimum χmin2, we allow one standard deviation of the parameter from the central fit. In our calculation, the SW quenching weights[23] was used to describe the probability distribution for cc¯ energy loss, and utilize EPS09 nuclear parton densities [43] and CTEQ6L proton parton distributions [44], and s= 0.18GeV which originates in the energy loss of the incident proton [45].

Table 1:
q^ for cc¯ energy loss and χ2/ndf constrained by fitting E866 data on RW(Fe)/Be(xF).
xF No.data q^ (GeV2/fm) χ2/ndf
0.20<xF<0.65 18 0.29±0.07 0.73
.30<xF<0.95 26 0.31±0.05 10.80
.20<xF<0.95 44 0.29±0.05 7.21
Show more

From Table 1, we can see that the theoretical results for the middle xF region (0.2 < xF < 0.65) agree well with the data for q^=0.29±0.07 GeV2/fm and the corresponding χ2/ndf=0.73, and for the region including the large xF (0.3 < xF < 0.95) the calculated results greatly deviate from the experimental data (q^=0.31±0.05 GeV2/fm, χ2=10.80). The reason may be that nuclear absorption effect plays a role in the suppression of J/ψ formation for large xF region, which hinders the exact constraint of the transport coefficient q^. This provides the insight that we should use the experimental data for the middle xF region to constrain the massive parton energy loss from the J/ψ formation. Then, q^=0.29±0.07 GeV2/fm is the determined value. By comparing with the value q^=0.32±0.04 GeV2/fm obtained from the nuclear Drell-Yan data with SW quenching weights [46], we find that these two values are nearly equal. This indicates that the radiative energy loss of a parton should become independent of its mass at high energy, as discussed in Armesto et al. [47] and in the earlier Dokshitzer-Kharzeev article [48].

In addition, the origin of the uncertainty with respect to our calculated results may originate from the uncertainty of the nuclear parton distribution functions especially for the nuclear modification of gluon densities. Recently, the K. J. Eskola etal. group proposes a new set of nuclear parton distribution functions EPPS16 [49], which initially imposed constraints on the experimental data from LHC proton-lead collisions and provided the uncertainty estimates from the central fit for each flavor. The comparison of the calculated results RW(Fe)/Be(xF) modified only by the nuclear effects of the parton distribution functions from the EPPS16 (dashed lines) and EPS09 (solid lines) are shown in Fig.2. It is found that for E866 energy (s=38.79 GeV)the difference between the results obtained using the EPPS16 and EPS09 is very small. Moreover, for RHIC energy (s=200.0 GeV), the difference is slightly obvious in the region y < -1.5, and for LHC energy (s=5.0 TeV) the difference becomes increasingly obvious with the increase of y in the range y > 0. From Fig.2, we also can see that the tendency of the solid and dashed lines are almost identical with the increase of xF or y. By means of the EPPS16 nuclear parton distribution functions, the transport coefficient q^ for the colored cc¯ energy loss extracted from the E866 experimental data in the middle xF region (0.20 < xF < 0.65) is also q^=0.29±0.05 GeV2/fm (according to the central fit of EPPS16). The errors of q^ which originate from the uncertainty of EPPS16 are analyzed: q^=0.33±0.04 GeV2/fm according to the EPPS16 error sets S1 and q^=0.26±0.05 GeV2/fm according to error sets S1+.

Fig. 2.
A comparison of the calculated results modified only by the nuclear effects of the parton distributions from EPPS16 (dashed lines) and EPS09 ( solid lines)
pic

To intuitively display the charmonium energy loss effect on the J/ψ formation cross-section ratio in p-A collisions by means of the values of the transport coefficient q^ shown in Table 1, our numeric results are compared with the corresponding E866 experimental data in Fig.3 (0.20 < xF < 0.65) and Fig.4 (0.30 < xF < 0.95). The J/ψ predictions displayed by the solid curves are obtained with the consideration of the nuclear effects of parton distributions and the energy loss effects of the incident proton and the color octet cc¯. The tendency of the solid lines in Fig.3 and Fig.4 indicates that the theoretical results associated with the charmonium energy loss effect agree well with the experimental data. This implies that the effect of the cc¯ energy loss mainly contributes to the J/ψ suppression for hadronization occurring outside the nucleus.

Fig. 3.
E866 J/ψ suppression data for the range 0.2 < xF < 0.65 in p-W(Fe) collisions [10, 11] compared to the energy loss model. The theoretical results for the nuclear effects of the quark (quark and gluon) density and the incident proton energy loss effect are represented by the dotted (dashed) lines, and the solid curves represent the calculations including the two aforementioned effects and the cc¯ energy loss effect. Error bars represent the statistical uncertainty.
pic
Fig. 4.
E866 J/ψ suppression data for the range 0.3 < xF < 0.95 in p-W(Fe) collisions [10, 11] compared to the energy loss model. The other comments are the same as those in Fig. 3.
pic

In order to constrain the influence of the cc¯ energy loss on RW(Fe)/Be(xF), in Fig.3 and Fig.4 we provide the dashed lines which correspond only to the calculations with the nuclear effects on the parton distribution functions and the energy loss of the proton beam. In Fig.3, the comparison between the J/ψ predictions with (solid line) and without (dashed line) cc¯ energy loss shows that the strength of the J/ψ suppression in p-W (p-Fe) collisions induced by cc¯ energy loss is approximately equal in the range 0.20 < xF < 0.65. Nevertheless, in Fig.4, the comparison between the trend of the solid and dashed lines displays that the nuclear suppression on RW/Be(xF) and RFe/Be(xF) due to cc¯ energy loss decreases gradually with the increase of xF in the range 0.65 < xF < 0.80 and further reduces slowly in xF > 0.80. For Fig.3, from the gap between the solid and dashed lines, we can also determine that the suppression strength for RW/Be(xF) is about 10%, which is larger than that (approximately 5%) of RFe/Be(xF). The comparison between the J/ψ predictions as indicated by the solid line for RW/Be(xF) and that for RFe/Be(xF) reveal that the energy loss of the charmonium plays a more important role in the suppression of J/ψ cross-section ratios RW/Be(xF) than RFe/Be(xF). This indicates that the effect of the color octet cc¯ energy loss should be extremely important for large targets. The same conclusion can be drawn from Fig.4.

In addition, for investigating the nuclear effects of gluon distribution functions on J/ψ suppression, we describe the theoretical results with only the nuclear modification of quark distributions and energy loss of the proton beam as the dotted lines in Fig.3 and Fig.4. It can be seen that the difference between the dotted and dashed lines is small, especially for the range xF > 0.7, which means that the nuclear effects of the gluon distributions in the nucleon have little influence on J/ψ suppression within the middle and large xF range (0.2 < xF < 0.95) for E866 energy (Ep=800 GeV).

Furthermore, with xF=2ms sinh y and E=Epeym/s, J/ψ the formation cross-section ratios with y as a variable are calculated for RHIC (s=200 GeV) and LHC (s=5.0 TeV) experimental data. The energy loss ε of the octet cc¯ also causes rescaling of the variable y:

y=y+ln(E+εE), (11)

and then

x1=msey,x2=msey. (12)

Considering the nuclear geometry effect of the length that the colored cc¯ passes through in the nuclear target and using SW quenching weights, the theoretical results RAu/d(y) modified by this colored cc¯ energy loss model are compared with the RHIC [16] experimental data in Fig. 5. The theoretical result obtained by the nuclear modification of the parton distribution functions and the energy loss effects of the proton beam and the color octet cc¯ (q^=0.29±0.07 GeV2/fm) is shown as the solid line. The tendency of the solid curve steeply decreases with the increase of y in the range y < 0.5 and decrease gradually in the range 0.5 < y < 2.4. The dashed lines correspond to calculations only with the nuclear effects on the quark and gluon distribution functions and the energy loss of the proton beam. The drift of the dashed profile shows an obvious flat behavior in the range y < -1.5, and then decrease with the increase of y, which is approximately consistent with the solid line. In addition, the calculated results of RAu/d(y) containing the modification induced by the nuclear effect of the gluon density shows an enhancement in the range y < -0.5. The physical reason may be that the gluon anti-shadowing effect induces the enhancement in this coverage. From Fig. 5, we can see that there is a small gap between the solid and dashed lines and it becomes smaller with an increase of y. In addition, the two curves coincide at approximately y > 2.0. This means that the suppression of the J/ψ production caused by the energy loss of the colored cc¯ is small.

Fig. 5.
J/ψ suppression data from d-Au collisions for the range -2.2 < y < 2.4 at RHIC [16] compared to the energy loss model. The other comments are the same as those in Fig. 3.
pic

Furthermore, in order to discuss the suppression induced by the nuclear modification from the gluon distributions on J/ψ production for high energy, the dotted line denotes the theoretical result with only the nuclear effects of the quark distribution functions and energy loss of proton beam is given in Fig. 5. The tendency of the dotted line is nearly flat with the increase of y in the region -2.2 < y < 2.4. The small suppression (about 3%) due to the nuclear modification of the quark distributions and energy loss of the proton beam implies that for RHIC energy, the incident proton energy loss in the initial state and the nuclear effects of the quark distribution functions have little influence on J/ψ production in the range -2.2 < y < 2.4. However, the large deviation between the dashed and dotted lines mean that the nuclear effects of gluon distributions in the nucleus play the main role in the J/ψ production at RHIC energy in the region -2.2 < y < 2.4.

In Fig.6, we compare our calculated results based on this energy loss model with the J/ψ suppression data for the range -4.46 < y < 3.53 in p-Pb collisions from ALICE [14] (LHCb [15] ) at LHC energy. The solid line indicates the theoretical result obtained by the nuclear modification of the parton distribution functions and the energy loss effects of the proton beam and the color octet cc¯ (q^=0.29±0.07 GeV2/fm). From Fig.6, we can see that RPb/p(y) described by the solid line transitions into a trend indicating an enhancement in y < -3.53 and decrease with the increase of y in -4.46 < y < 3.53. The calculation with the nuclear modification on parton densities and the energy loss effect of the incoming proton is described as the dashed curve. The tendency of the dashed profile displays a high similarity with that of the solid line. There is an enhancement in the range -4.4 < y < -3.8 both in the solid and dashed lines which contain the modification induced by the nuclear effect of the gluon distribution functions, which would be induced by the gluon anti-shadowing effect in this coverage. In Fig. 6, it is shown that the solid and dashed curves nearly coincide at about y < -3.0, and there is a small gap between them in the range y > -3.0. Moreover, the gap is almost equal to the increase of y for y > -3.0. This implies that the energy loss effect of the colored cc¯ has little influence on the suppression of the J/ψ production.

Fig. 6.
J/ψ suppression data from p-Pb collisions in the range -4.46 < y < 3.53 from ALICE [14] (LHCb [15] ) at LHC compared to the energy loss model. The other comments are the same as those in Fig. 3.
pic

In addition, the calculated result with only the nuclear effect of the quark distribution functions and the energy loss effect of the incoming proton is displayed as the dotted line in Fig. 6. The dotted line is approximately equal to 1.0 with the increase of y in -4.46 < y < 3.53. The suppression induced by the nuclear effects of the quark distribution functions and energy loss effect of the incoming proton can be ignored (about 1%). This indicates that at the LHC energy, the incident proton energy loss in the initial state and the nuclear effects of the quark distribution functions have little influence on the calculations related to the suppression of the J/ψ production in -4.46 < y < 3.53. Nevertheless, the significant deviation from the dashed and dotted curves indicate that the nuclear modification of the gluon distribution functions in nucleon has a dominant role on the J/ψ suppression at LHC energy in the region -4.46 < y < 3.53. As displayed in Ref. [38], the nuclear modification of the gluon distribution function given by the different nuclear parton distribution sets exhibit obvious distinction. Therefore, operating precise measurements on nuclear parton distribution functions can help to exactly constrain the charmonium energy loss in cold nuclear matter at high energies such as RHIC and LHC energy.

Finally, as shown in Fig.5 and Fig.6, for the small kinematic coverage of LHC [14,15] (-7.31 × 10-2 < xF < 7.31 × 10-2) and RHIC[16](-8.70 × 10-2 < xF < 0.125) experiments, the nuclear effects of gluon distributions in the nucleus play the main role on J/ψ suppression. This further supports intuitively the prediction that the gluon shadowing or gluon saturation could cause J/ψ suppression for small xF region at high energy. For LHC and RHIC energy, the effect of the proton energy loss should be negligible since the proton energy in the nuclear rest frame is extremely large.

4 Summary

The experiment on J/ψ formation from proton-nucleus collisions provides a good environment to test the microscopic dynamics of medium-induced charmonium energy loss. Considering the volatility of the propagation path for the charmonium traversing the nuclear target, the charmonium energy loss is investigated using SW quenching weights. Based on the CERN subroutine MINUIT, by minimization of the function of χ2, the transport coefficient q^ for cc¯ energy loss is determined by fitting the data for 0.2 < xF < 0.65: q^=0.29±0.07 GeV2/fm with χ2/ndf=0.73. By comparing with the value q^=0.32±0.04 GeV2/fm obtained from the nuclear Drell-Yan data with SW quenching weights, we determined that these two values are nearly equal. This indicates that radiative energy loss of a parton should become independent of its mass at high energy. In addition, in view of the deviation between the modification of the parton distribution functions of the different sets, we consider the uncertainty of our calculated results originating from the nuclear parton densities by analyzing the uncertainties of the nuclear parton distribution functions. Based on the recent EPPS16 parton distribution set, the errors of q^ from the uncertainty of the recent EPPS16 sets are calculated: q^=0.33±0.04 GeV2/fm according to EPPS16 error sets S1 and q^=0.26±0.05 GeV2/fm according to S1+. With the central fit of EPPS16, the value of q^ is extracted from the E866 experimental data for the region 0.20 < xF < 0.65 is still q^=0.29±0.05 GeV2/fm. By comparing with the data at RHIC and LHC, we find that for the small kinematic coverage of LHC (-7.31 × 10-2 < xF < 7.31 × 10-2) and RHIC(-8.70 × 10-2 < xF < 0.125) experiment, the nuclear effects of gluon distributions in the nucleus play the main role in J/ψ suppression. In addition, due to the gigantic proton energy, the energy loss effect of proton beam has little influence. Therefore, to further exactly constrain the charmonium energy loss in cold nuclear medium, in the future, it would be desirable to perform precise measurements on J/ψ suppression from p-A collisions for middle xF kinematic coverage.

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