Direct
photon
production at
mid-ra
pidity in Pb–Pb collisions at
pan id="mmlsi1" class="mathmlsrc">mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si1.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=1c8185232f9746b818569f8c750d7a2c">mg class="imgLazyJSB inlineImage" height="15" width="105" alt="View the MathML source" style="margin-top: -5px; vertical-align: middle" title="View the MathML source" src="/sd/grey_pxl.gif" data-inlimgeid="1-s2.0-S0370269316000320-si1.gif">pt>mg height="15" border="0" style="vertical-align:bottom" width="105" alt="View the MathML source" title="View the MathML source" src="http://origin-ars.els-cdn.com/content/image/1-s2.0-S0370269316000320-si1.gif">pt>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si1.gif" overflow="scroll"><msqrt><msub><mrow><mi>smi>mrow><mrow><mi mathvariant="normal">NNmi>mrow>msub>msqrt><mo>=mo><mn>2.76mn><mtext> mtext><mtext>TeVmtext>math>pan>pan>pan> was studied in the transverse
mo
mentu
m range
pan id="mmlsi148" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si148.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=0013d3c9759dbd106f0bce3f81d2dae8" title="Click to view the MathML source">0.9<pT<14 GeV/cpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si148.gif" overflow="scroll"><mn>0.9mn><mo><mo><msub><mrow><mi>pmi>mrow><mrow><mi mathvariant="normal">Tmi>mrow>msub><mo><mo><mn>14mn><mtext> mtext><mtext>GeVmtext><mo stretchy="false">/mo><mi>cmi>math>pan>pan>pan>. Photons were detected with the highly seg
mented electro
magnetic calori
meter PHOS and via conversions in the ALICE detector
material with the
pan id="mmlsi4" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si4.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=1166737fefdecce3d6290006e66f4e08" title="Click to view the MathML source">ep>+p>ep>−p>pan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si4.gif" overflow="scroll"><msup><mrow><mi>emi>mrow><mrow><mo>+mo>mrow>msup><msup><mrow><mi>emi>mrow><mrow><mo>−mo>mrow>msup>math>pan>pan>pan>
pair reconstructed in the central tracking syste
m. The results of the two
methods were co
mbined and direct
photon s
pectra were
measured for the 0–20%, 20–40%, and 40–80% centrality classes. For all three classes, agree
ment was found with
perturbative QCD calculations for
pan id="mmlsi5" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si5.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=f876eeae8231e04158b538b59eb9bcfd" title="Click to view the MathML source">pT≳5 GeV/cpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si5.gif" overflow="scroll"><msub><mrow><mi>pmi>mrow><mrow><mi mathvariant="normal">Tmi>mrow>msub><mo>≳mo><mn>5mn><mtext> mtext><mtext>GeVmtext><mo stretchy="false">/mo><mi>cmi>math>pan>pan>pan>. Direct
photon s
pectra down to
pan id="mmlsi6" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si6.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=145471da8223133907c91fcc1011f6da" title="Click to view the MathML source">pT≈1 GeV/cpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si6.gif" overflow="scroll"><msub><mrow><mi>pmi>mrow><mrow><mi mathvariant="normal">Tmi>mrow>msub><mo>≈mo><mn>1mn><mtext> mtext><mtext>GeVmtext><mo stretchy="false">/mo><mi>cmi>math>pan>pan>pan> could be extracted for the 20–40% and 0–20% centrality classes. The significance of the direct
photon signal for
pan id="mmlsi7" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si7.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=4067fc100418e5d9dc8ef576fcc34c21" title="Click to view the MathML source">0.9<pT<2.1 GeV/cpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si7.gif" overflow="scroll"><mn>0.9mn><mo><mo><msub><mrow><mi>pmi>mrow><mrow><mi mathvariant="normal">Tmi>mrow>msub><mo><mo><mn>2.1mn><mtext> mtext><mtext>GeVmtext><mo stretchy="false">/mo><mi>cmi>math>pan>pan>pan> is 2.6
m>σ m> for the 0–20% class. The s
pectru
m in this
pan id="mmlsi8" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si8.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=aa58cb03581d230341ba1ff810fef8b0" title="Click to view the MathML source">pTpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si8.gif" overflow="scroll"><msub><mrow><mi>pmi>mrow><mrow><mi mathvariant="normal">Tmi>mrow>msub>math>pan>pan>pan> range and centrality class can be described by an ex
ponential with an inverse slo
pe
para
meter of
pan id="mmlsi9" class="mathmlsrc">pan class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0370269316000320&_mathId=si9.gif&_user=111111111&_pii=S0370269316000320&_rdoc=1&_issn=03702693&md5=2e8066a435697eed598476449755381f" title="Click to view the MathML source">(297±12p>statp>±41p>systp>) MeVpan>pan class="mathContainer hidden">pan class="mathCode"><math altimg="si9.gif" overflow="scroll"><mo stretchy="false">(mo><mn>297mn><mo>±mo><msup><mrow><mn>12mn>mrow><mrow><mtext>statmtext>mrow>msup><mo>±mo><msup><mrow><mn>41mn>mrow><mrow><mtext>systmtext>mrow>msup><mo stretchy="false">)mo><mtext> mtext><mtext>MeVmtext>math>pan>pan>pan>. State-of-the-art
models for
photon
production in heavy-ion collisions agree with the data within uncertainties.