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High-
$ p_{\rm T} $ prompt photons mainly arise from two possible mechanisms in hadronic collisions, produced directly in the hard sub-processes referred to as "direct" photons or fragmented from an energetic parton. We consider that the NLO-inclusive cross-section for the production of prompt photons with transverse momentum$ p_{\rm T}^{\gamma} $ is given by the sum of the fragmentation and direct contributions, written as [1, 50],$ \begin{split} \sigma\left(p_{\rm T}^{\gamma}\right)=&\hat{\sigma}^D\left(p_{\rm T}^{\gamma};\mu;M;M_F\right)\\ &+\sum\limits_k\int_0^1\frac{{\rm d}z}{z}\hat{\sigma}^F\left(p_{\rm T}^{\gamma}/z;\mu;M;M_F\right)D_k^{\gamma}\left(z;M_F\right), \end{split} $
(1) where
$ \mu $ is the renormalization scale,$ M $ is the initial state factorization scale, and$ M_F $ is an arbitrary final state fragmentation scale. The contribution$ \hat{\sigma}^F $ denotes the partonic cross-section for producing a parton convoluted with the PDF of the incoming proton, and$ D_k^{\gamma} $ is the fragmentation function of a parton$ k $ (quarks, anti-quarks, and gluon) into a photon.$ \hat{\sigma}^D $ includes the partonic cross-section for producing a direct photon and the corresponding PDFs. Experimentally, there are also secondary photons originated from hadron decay during the collisions, and therefore an isolation cut would be applied for the substantial production of photons. A photon is isolated if the amount of deposited hadronic transverse energy$ E_{\rm T} $ is not more than a specific upper limit$ E_{\rm T}^{\rm iso} $ in a fixed radius$ R_{\rm iso}=\sqrt{(\eta-\eta_\gamma)^2+(\phi-\phi_\gamma)^2} $ in pseudo-rapidity and azimuthal angle around the photon direction. This restriction on the yields of isolated photons could not only reject the secondary decay photons, but also reduce the contribution from fragmentation processes. In the following, we focus on the production of isolated photons and isolated photon-tagged jets in hadronic collisions.We calculate isolated photon and jet productions in proton-proton collisions at 8 TeV using the JETPHOX NLO pQCD program [1, 49, 50] with CT14 nPDFs [41] in accordance with the ATLAS experiment [16]. The isolated energy cut for a photon has been set as
$ E_{ \rm T}^{ \rm iso}<6 $ GeV, and the isolated cone of radius in the pseudo-rapidity and azimuthal angle plane is$ R_{\rm cone}=0.4 $ . Moreover, photons are selected if their transverse momentum$ p_{\rm T}^{\gamma}>130 {\rm GeV} $ and$ |\eta^{\gamma}|<2.37 $ , except for$ 1.37<|\eta^{\gamma}|<1.56 $ . Jets are reconstructed by the anti-$ k_{t} $ algorithm with cone size$ R=0.6 $ and$ p_{\rm T}^{\rm jet}>100 {\rm GeV} $ and$ |\eta^{\rm jet}|<4.4 $ . In Fig. 1, we calculate the differential cross-section$ {\rm d}\sigma/{\rm d}p_{\rm T}^{\gamma} $ up to$ p_{\rm T}^{\gamma}=1 $ TeV in proton-proton collisions at$ \rm 8 $ TeV, and our theoretical predication shows good agreement with the ATLAS experimental results. -
The inclusive cross-section for the isolated photon production in proton-nucleus collisions could be evaluated by using nPDFs as substitutes for free-nucleon PDFs in the collinear factorization framework as stated above, which could effectively include different CNM effects.
In our calculations, we obtain the nPDFs
$ f_i^A(x, Q^2) $ by multiplying the CT14 PDFs [41] with a flavor- and scale-dependent factor$ R_i^A(x, Q^2) $ taken from four different parameterizations, DSSZ [34], EPPS16 [35], nCTEQ15 [42], and nIMParton [43]. These four parameterizations for the nPDFs are similar, in that they categorize CNM effects with Bjorken x region into shadowing, anti-shadowing, EMC effect, and so on, but differ in the specific formalisms and parameters for describing the CNM effects and the input experimental data used in the global fits. DSSZ, nCTEQ15, and EPPS16 could be convoluted in the expression for calculating the photon production at NLO, because they are also quantified in the NLO pQCD framework. The LO results for photon production are applied with nIMParton parameterization to maintain the consistency of the analysis.The nuclear modification factors in proton+lead collisions are defined as:
$ R_{\rm pPb}=\frac{{\rm d}\sigma^{\rm pPb}/{\rm d}p_{\rm T}}{\langle N_{\rm coll}\rangle {\rm d}\sigma^{\rm pp}/{\rm d}p_{\rm T}} $
(2) with
$ \langle N_{\rm coll}\rangle $ representing the number of binary nucleon-nucleon collisions by the Glauber model [51].Now we can make our theoretical predictions for the isolated prompt photon production in p
$ + $ p and p$ + $ Pb collisions at the very forward rapidity region$ \rm 3<\eta^{\gamma}<4 $ at$ \rm \sqrt{s_{NN}}=8.16 $ TeV with ATLAS isolated cuts for photons [16], along with the photon transverse momentum constrained in the range$ 40~{\rm GeV}<p_{\rm T}^{\gamma}<300~{\rm GeV} $ . We display the nuclear modification ratio$ R_{\rm pPb}^{\gamma} $ as a function of$ p_{\rm T}^{\gamma} $ in the upper panel of Fig. 2. The momentum fraction carried by the initial parton from the incoming particle can be approximately estimated to LO as$ x_{1, 2}= $ $\displaystyle\frac{p_{\rm T}}{\sqrt{s_{NN}}}\left({ e}^{\pm y_1}+{e}^{\pm y_2}\right) $ , where$ x_1\left(x_p\right) $ is the initial parton coming from the proton in the$ +z $ direction,$ x_2(x_{\rm pb}) $ is the initial parton coming from lead in the$ -z $ direction in$ \rm p+Pb $ collisions, and$ y_{1, 2} $ is the rapidity of$ \gamma $ and the associated jet respectively. The estimated average Bjorken$ \langle x_{\rm Pb}\rangle $ has been defined as the event's average value of Bjorken$ x_{\rm Pb} $ in the JetPhox simulation. In the bottom panel of Fig. 2, we show the estimation of the parton's average momentum fraction off-nucleus based on NLO results in JETPHOX. We have checked that$ \langle x_{\rm Pb}\rangle $ for the nPDF parameterizations vary slightly from each other. We can see that the average Bjorken$ \langle x_{\rm Pb}\rangle $ is lower than 0.055 at the very forward rapidity region, which represents the shadowing effect dominating the CNM effects. Moreover, the average Bjorken$ \langle x_{\rm Pb}\rangle $ has a positive linear dependence with$ p_{\rm T}^{\gamma} $ expected in its LO estimation.Figure 2. (color online) (Upper) Comparison between the nuclear modification ratios
$R_{\rm pPb}$ for p-Pb collisions at$\sqrt{s}$ = 8.16 TeV and$\rm 3 < \eta^{\gamma} < 4$ using the nCTEQ15, EPPS16, DSSZ, and nIMParton nuclear modifications and the CT14 free-proton PDFs. (Bottom) Corresponding average Bjorken$\langle x_{\rm Pb}\rangle$ as function of$ p_{\rm T}^{\gamma}$ .In Fig. 2, we see that the shadowing effect of DSSZ is unremarkable on the suppression of isolated photon production in p
$ + $ Pb collisions when the average Bjorken$ \langle x_{\rm Pb}\rangle<0.055 $ . We also notice that DSSZ's$ R_{\rm pPb}^{\gamma}(p_{\rm T}^{\gamma}) $ shows a very weak$ p_{\rm T}^{\gamma} $ dependence, which means its shadowing effect is nearly independent of the photon's transverse momentum in DSSZ at the forward rapidity region. Meanwhile the other three parameterizations' shadowing effects decrease with$ p_{\rm T}^{\gamma} $ increasing upon$ 3<\eta^{\gamma}<4 $ . Additionally, we observe that the shadowing of the brand-new nPDF parametrization, nIMParton, is only weaker than that of nCTEQ15 in our discussion.In Fig. 3, a similar phenomenon of the positively linear correlation between
$ \langle x_{\rm Pb}\rangle $ and$ p_{\rm T}^{\gamma} $ has been shown at backward rapidity$ -4<\eta^{\gamma}<-3 $ . However, the estimated average Bjorken$ \langle x_{\rm Pb}\rangle $ ranges from 0.25 to 0.8, which mostly correspond to the EMC effect. We could go a little further to distinguish the EMC maxima of the four different parameterizations from each nuclear modification factor's extreme point. For example, nIMParton's EMC minimum appears at$ p_{\rm T}^{\gamma}=150 $ GeV and the corresponding average Bjorken is located around$ \langle x_{\rm Pb}\rangle=0.5 $ , which is the lowest in our results. We further investigate the correlations between$ x_{\rm Pb} $ and$ p_{\rm T}^{\gamma} $ at both forward and backward rapidities to NLO, as shown in Fig. 4. We observe the broadening of Bjorken$ x_{\rm Pb} $ at a specific$ p_{\rm T}^{\gamma} $ interval owing to higher corrections, and the spreading of$ x_{\rm Pb} $ at small$ p_{\rm T}^{\gamma} $ is rather wider. Additionally, we can see a very dense statistics cluster around the low$ p_{\rm T}^{\gamma} $ in our Monte-Carlo simulation, because of the possibility distribution of the hard subprocesses for the photon production following double-logarithmic declining with the photon transverse momentum.Figure 3. (color online) Same as Fig. 2, except at backward rapidity
$\rm -4 < \eta^{\gamma} < -3$ .Figure 4. (color online) (Left) NLO fluctuations at forward rapidity
$ \rm 3<\eta^{\gamma}<4 $ ; (Right) NLO fluctuations at backward rapidity$ -4<\eta^{\gamma}<-3 $ .Noting that the nuclear modification factor is sensitive to the nPDF and p+p baseline [52], we may calculate the ratio of the photon production at forward and backward rapidity; this could eliminate the large uncertainty in the free-nucleon PDFs, which could be used to probe the CNM effects with less arbitrariness [12-14]. We define the forward-backward yield asymmetry as:
$ Y_{\rm p Pb}^{\rm asym}=\frac{{\rm d}\sigma/{\rm d}p_T({\rm p+Pb} \rightarrow \gamma+X)|_{\eta\in[\eta_1, \eta_2]}}{{\rm d}\sigma/{\rm d}p_{\rm T}({\rm p+Pb} \rightarrow \gamma+X)|_{\eta\in[-\eta_2, -\eta_1]}} . $
(3) Our predictions of the forward-to-backward yield asymmetries
$ Y_{\rm pPb}^{\rm asym} $ for the isolated prompt photon production in p+Pb collisions at$ \rm \sqrt{s}=8.16 $ TeV and$ \rm 3 < |\eta^{\gamma}| < $ 4 are shown in Fig. 5. As a result of the symmetry of the colliding system, there is nearly no forward-to-backward yield asymmetry observed in proton-proton collisions.$ Y_{\rm pPb}^{\rm asym} $ is larger than one in p+Pb collisions, which means the photon production suffers more suppression in the backward-rapidity region. Overall, the EMC effect reduces the photon production more effectively than the shadowing effect does. Moreover, we notice that the value of$ Y_{\rm pPb}^{\rm asym} $ starts decreasing to one with all parameterizations owing to the decreasing of the EMC effect at relatively high$ p_{\rm T}^{\gamma} $ . This manifestation seems less obvious in nCTEQ15, as its EMC maximum is close to the highest boundary of$ p_{\rm T}^{\gamma} $ and our approximate curve fitting.Figure 5. (color online) Comparison between the forward-to-backward asymmetry
$\rm Y_{asym}$ for p-Pb collisions at$\sqrt{s_{NN}}$ = 8.16 TeV and$\rm 3 < \eta^{\gamma} < 4$ using the nCTEQ15, EPPS16, DSSZ, and nIMParton nuclear modifications and the CT14 free-proton PDFs.In order to further explore the impact of input nuclear modifications on the cross-section of isolated prompt photon productions in proton-nucleus collisions, we further discuss the isolated photon's nuclear modification factor
$ R_{\rm pPb}^{\gamma}(\eta^{\gamma}) $ as a function of the photon's rapidity$ \eta^{\gamma} $ at both forward and backward rapidities. The Fig. 6 shows a growing suppression of the photon productions from DSSZ, EPPS16, nIMParton, and nCTEQ15 at forward pseudo-rapidity, which quantitatively appears in accordance with the$ R_{\rm pPb}^{\gamma}(p_{\rm T}^{\gamma}) $ at$ p_{\rm T}^{\gamma}=50~{\rm GeV} $ owing to the highest statistics at the lowest-$ p_{\rm T}^{\gamma} $ region in the Monte-Carlo simulations exhibited above in Fig. 2. However,$ R_{\rm pPb}^{\gamma}(\eta^{\gamma}) $ shows very weak$ \eta^{\gamma} $ dependence, because the variation of Bjorken$ x_{\rm Pb} $ is at the magnitude of$ 10^{-3} $ in the$ 3<\eta^{\gamma}<4 $ region, shown at the bottom of Fig. 6. Combining the results of$ R_{\rm pPb} $ evolved with$ p_{\rm T}^{\gamma} $ and$ \eta^{\gamma} $ , the suppression pattern of isolated photons could be quantitatively analyzed through$ \langle x_{\rm Pb}\rangle $ at both forward and backward rapidities. In Fig. 7, the nuclear modification factors using the four different nPDFs all show a nearly positive linear relation with$ \eta^{\gamma} $ , the values of which agree with$ R_{\rm pPb}^{\gamma}(p_{\rm T}^{\gamma}) $ through the average Bjorken$ \langle x_{\rm Pb}\rangle $ , as shown in Fig. 7 and Fig. 3, respectively. The nCTEQ15 parameterization gives a stronger suppression than the others, which could be confirmed in the prediction of$ R_{\rm pPb}^{\gamma}\left(p_{\rm T}^{\gamma}\right) $ at the low-$ p_{\rm T}^{\gamma} $ region in Fig. 3.Figure 6. (color online) Same as Fig. 2, but as a function of photon rapidity
$\eta^{\gamma}$ .Figure 7. (color online) Same as Fig. 2, but as a function of photon rapidity
$\eta^{\gamma}$ .
Probing cold nuclear matter effects with the productions of isolated-${\gamma} $ and ${\gamma} $ +jet in p+Pb collisions at ${\sqrt{{s}_{{NN}}}}= $ 8.16 TeV
- Received Date: 2019-01-19
- Available Online: 2019-04-01
Abstract: We investigate cold nuclear matter (CNM) effects on the productions of isolated prompt photons and