Cargando…
Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries
The nuclear modification factor $R_{\rm AA}$ has been satisfactorily described by various jet quenching models. Nonetheless, all these formalisms, until very recently, underpredicted the high-$p_{\rm T}$ (> 10 GeV) elliptic flow $v_2$. We find that the simultaneous description of these observable...
| Autores principales: | , , , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
SISSA
2019
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.22323/1.345.0070 http://cds.cern.ch/record/2665945 |
| _version_ | 1780961966629584896 |
|---|---|
| author | Andres, Carlota Armesto, Néstor Niemi, Harri Paatelainen, Risto Salgado, Carlos A. |
| author_facet | Andres, Carlota Armesto, Néstor Niemi, Harri Paatelainen, Risto Salgado, Carlos A. |
| author_sort | Andres, Carlota |
| collection | CERN |
| description | The nuclear modification factor $R_{\rm AA}$ has been satisfactorily described by various jet quenching models. Nonetheless, all these formalisms, until very recently, underpredicted the high-$p_{\rm T}$ (> 10 GeV) elliptic flow $v_2$. We find that the simultaneous description of these observables requires to strongly suppress the quenching for the first $\sim 0.6$ fm after the collision. This shows the potential of jet quenching observables to constrain the dynamics of the initial stages of the evolution. |
| id | cern-2665945 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2019 |
| publisher | SISSA |
| record_format | invenio |
| spelling | cern-26659452019-10-15T15:27:51Zdoi:10.22323/1.345.0070http://cds.cern.ch/record/2665945engAndres, CarlotaArmesto, NéstorNiemi, HarriPaatelainen, RistoSalgado, Carlos A.Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetriesnucl-thNuclear Physics - Theoryhep-phParticle Physics - PhenomenologyThe nuclear modification factor $R_{\rm AA}$ has been satisfactorily described by various jet quenching models. Nonetheless, all these formalisms, until very recently, underpredicted the high-$p_{\rm T}$ (> 10 GeV) elliptic flow $v_2$. We find that the simultaneous description of these observables requires to strongly suppress the quenching for the first $\sim 0.6$ fm after the collision. This shows the potential of jet quenching observables to constrain the dynamics of the initial stages of the evolution.SISSAarXiv:1902.07643JLAB-THY-19-2891oai:cds.cern.ch:26659452019-02-20 |
| spellingShingle | nucl-th Nuclear Physics - Theory hep-ph Particle Physics - Phenomenology Andres, Carlota Armesto, Néstor Niemi, Harri Paatelainen, Risto Salgado, Carlos A. Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title | Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title_full | Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title_fullStr | Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title_full_unstemmed | Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title_short | Constraining energy loss from high-$p_{\rm T}$ azimuthal asymmetries |
| title_sort | constraining energy loss from high-$p_{\rm t}$ azimuthal asymmetries |
| topic | nucl-th Nuclear Physics - Theory hep-ph Particle Physics - Phenomenology |
| url | https://dx.doi.org/10.22323/1.345.0070 http://cds.cern.ch/record/2665945 |
| work_keys_str_mv | AT andrescarlota constrainingenergylossfromhighprmtazimuthalasymmetries AT armestonestor constrainingenergylossfromhighprmtazimuthalasymmetries AT niemiharri constrainingenergylossfromhighprmtazimuthalasymmetries AT paatelainenristo constrainingenergylossfromhighprmtazimuthalasymmetries AT salgadocarlosa constrainingenergylossfromhighprmtazimuthalasymmetries |