October 10, 2013
11:00AM
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12:00PM
4138 PRB
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2013-10-10 10:00:00
2013-10-10 11:00:00
Nuclear Theory Seminar - Jacopo Ghiglieri (McGill University, Canada) "The thermal photon rate at NLO"
We present a calculation of the rate for photon production from a weakly-coupled quark-gluon plasma at next-to-leading order. We first give an overview of the leading-order (e^2g^2) result and show how it decomposes in a region dominated by 2<->2 processes (gq->gamma q and qqbar ->gamma g) and in one dominated by collinear radiation processes. At NLO (e^2g^3) both regions receive order-g corrections from momenta of order gT. We show how Euclidean and sum rule techniques can be introduced and how this technological advancement renders the calculation simpler than expected. The resulting correction is O(15-20%) for alpha s=0.3 and k/T<10. Finally, we show how similar techniques can be applied to deal with highly energetic partons and jets.
4138 PRB
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2013-10-10 11:00:00
2013-10-10 12:00:00
Nuclear Theory Seminar - Jacopo Ghiglieri (McGill University, Canada) "The thermal photon rate at NLO"
We present a calculation of the rate for photon production from a weakly-coupled quark-gluon plasma at next-to-leading order. We first give an overview of the leading-order (e^2g^2) result and show how it decomposes in a region dominated by 2<->2 processes (gq->gamma q and qqbar ->gamma g) and in one dominated by collinear radiation processes. At NLO (e^2g^3) both regions receive order-g corrections from momenta of order gT. We show how Euclidean and sum rule techniques can be introduced and how this technological advancement renders the calculation simpler than expected. The resulting correction is O(15-20%) for alpha s=0.3 and k/T<10. Finally, we show how similar techniques can be applied to deal with highly energetic partons and jets.
4138 PRB
America/New_York
public
We present a calculation of the rate for photon production from a weakly-coupled quark-gluon plasma at next-to-leading order. We first give an overview of the leading-order (e^2g^2) result and show how it decomposes in a region dominated by 2<->2 processes (gq->gamma q and qqbar ->gamma g) and in one dominated by collinear radiation processes. At NLO (e^2g^3) both regions receive order-g corrections from momenta of order gT. We show how Euclidean and sum rule techniques can be introduced and how this technological advancement renders the calculation simpler than expected. The resulting correction is O(15-20%) for alpha s=0.3 and k/T<10. Finally, we show how similar techniques can be applied to deal with highly energetic partons and jets.
