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2019:groups:higgs:lightscalars [2019/06/28 09:05] jonathan.butterworth |
2019:groups:higgs:lightscalars [2019/06/28 11:15] (current) suzanne.gascon |
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* Quick contur study using the BNT ALP UFO file. All couplings set to zero except the photons which is scanned over. {{ :2019:groups:higgs:combinedhybrid.pdf | 2D scan }}. Over a wide range of $\phi$ masses ($M_{ALP}$ on the plot) the sensitivity extends down to $C_{\gamma\gamma}/\Lambda \approx 3$ TeV$^{-1}$. Here the scan is performed over the following ranges: $m_a:$ 1 to 50 GeV, $g_{a\gamma\gamma}$: 10 to $10^{-6}$, $g_{aZ\gamma}$: 10 to $10^{-6}$ | * Quick contur study using the BNT ALP UFO file. All couplings set to zero except the photons which is scanned over. {{ :2019:groups:higgs:combinedhybrid.pdf | 2D scan }}. Over a wide range of $\phi$ masses ($M_{ALP}$ on the plot) the sensitivity extends down to $C_{\gamma\gamma}/\Lambda \approx 3$ TeV$^{-1}$. Here the scan is performed over the following ranges: $m_a:$ 1 to 50 GeV, $g_{a\gamma\gamma}$: 10 to $10^{-6}$, $g_{aZ\gamma}$: 10 to $10^{-6}$ | ||
* Checking at an example point in the above scan, $M_{ALP} = 1.8$ GeV, $C_{\gamma\gamma}/\Lambda = 5.2$ TeV$^{-1}$, all other couplings set to zero. The $\phi$ decays 100% to $\gamma\gamma$ as expected (width $10^{-7}$ GeV). The main production mechanisms are $\gamma, W$ or $Z$ + $\phi$. $gg \rightarrow \phi$ is zero. The different subprocess cross sections are visible in the example Herwig output file: {{ :2019:groups:higgs:lhc-s101-runpoint_0095.out.txt | lhc-s101-runpoint_0095.out}} | * Checking at an example point in the above scan, $M_{ALP} = 1.8$ GeV, $C_{\gamma\gamma}/\Lambda = 5.2$ TeV$^{-1}$, all other couplings set to zero. The $\phi$ decays 100% to $\gamma\gamma$ as expected (width $10^{-7}$ GeV). The main production mechanisms are $\gamma, W$ or $Z$ + $\phi$. $gg \rightarrow \phi$ is zero. The different subprocess cross sections are visible in the example Herwig output file: {{ :2019:groups:higgs:lhc-s101-runpoint_0095.out.txt | lhc-s101-runpoint_0095.out}} | ||
- | * Some more scans as suggested by Aoife and Jose:{{:2019:groups:higgs:combinedhybrid50.png?200|}} | + | * Some more scans as suggested by Aoife and Jose: |
+ | * {{:2019:groups:higgs:combinedhybrid50.png?200|}} | ||
+ | * {{:2019:groups:higgs:combinedhybrid30.png?200|}} | ||
+ | * {{:2019:groups:higgs:combinedhybrid10.png?200|}} | ||
For instance, Higgs composite models with additional light scalars:[[https://arxiv.org/pdf/1810.11142.pdf|1710.11142]], [[https://arxiv.org/pdf/1902.08690.pdf|1902.08690]]. | For instance, Higgs composite models with additional light scalars:[[https://arxiv.org/pdf/1810.11142.pdf|1710.11142]], [[https://arxiv.org/pdf/1902.08690.pdf|1902.08690]]. | ||
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Please send to Gregory, Susan and Jose by Thursday morning (so we can give a synthesis to the speaker by ~Thursday noon and also circulate among us) | Please send to Gregory, Susan and Jose by Thursday morning (so we can give a synthesis to the speaker by ~Thursday noon and also circulate among us) | ||
+ | Thank you all for all the work, and let's not stop here! {{ :2019:groups:higgs:suzannegregorylightscalarlhc2019slides.ppt | Here }} are the slides shown in the summary session on June 28, 2019. |