Difference between revisions of "Neutrino Mass WG Telecon"

From CMB-S4 wiki
Jump to: navigation, search
Line 5: Line 5:
 
To be modeled off of the Science Book chapter, with updates and some new ingredients
 
To be modeled off of the Science Book chapter, with updates and some new ingredients
  
* Brief Intro
+
* [[Brief Intro]]
  
* CMB Lensing / forecasting
+
* [[CMB Lensing / forecasting]]
 
Goals:  
 
Goals:  
  
Line 22: Line 22:
 
-Discuss influence of priors on conclusions about hierarchy, mass scale
 
-Discuss influence of priors on conclusions about hierarchy, mass scale
  
* Additional CMB - S4 probes
+
* [[Additional CMB - S4 probes]]
 
Goals:
 
Goals:
  
 
- Add cluster based forecasts, add cross-correlation based forecasts
 
- Add cluster based forecasts, add cross-correlation based forecasts
  
*S4 constraints in context with lab experiments and neutrino model-building  
+
*[[S4 constraints in context with lab experiments and neutrino model-building]]
 
Goals:  
 
Goals:  
  

Revision as of 09:48, 7 August 2018

Neutrino Mass Analysis Working Group Plan Through December 2018

Outline of Science Chapter

To be modeled off of the Science Book chapter, with updates and some new ingredients

Goals:

-Add updates with new noise levels

-What can we say about CMB lensing vs RSD, weak lensing, Lyman-alpha, cluster abundance?

-Add discussion of systematics and why the measurement should be robust

-Expand on tau limitation. What you actually need to know about foregrounds and noise given the tau limits. Options for improving tau?

-Discuss model independence with cross-correlations

-Discuss influence of priors on conclusions about hierarchy, mass scale

Goals:

- Add cluster based forecasts, add cross-correlation based forecasts

Goals:

-Include input from neutrino phenomenologists and experimentalists

-Potentially add: updates regarding Miniboone results? Updates regarding stronger hints of Normal Hierarchy or delta?

-Detection scenarios: expand on Section 3.5 and Table 3-2 in Science Book

-Discussion of how Mnu constraints inform model building



To-do before September Meeting:

-Preliminary forecasts on neutrino mass for each key observable

-Have conclusions in hand OR identify specific outstanding issues for what we can say about CMB lensing vs other methods

-Tau limitation and prospects for improvement

-Impact of priors

-Summary of content for context with lab experiments / model-building for comments


To-do by November:

-Draft of chapter available for circulation