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Zimányi Winter School, 2013/12/05 Csörgő, T. 1 Observables and initial conditions from exact rotational hydro solutions T. Csörgő 1, I. Barna 1 and M.I.

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Presentation on theme: "Zimányi Winter School, 2013/12/05 Csörgő, T. 1 Observables and initial conditions from exact rotational hydro solutions T. Csörgő 1, I. Barna 1 and M.I."— Presentation transcript:

1 Zimányi Winter School, 2013/12/05 Csörgő, T. 1 Observables and initial conditions from exact rotational hydro solutions T. Csörgő 1, I. Barna 1 and M.I. Nagy 1,3 1 MTA Wigner Research Center for Physics, RMKI 1 MTA Wigner Research Center for Physics, RMKI 3 ELTE University, Budapest, Hungary Continuation: observables Two different family of equations of state Single particle spectra Elliptic and higher order flows Oscillations of HBT radii What have we learnt? Summary Manuscript in preparation arXiv:1309.4390v2

2 Zimányi Winter School, 2013/12/05 Csörgő, T. 2 Rotated Gaussian solutions Rotated Gaussian solutions Note: (r’, k’) in fireball frame rotated wrt lab frame (r,k) Note: in this talk, rotation in the (X,Z) impact parameter plane !

3 Zimányi Winter School, 2013/12/05 Csörgő, T. 3 Role of EoS on acceleration Role of EoS on acceleration Lattice QCD type Eos is explosive Tilt angle  integrates rotation in (X,Z) plane: sensitive to EoS!

4 Zimányi Winter School, 2013/12/05 Csörgő, T. 4 Single particle spectra Single particle spectra In the rest frame of the fireball: Rotation increases effective temperatures both in the longitudinal and impact parameter direction in addition to Hubble flows

5 Zimányi Winter School, 2013/12/05 Csörgő, T. 5 Directed, elliptic and other flows Directed, elliptic and other flows Note: model is fully analytic As of now, only X = Z = R(t) spheroidal solutions are found → vanishing odd order flows See next talk for fluctuations From the single particle spectra → flow coefficents v n

6 Zimányi Winter School, 2013/12/05 Csörgő, T. 6 Reminder: Universal w scaling of v 2 Reminder: Universal w scaling of v 2 Notes: Rotation does not change this Just modifies Radial flow parameters See +for more details

7 Zimányi Winter School, 2013/12/05 Csörgő, T. 7 HBT radii for rotating spheroids HBT radii for rotating spheroids New terms with blue → Rotation decreases HBT radii similarly to Hubble flow. Diagonal Gaussians in natural frame

8 Zimányi Winter School, 2013/12/05 Csörgő, T. 8 HBT radii in the lab frame HBT radii in the lab frame HBT radii without flow But spheriodal symmetry of the solution Makes several cross terms vanish → need for ellipsoidal solutions

9 Zimányi Winter School, 2013/12/05 Csörgő, T. 9 HBT radii in the lab frame HBT radii in the lab frame HBT radii without flow But spheriodal symmetry of the solution Makes several cross terms vanish → need for ellipsoidal solutions

10 Zimányi Winter School, 2013/12/05 Csörgő, T. 10 Qualitatively rotation and flow similar Qualitatively rotation and flow similar But need more time dependent calculations and less academic studies (relativistic solutions)

11 Zimányi Winter School, 2013/12/05 Csörgő, T. 11 Summary Summary Observables calculated Effects of rotation and flow Combine and have same mass dependence Spectra: slope increases v 2 : universal w scaling remains valid HBT radii: Decrease with mass intensifies Even for spherical expansions: v 2 from rotation. Picture: vulcano How to detect the rotation? Next step: penetrating probes

12 Zimányi Winter School, 2013/12/05 Csörgő, T. 12 Summary Summary Observables calculated Effects of rotation and flow Combine and have same mass dependence Spectra: slope increases v 2 : universal w scaling remains valid HBT radii: Decrease with mass intensifies Even for spherical expansions: v 2 from rotation. Picture: vulcano How to detect the rotation? Next step: penetrating probes


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