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--- energy:muon_forum [2021/10/27 11:04] – [Past Muon Forum Meetings and their Focus Areas (with recordings)] sergo
+++ energy:muon_forum [2022/08/09 10:36] (current) – [Parameters for Physics Studies in mu+mu- collisions] sergo
@@ Line 5: / Line 5: @@
 Please use instructions from here https://snowmass21.org/start or email the contact people below in order to join the slack channel and the mailing list)
+=====Forum Reports=====
+<color #ed1c24>Draft released to Snowmass community on 06/23/2022:</color>  [[https://drive.google.com/file/d/10j0k1z1OrDdBx6S-ohCa0Y0PA5bGeTDf/view?usp=sharing|Link to the document]]
+  *Please provide your feedback in this google file: [[https://docs.google.com/document/d/16gV4-ELOmve1TEkkcTP8R6eFN9WrZcwjZhMskZ7P5yY/edit?usp=sharing|Feedback Doc]]
+  *Author sign up via Indico registration (** the sign up does not require direct contributions to the Report and is rather an expression of support and interest to what is described in the document**): [[https://indico.fnal.gov/event/55041/|Indico Link]]
 ===== Forum Coordinators =====
@@ Line 16: / Line 22: @@
 ===== Past Muon Forum Meetings and their Focus Areas (with recordings) =====
-<color #ed1c24>**Upcoming:**</color> tbd
+[[https://indico.fnal.gov/event/53010/|Muon Collider Agora Event 02/16/2022]]
+[[https://indico.fnal.gov/event/52423/|Detector Technologies 01/11/2022]]
+[[https://indico.fnal.gov/event/51676/|Discussion of the Snowmass Muon Collider Forum Report 11/30/2021]]
 [[https://indico.fnal.gov/event/51315/|Synergies with precision muon. Comparison of BiB at different energies 10/12/2021]]
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 ===== Parameters for Physics Studies in mu+mu- collisions   =====
-Points shown in <color #ed1c24>RED</color> are to be included into the Snowmass Summary plots/tables. Additional points (in black) are optional, but can be used to demonstrate performance in the presence of realistic beam background connditions.
+Points shown in <color #ed1c24>**RED**</color> to be included into the Snowmass Summary plots/tables. Additional points (in black) are optional, but can be used to demonstrate performance in the presence of realistic beam background connditions.
-|COM Energy | <color #ed1c24>**125 GeV**</color> | 1.5 TeV | <color #ed1c24>**3 TeV**</color>  | 6 TeV  |  <color #ed1c24>**10 TeV**</color> | 14 TeV | <color #ed1c24>**30 TeV**</color> |
+|COM Energy | <color #ed1c24>**125 GeV**</color> | 1.5 TeV | <color #ed1c24>**3 TeV**</color>  | 6 TeV  |  <color #ed1c24>**10 TeV**</color> | 14 TeV |  30 TeV |
-|Total Luminosity (ab-1)/ per IP|  <color #ed1c24>0.010 (conserv.) - 0.025 (optim.)</color>  |  0.25 |  <color #ed1c24>1.0</color> |  4.0  |  <color #ed1c24>10</color> | 10 | <color #ed1c24>10</color> |
+|Total Luminosity (ab-1) |  <color #ed1c24>0.020 </color>|  0.25 |  <color #ed1c24>1.0</color> |  4.0  |  <color #ed1c24>10</color> | 10 | 10 |
 <color #00a2e8>**Comments:**</color>\\
-- Total luminosity is per interaction point and assumes 5 years of datataking. \\
+- Total luminosity is per interaction point and assumes 5 years of datataking at each energy. \\
-- Higgs Factory 125 GeV  luminosity projections correspond to conservative and optimistic scenarios.
+- Higgs Factory 125 GeV luminosity projections are higher than those corresponding to the MAP design and assume improvements from recent advancements in technology and potentially a higher duty cicle. The projection assumes  narrow energy spread of the beam, which is beneficial for Higgs production and width measurements. \\
-The projections assume very narrow energy spread of the beam, which is beneficial for Higgs production and width measurements. \\
 - Two detectors can be planned (except for 125 GeV), which will further increase luminosity by a factor of 2.\\
 - Please contact us for configurations not included in the table or with any other questions.\\