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Mee#ng wiki is found at h2ps://zzz.physics.umn.edu/lowrad/mee#ng8 Click on the “Detailed Agenda” and upload your talks there AARM Collabora#on Mee#ng at SDSM&T AARM Community and Collabora#ve Tools (P. Cushman) Discussion of what the community needs on website. Task assignment and priori9za9on Dark Ma2er infrastructure priori#es (R. Schnee) Resourcesharing to/from broader community informed by these priori9es. 0νββ background infrastructure priori#es (J. Detwiler) SURF Tours leave promptly at 2 pm 25:30 is a G2 DM mee=ng (LZ + SuperCDMS) Hisega Room Introduc#on Today

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Page 1: Introduc#on&Today& · &Do&neutron&benchmark&experiments&of&hadronic&showers&underground& $ VVD \ D Q G $ FT X LVLWLR Q R I5 D G LR S X UH 0 D WH ULD OV D FR R S H UD WLY H D S S UR

Mee#ng  wiki  is  found  at  h2ps://zzz.physics.umn.edu/lowrad/mee#ng8    Click  on  the  “Detailed  Agenda”  and  upload  your  talks  there  

AARM  Collabora#on  Mee#ng  at  SDSM&T  

 AARM  Community  and  Collabora#ve  Tools            (P.  Cushman)      Discussion  of  what  the  community  needs  on  website.        Task  assignment  and  priori9za9on  

   Dark  Ma2er    infrastructure  priori#es                    (R.  Schnee)      Resource-­‐sharing  to/from  broader  community  informed  by  these  priori9es.  

   0νββ  background  infrastructure  priori#es      (J.  Detwiler)  

     SURF  Tours  leave  promptly  at    2  pm  

     2-­‐5:30  is  a  G2  DM  mee=ng  (LZ  +  SuperCDMS)    Hisega  Room  

Introduc#on  Today  

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   May  21  (Thursday  Morning)  Bump  Lounge,  Surbeck  Center.    Gotomee#ng    All  talks  provide  bullet  points  for  discussion.  Unless  otherwise  designated,  assume  15  min  for  the  talk  and  5  minutes  for  discussion.  Discussion  topics  that  require  more  9me  should  be  noted  by  the  working  group  leaders  and  revisited  during  the  parallel  sessions.    8:30  Screening  

 Surface  Screening  with  XIA        (J.  Cooley)    Large  volume  screening  detector      (J.  Reichenbacher)    Beta  Cage              (R.  Schnee)    Ultratrace  polymer  analysis  via  ICP-­‐MS  (I.  Arnquist)    Low  radon  clean  rooms          (R.  Bunker)    Update  on  the  BHUC          (B.  Mount  -­‐  remote)  

10:15  Coffee    10:45    Radiogenics,  alpha-­‐n  

 Code  comparisons  and  cross  sec#ons    (S.  Scorza)    Neutron-­‐channel  reac#on  codes      (C.  Zhang)  

11:25  Simula=ons    GEANT4  status  and  prospects      (D.  Wright)    FLUKA  vs  Geant            (A.  Kennedy)    Depth  Requirements  for  G3  LAr      (A.  Hime  -­‐  remote)    Cosmogenic  Ac#va#on  codes        (D.M.  Mei)  

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   May  21  (Thursday  Adernoon)  

2:00          Neutrons    Bump  lounge    Neutral  par#cle  simula#ons  for  PICO-­‐2L  (20  min)                                        (A.  Robinson)    Veto  shield  and  neutron  correla#ons.  Data  access  invita#on  (A.  Villano)    Gadolinium  neutron-­‐capture  gammas  in  Geant4                                          (Y.  Chen)    Soudan  Liquid  Scin#llator  detector  (10  min)                                                            (C.  Zhang)  

 3:20  Coffee    3:50  -­‐  5:30  Working  Groups  

 Cleanliness  protocol,  Surface  Contamina#on  &  Radon  Plateout      Leaders:  R.  Bunker,  J.  Cooley  (Bump  Lounge)    Priori#es  in  simula#on  and  neutron  background  es#ma#on      Leaders:  A.  Villano,  D.  Wright  (Hisega  Room:  access  code  1626019#)  

 5:30  –  6:00  Report  from  working  groups  –  Integra#on  discussion  (Bump  Lounge)    7:00    Group  Dinner  at  Kathmandu  

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Communica=on  and  Collabora=on  on    common  issues  related  to    

Assay  and  Acquisi=on  of  Radiopure  Materials  Priscilla  Cushman  

University  of  Minnesota  

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               The  Model  and  Funding  of  AARM  have  evolved    2009-­‐12:      NSF  grant  (DUSEL  S4)  •    Characterize  backgrounds  at  all  levels  of  Homestake  •   Design  a  common  low  background  coun9ng  facility  •   Develop  common  screening  tools  (R&D  as  needed)    2012-­‐14:  Cooperate  to  help  understand  and  mi#gate  backgrounds.      Simula=on  recognized  as  a  major  “infrastructure”    

           Validate  and  improve  current  simula#on  tools        Major  advances  in  GEANT4  treatment  of  cosmogenic  neutrons        Con#nued  improvements  in  (alpha,n)  physics  and  cross-­‐sec#ons      

Background  characteriza=on  more  broadly  defined  as                  Community  Materials  Assay  Database                Neutron  benchmarking  (data  vs  sim)              Integra#on/Promo#on  of  exis#ng  assay  resources  around  the  world            and  the  development  of  a  unified  plan  to  increase  availability      

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                             “Integra=ve  Tools  for  Underground  Science”      Principle  Inves#gators                          Priscilla  Cushman  (University  of  Minnesota)                          Jodi  Cooley  (Southern  Methodist  University)                                    Toni  Empl  (University  of  Arkansas,  Li2le  Rock)                          Angela  Reise2er  (Evansville  University)                          Richard  Schnee  (Syracuse  University  !  SDSM&T)  

•  Cosmogenic  Simula#on  Group    •  Universal  Materials  Database  

•  Radiogenic  Cross  Sec#on  Working  Group  

•  FLUKA-­‐Geant4  Compara#ve  Study  Group  

•  Neutron  Benchmarking  Data  Group  

Funding  model:    NSF  Grant  for  Specific  Tasks  iden#fied  by  the  community  as  high  priority,    

 but  not  covered  directly  by  the  experiment.        

   AARM  is    Organized  by  working  group.      Bi-­‐annual  workshops  combine  talks  on  new  developments  with  Working  Group  sessions  devoted  to  work  and  planning.    

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                   Snowmass  Community  Planning    2013:    APS  Div.  of  Par=cles  and  Fields  planning  exercise  for  HEP    

         Resulted  in  a  strong  case  for  Underground  Infrastructure  in                                                                                                    the  main  document    and  in  accompanying  white  papers.    

         However,  momentum  lagged  in  the  face  of  budget  reali#es            Underground  Space  is  a  “Laboratory  Capability”  “Experimental  needs  worldwide  far  outstrip  current  assay  capability.  Opera#on  as  a  user  facility  across  mul#ple  sites  with  exis#ng  exper#se  is  the  most  efficient  use  of  resources  and  personnel.”    “There  is  enough  U.S.  infrastructure  space  for  the  future  if  exis#ng  U.S.  underground  labs  are  maintained.  Substan#al  past  agency  investment  and  future  leverage  of  state,  university,  private  and  other  agency  (e.g.,  non-­‐prolifera#on)  funds  make  it  cost  effec#ve  and  a2rac#ve  to  maintain  these  sites  for  smaller  experiments,  generic  R&D,  and  as  elements  of  a  centrally  managed  materials  assay  consor#um.”  

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A  DOE-­‐proposed  Workshop  (summer  2014)      to  define  Low  Background  Infrastructure  was  delayed        

 The  G2  Down-­‐Select  and  a  reduced  budget  changed  the  landscape    

 US  agencies  look  to  the  2  major  dark  ma2er  experiments  to  quan#fy  needs    Other  DM  experiments  are  considered  G3  R&D    0νββ  is  considered  G3  and  not  well-­‐integrated  into  the  bigger  picture  

 In  response,  LZ  and  SuperCDMS    must  coordinate  background  needs.      

 March  mee#ng  at  PNNL,  Second  mee#ng  today  at  SDSM&T    AARM’s  role  is  to  provide  tools  to  facilitate  coopera#on  within  G2,  but  also  to  

 broaden  par#cipa#on  to  other  experiments  both  US  and  interna#onal.      Natural  Partnership  with  LRT.  

 LRT  conferences  for  en#re  underground  community    Couple  with  planning  for  interim  working  groups  

AARM  Going  forward  

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AARM  Going  forward  March  2014:    Workshop  at  FNAL  to  iden#fy  the  highest  priority  items.  Enable  AARM  to  con#nue  to  facilitate  exchange  of  ideas  and  foster  new  proposals    

Integra=ve  Website  with  o    All  relevant  publica#ons  and  links  organized  in  one  place  

   Including  all  the  AARM  workshop  talks  and  the  LRT  talks/proceedings  o     Contact  informa#on  and  scheduling  tools  for  woldwide  assay  centers  

   Including  HPGe,  Surface  assay,  ICPMS,  NAA    etc  o    Community  Assay  Database,  including  hooks  from  the  assay  centers  o    GEANT/FLUKA/MCNP  code  tools,  code  benchmarking  and  updates  o    Nuclear  Databases,  alpha-­‐n,  SOURCES4  etc  o    Cleaning  and  Handling  Protocols.    Standardize  Assay  Prep  o    Cosmogenic  Ac#va#on,  underground  storage,  transport  shielding  o    Data  on  radon  plateout  and  diffusion  in  various  materials    AND  the  work/computa#on/research  that  has  to  be  done  to  populate  those  pages!  e.g.  Perform  experiments  to  quan#fy  radon  plateout  and  diffusion  in  many  materials  

 Develop  new  surface  screening  techniques    Do  neutron  benchmark  experiments  of  hadronic  showers  underground  

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Assay  and  Acquisition  of  Radiopure  Materialsa  cooperative  approach  to  low  radiation  techniques  and  sensitive  background  measurement

Home

Community

Facilities  and

Scheduling:

Detectors  info

Assay  request

Storage  request

Community  Assay

Database

Background  Studies

Laboratory  Materials

Clean-­handling

Procedures

Resources:

Publications

AARM  presentations

LRT  presentations

Go  to  Lowrad  Wiki

Interdisciplinary

Research  Portals

The  purpose  of  this  website  is  to  share  knowledge  and

resources  across  the  community  of  those  involved  in

low-­radioactivity  experimental  techniques.  The  tasks

covered  include

1.   Coordinating  users  and  providers  of  sensitive

assay  facilities

2.   Linking  to  information  on  availability  of  radiopure

materials

3.   Sharing  knowledge  concerning  backgrounds  in

low-­background  experiments

NEWS:

The  next  AARM  meeting  is  May  20-­21,  2015.  It  will  beheld  right  after  the  Conference  on  Science  at  SURFhosted  at  the  South  Dakota  School  of  Mines  &Technology.

Summary  agenda  on  the  AARM  wiki  and  copied  below.For  more  detail  see  the  full  agenda.

May  20  (Wednesday)12:30-­1:45 Discussion  over  box  lunch:

AARM  (website  and  other  common  tools)

G2  collaboration  infrastructure  priorities

0νββ  background  infrastructure

2:00-­5:00 SURF  tour  or  LZ-­SuperCDMS  meetingSuggestions?  Send  them  to  [email protected]  and  [email protected]  

The  AARM  Integra=on  Website  

Rota#ng  picture  and  contact  informa#on  for    Labs  &  Experiments  

Home  Page  

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The  AARM  Integra=on  Website  

 Facili#es  and  Scheduling:  Detector  Info    What  the  Assay  Facility  Manager  submits        Up  to  date  informa#on  on  screening  available  at  labs.        Form  defines  relevant  informa#on  and  sorts  it  

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The  AARM  Integra=on  Website    Facili#es  and  Scheduling:  Assay  or  Storage  Request    What  the  user  submits      Check  out  the  available  assay  from  Detector  Info      Fill  out  request  form  –  goes  to  the  contact  listed    Storage  request  also  available  

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The  AARM  Integra=on  Website    Resources:      Easy  reference  for  relevant  papers      Links  to  LRT  and  AARM  presenta#ons      Add  your  own  papers    

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The  AARM  Integra=on  Website  Step  1:  TENDL  vs  EMPIRE  cross  sec#ons  comparison    TENDL  2011  and  2012  have  been  considered  as  the  USD  website  inputs.  TENDL  is  a  nuclear  data  library  (validated)  which  provides  the  output  of  the  TALYS  nuclear  model  code  system.  EMPIRE  cross  sec#on  are  the  input  libraries  of  SOURCES4    Step  2:  USD  website  vs  SOURCES4  calcula#ons:  compare  the  radiogenic  neutron  spectra  coming  from  both  codes.    

Compiled  plots  and  data  from  AARM  studies  Portals  to  other  relevant  websites  

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The  AARM  Integra=on  Website  Compiled  plots  and  data  from  AARM  studies  Portals  to  other  relevant  websites  

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The  AARM  Integra=on  Website  Register  your  name  and  find  others  with  common  interests.    

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AARM  recognized  10  years  ago  the  need  for  an  Assay  Database      with  an  easy-­‐to-­‐use  interface  to  enter  new  data      and  to  search  for  radiopure  materials,  vendors,  etc.  

The  Majorana  database  (J.  Loach)  was  chosen  as  a  template    The  more  globally  used,  the  more  useful  for  everyone.    •  Began by entering legacy data:

~300 assays; data from ILIAS, EXO and XENON100

•  Now have ~ 1000 assays, primarily historical. •  Database is being used by SuperCDMS and DarkSide, LZ evaluating it

•  In the process of adding features to the software for easier distributed use.  

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Discussion  Our  funding  supported  specific  projects  which  are  now  being  collected  on  the  integra#on  website.    It  also  supported  twice-­‐a-­‐year  workshops  to  share  resources  and  informa#on    But  AARM  Scien#fic  Collabora#on  has  always  been  a  loose  collec#on  of  scien#sts  involved  in  low-­‐background  studies…    This  will  con#nue    

 Website  is  our  organiza#onal  tool    What  do  you  need??    •  Radiopurity.org      How  can  we  grow  the  database?                                                                              

                 Balance  between  proprietary  vs  open?                    Geant4  material  tools?  

 •  Facility  informa#on  (requires  maintenance  by  manager)  

Requests  from  users  (requires  prompt  response  and  screener  availability)                            

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Discussion  What  do  you  need??    •  Resources:      U#lity  of  one-­‐stop  shopping  

               Hard  to  maintain  –  needs  the  community  to  populate  it                  Need  eyeballs  so  that  your  paper  gets  extra  exposure  there    

•  Community:    How  do  we  construct  a  forum  that  doesn’t  get  hijacked?          Chat  rooms?  Topical  collabora#ve  portals?            Adver#se  your  new  project  or  proposal  and  look  for  collaborators          New  ideas  discussion  thread?    

•  Background  studies:    What  else  should  be  there?                      Do  you  want  your  link  there?    

•  Is  this  sustainable  with  no  funding?            Probably  only  if  the  experiments  themselves  find  this  useful  and          contribute  manpower  and  individuals  find  it  useful        OR  we  could  lobby  for  minimal  funding  as  a  group              How  much  $$  ?  Who  are  the  proposers?