role of dynamic geometry in jet tomography

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Role of Dynamic Geometry in Jet Tomography. William Horowitz Columbia University December 12, 2005. In conjunction with Simon Wicks, Magdalenda Djordjevic, and Miklos Gyulassy. Motivation. Past tomographic models simplified the calculation by neglecting either: Multigluon fluctuations - PowerPoint PPT Presentation

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Heavy Flavor Productions Workshop12/12/05 William Horowitz

Role of Dynamic Geometry in Jet Tomography

William HorowitzColumbia UniversityDecember 12, 2005

In conjunction with Simon Wicks, Magdalenda Djordjevic, and Miklos Gyulassy

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Motivation

• Past tomographic models simplified the calculation by neglecting either:– Multigluon fluctuations– Path length fluctuations

• For fixed-length calculations, reasonable but unjustifiable length L~5 fm used

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Significance of Nuclear Profile

• Simpler densities create a surface biasHard Cylinder Hard Sphere Woods-Saxon

Toy model for purely geometric radiative loss from Drees, Feng, Jia, Phys. Rev. C.71:034909

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Edgy Geometry

• We use the Woods-Saxon nuclear geometry, which has a fuzzy “edge”

• There is no unique, natural LWS definition– Two examples (of many possibilities):

• We will use the latter formula

,)0(

)ˆ( 0

ρ

dllnxρL

ρ

dllnxρL

)ˆ( 0

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Partonic RAA Model

– where P incoherently convolves DGLV energy loss (including multigluon fluctuations) with the infinite-time elastic energy loss for fixed s

)(

);;,(ε,ε1ε);(),;(

2

bN

pbφxLPdbxTxdpbφR

coll

Tn

AA

TAA

Momentum Jacobian as survival probability; see, e.g., Gyulassy, nucl-th/0403032

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Volume Emission of Partons

• fixed pT = 15 GeV, yT = = 0, and s = .3

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Average Lengths of Emission

• Dynamic volume depends on partonic species and pT

– For pT = 5, 10, 15, 20 GeV, s = .3

– <Lg> = 1.74, 1.93, 2.16, 2.41 fm

– <Lu> = 3.83, 4.21, 4.47, 4.62 fm

– <Lc> = 4.65, 4.43, 4.48, 4.50 fm

– <Lb> = 6.17, 5.69, 5.43, 5.29 fm

Heavy Flavor Productions Workshop12/12/05 William Horowitz

The Results

• Electrons • Pions

s = .3

Heavy Flavor Productions Workshop12/12/05 William Horowitz

The Results

• Electrons • Pions

s = .4

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Conclusions

• There are several large effects that must be taken into account in any energy loss model:– Multigluon fluctuations– Path length fluctuations– Collisional energy loss

– Running s

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Future Work

• Find more accurate analytic formulae for collisional loss– Molnár’s parton cascade provides

exact numerical answer

• Simultaneously treat elastic and inelastic energy loss– Find a more natural L?

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Future Work (cont’d)

• Allow s to run– Nonzero lower bound to theoretical

error

• Use even more accurate medium density– Hirano’s CGC-initial condition 3+1 D

evolving hydro background

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Let’s Eat!

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Partonic RAA Model

• Exploit the power law production rate to use the momentum Jacobian to define the probability of escape, (1-)n

– pT, final = pT, initial

– n is simply related to the exponent of the power law

– Assumes a slowly changing power law

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Combining Models

• Find a fixed L that reproduces the dynamical length-generated partonic RAA using proper initial spectra followed by fragmentation into pions and electrons

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Vary s

• We expect a big change since

• Erad ~ s3

• Eelas ~ s2

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Finding Fixed L

• Heavies • Lights

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Heavies alph=.4 BT and TG

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Theoretical Error from Length Uncertainty

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Volume Emission fors = .4

Heavy Flavor Productions Workshop12/12/05 William Horowitz

Volume Emission for s = .4 (cont’d)

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