6 research outputs found

    Alien Registration- Eon, Julia (Lovell, Oxford County)

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    https://digitalmaine.com/alien_docs/21164/thumbnail.jp

    Alien Registration- Eon, Julia (Lovell, Oxford County)

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    https://digitalmaine.com/alien_docs/21164/thumbnail.jp

    Challenges to the chiral magnetic wave using charge-dependent azimuthal anisotropies in pPb and PbPb collisions at sNN=\sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV

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    Charge-dependent anisotropy Fourier coefficients (vnv_n) of particle azimuthal distributions are measured in pPb and PbPb collisions at sNN= \sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV with the CMS detector at the LHC. The normalized difference in the second-order anisotropy coefficients (v2v_2) between positively and negatively charged particles is found to depend linearly on the observed event charge asymmetry with comparable slopes for both pPb and PbPb collisions over a wide range of charged particle multiplicity. In PbPb, the third-order anisotropy coefficient, v3v_3, shows a similar linear dependence with the same slope as seen for v2v_2. The observed similarities between the v2v_2 slopes for pPb and PbPb, as well as the similar slopes for v2v_2 and v3v_3 in PbPb, are compatible with expectations based on local charge conservation in the decay of clusters or resonances, and constitute a challenge to the hypothesis that the observed charge asymmetry dependence of v2v_2 in heavy ion collisions arises from a chiral magnetic wave

    Probing the chiral magnetic wave in pPb and PbPb collisions at sNN=5.02\sqrt{s_{NN}} = 5.02 TeV using charge-dependent azimuthal anisotropies

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    Challenges to the chiral magnetic wave using charge-dependent azimuthal anisotropies in pPb and PbPb collisions at sNN= \sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV

    No full text
    Charge-dependent anisotropy Fourier coefficients (vnv_n) of particle azimuthal distributions are measured in pPb and PbPb collisions at sNN= \sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV with the CMS detector at the LHC. The normalized difference in the second-order anisotropy coefficients (v2v_2) between positively and negatively charged particles is found to depend linearly on the observed event charge asymmetry with comparable slopes for both pPb and PbPb collisions over a wide range of charged particle multiplicity. In PbPb, the third-order anisotropy coefficient, v3v_3, shows a similar linear dependence with the same slope as seen for v2v_2. The observed similarities between the v2v_2 slopes for pPb and PbPb, as well as the similar slopes for v2v_2 and v3v_3 in PbPb, are compatible with expectations based on local charge conservation in the decay of clusters or resonances, and constitute a challenge to the hypothesis that the observed charge asymmetry dependence of v2v_2 in heavy ion collisions arises from a chiral magnetic wave

    Challenges to the chiral magnetic wave using charge-dependent azimuthal anisotropies in pPb and PbPb collisions at sNN=\sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV

    No full text
    Charge-dependent anisotropy Fourier coefficients (vnv_n) of particle azimuthal distributions are measured in pPb and PbPb collisions at sNN= \sqrt{\smash[b]{s_{_{\mathrm{NN}}}}} = 5.02 TeV with the CMS detector at the LHC. The normalized difference in the second-order anisotropy coefficients (v2v_2) between positively and negatively charged particles is found to depend linearly on the observed event charge asymmetry with comparable slopes for both pPb and PbPb collisions over a wide range of charged particle multiplicity. In PbPb, the third-order anisotropy coefficient, v3v_3, shows a similar linear dependence with the same slope as seen for v2v_2. The observed similarities between the v2v_2 slopes for pPb and PbPb, as well as the similar slopes for v2v_2 and v3v_3 in PbPb, are compatible with expectations based on local charge conservation in the decay of clusters or resonances, and constitute a challenge to the hypothesis that the observed charge asymmetry dependence of v2v_2 in heavy ion collisions arises from a chiral magnetic wave
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