update on diffuse extraterrestrial neutrino flux search with 2000 amanda-ii data
DESCRIPTION
Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data. Jessica Hodges, Gary Hill, Jodi Cooley. - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/1.jpg)
Update on diffuse Update on diffuse extraterrestrial neutrino extraterrestrial neutrino
flux search with 2000 flux search with 2000 AMANDA-II dataAMANDA-II data
Jessica Hodges, Gary Hill, Jodi Cooley
This version of the presentation has been expanded to include work done after the meeting – where part of the nch problem was found to be related to no cross-talk cleaning in the cascade fit
![Page 2: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/2.jpg)
Review of previous workReview of previous work
Jodi Cooley’s thesis work – presented Mons October 2003
Basic quality cuts 2-D cut against coincident muons 2-D cut against nch>50 and positive smoothness – likelihood ratio track/shower vs ldirc 2-D on cogz versus l.r. track/shower model rejection potential optimised on nch
![Page 3: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/3.jpg)
Review of previous workReview of previous work
Cuts developed on 50% of data After nch>80 cut – 6 events on atmospheric background of 3.3 Second 50% of data yielded 4 events Combined 100% data nch>87 – 9 events on atmospheric background of 4.5 One event believed to be a coincident muon What does this excess mean?
![Page 4: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/4.jpg)
New developmentsNew developments Reinvestigation of coincident muons using new dcorsika simulations
Discovery that the nch>50, positive smoothness cut isn’t justified (which was suggested by others earlier!)
Very recently started checking things with second 50% data, but only for nch less than 80 (less than where the cut would be)
![Page 5: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/5.jpg)
The 50<nch<80, The 50<nch<80, positive smoothness positive smoothness
problemproblem
Jodi noticed a bump in the nch distribtion above 50 channels
![Page 6: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/6.jpg)
The 50<nch<80, The 50<nch<80, positive smoothness positive smoothness
problemproblem
nch>50, big excess at positive smoothness
![Page 7: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/7.jpg)
The 50<nch<80, The 50<nch<80, positive smoothness positive smoothness
problemproblem
nch>50, big excess at positive smoothness
![Page 8: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/8.jpg)
First half of data set
ldirc versusl.r. track/shower
![Page 9: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/9.jpg)
First half of data set
ldirc versusl.r. track/shower
![Page 10: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/10.jpg)
Second half of data set
ldirc versusl.r. track/shower
![Page 11: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/11.jpg)
Second half of data set
ldirc versusl.r. track/shower
![Page 12: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/12.jpg)
Summary of the Summary of the 50<nch<80, positive 50<nch<80, positive smoothness problemsmoothness problem
Expect 14.1 atmospheric neutrinos First half data – 35 events Second half data – 15 events After cut – expect 8.2 atmos First half data – 9 events Second half data – 7 events
![Page 13: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/13.jpg)
Summary of the Summary of the 50<nch<80, positive 50<nch<80, positive smoothness problemsmoothness problem
Data Atmospheric neutrinos
Total Pass Fail Total Pass Fail
1. 35 9 26 14.1 8.2 5.9
2. 15 7 8 14.1 8.2 5.9
F. 50 16 34 28.2 16.4 11.8
![Page 14: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/14.jpg)
Summary of the Summary of the 50<nch<80, positive 50<nch<80, positive smoothness problemsmoothness problem
Data Atmospheric neutrinos
Total Pass Fail Total Pass Fail
1. 35 9 26 14.1 8.2 5.9
2. 15 7 8 14.1 8.2 5.9
F. 50 16 34 28.2 16.4 11.8
![Page 15: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/15.jpg)
Summary of the Summary of the 50<nch<80, positive 50<nch<80, positive smoothness problemsmoothness problem
26 events on 5.9 is quite a fluctuation 34 events on 10.8 is as well…. ….even accounting for all the plots I’ve looked at in my life
![Page 16: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/16.jpg)
Second half nch plotSecond half nch plot
![Page 17: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/17.jpg)
First half nch plotFirst half nch plot
![Page 18: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/18.jpg)
Full year nch plotFull year nch plot
Still a bump in the full year
![Page 19: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/19.jpg)
Full year smoothness Full year smoothness plotplot
Still an excess at positive smoothness
![Page 20: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/20.jpg)
Examine the 34 events Examine the 34 events
Look at distributions, both 1 and 2 dimensional See if any of the events lie in “bad” corners of the cut space – indicative of background
![Page 21: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/21.jpg)
line fit velocityline fit velocity
Excess at slow velocities
![Page 22: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/22.jpg)
smoothness, ndircsmoothness, ndircExcess at largest smoothness
Excess at largest ndirc!
![Page 23: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/23.jpg)
likelihood ratios, likelihood ratios, up/down, track/showerup/down, track/shower
Maybe trend to lower ratios
Tendency to lower ratios as seen already
![Page 24: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/24.jpg)
ldirc, ldirbldirc, ldirb
Nothing obviously bad
![Page 25: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/25.jpg)
Cosine zenith, nchCosine zenith, nchMaybe less vertical than expected
Higher nch as observed already
![Page 26: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/26.jpg)
Distributions of the 34 Distributions of the 34 eventsevents
Looks ok
![Page 27: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/27.jpg)
Distributions of the 34 Distributions of the 34 eventsevents
Maybe a pileup toward low speed and high smoothness
![Page 28: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/28.jpg)
Distributions of the 34 Distributions of the 34 eventsevents
No obvious disagreement
![Page 29: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/29.jpg)
My conclusions about My conclusions about nch>50, positive nch>50, positive
smoothnesssmoothness Some of the 34 events are some kind of unsimulated background, some are good track eventsThe difference between the two data halves is certainly a fluctuation on these underlying distributions Hard to imagine a periodic signal that just happens to coincide with our data separation by file numbers
![Page 30: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/30.jpg)
My conclusions about My conclusions about nch>50, positive nch>50, positive
smoothnesssmoothness Some of these events are very nice tracks with long direct lengths Eliminate the original cut – maybe look at cutting on line fit velocity vs smoothness Tighten other cuts Good events will survive to higher levels Bad events will get eliminated elsewhere See what happens in subsequent years
![Page 31: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/31.jpg)
Passing rates with Passing rates with tightened cutstightened cuts
Start with cuts just described Tighten gradually until events disappear Examine passing rates of data and simulation
![Page 32: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/32.jpg)
Passing rates with Passing rates with tightened cutstightened cuts
l.r. up to zenith-weighted downgoing fit - jkchi(12)-jkchi(11) = 35 - 53 ldirb(11) = 10 - 28 ndirc(11) = 155 - 200 | smootallphit(11) | = 0.275 - 0.05 10 cut sets defined (40 - 49)
![Page 33: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/33.jpg)
First half data vs cut First half data vs cut levellevel
![Page 34: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/34.jpg)
Second half data vs cut Second half data vs cut levellevel
![Page 35: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/35.jpg)
Total data vs cut levelTotal data vs cut level
![Page 36: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/36.jpg)
Limit setting potential Limit setting potential versus cut levelversus cut level
E2 (E) < 2.35 10-7
GeV-1 cm-2 s-1 sr-1
![Page 37: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/37.jpg)
The cut against The cut against coincident muonscoincident muons
Original cut: slope 18 New cut: slope 4
![Page 38: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/38.jpg)
The cut against The cut against coincident muonscoincident muons
Original cut: slope 18 MRF : 0.2348
![Page 39: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/39.jpg)
The cut against The cut against coincident muonscoincident muons
New cut: slope 4 MRF : 0.2379
![Page 40: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/40.jpg)
Outlook for the 2000 Outlook for the 2000 diffuse analysisdiffuse analysis
Some sort of weird effect was seen in the 1st 50%, but not in the 2nd
Eliminate the problematic cut Tighten cut against coincident muons
![Page 41: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/41.jpg)
Explanation of one part Explanation of one part of the nch>50, positive of the nch>50, positive smoothness problemsmoothness problem
Clue (Doug Cowen) – cascade fit is very sensitive to noise hits If the Monte Carlo and data have slightly different noise, then a cascade fit comparison might not make sense
![Page 42: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/42.jpg)
The cascade fit was The cascade fit was performed before the performed before the cross talk filter was cross talk filter was
applied!applied! Cascade fits on data have been done with all the cross talk present Monte Carlo contains no cross talk Likelihood ratios based on different hit selections make no sense
![Page 43: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/43.jpg)
track/shower l.r. before track/shower l.r. before nch>50 cutnch>50 cut
Dramatic improvement in the agreement of this variable!
![Page 44: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/44.jpg)
Bump in nch, correlates Bump in nch, correlates with excess at positive with excess at positive
smoothnesssmoothness
![Page 45: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/45.jpg)
track/shower l.r., ldirc track/shower l.r., ldirc vs t/s l.r. for nch>50, vs t/s l.r. for nch>50, positive smoothnesspositive smoothness
![Page 46: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/46.jpg)
Same plots, with Same plots, with consistent cross talk consistent cross talk
cleaningcleaning
![Page 47: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/47.jpg)
Data and simulation now agree! (in shape)
![Page 48: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/48.jpg)
Where they did not before
![Page 49: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/49.jpg)
Place a new cut – data and atmos neutrinos are now both split about 50:50 about this cut
![Page 50: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/50.jpg)
Place a new cut – data and atmos neutrinos are now both split about 50:50 about this cut
![Page 51: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/51.jpg)
Place a different cut – excess now shows up in corner, but that’s where the E-2 is more prevalent…
![Page 52: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/52.jpg)
Place a different cut – excess now shows up in corner, but that’s where the E-2 is more prevalent…
![Page 53: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/53.jpg)
Examine the 22 events in Examine the 22 events in the cornerthe corner
![Page 54: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/54.jpg)
Examine the 22 events Examine the 22 events in the cornerin the corner
![Page 55: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/55.jpg)
![Page 56: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/56.jpg)
Examine the 22 events Examine the 22 events in the cornerin the corner
![Page 57: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/57.jpg)
Examine the 22 events Examine the 22 events in the cornerin the corner
![Page 58: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/58.jpg)
Examine the 22 events Examine the 22 events in the cornerin the corner
![Page 59: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/59.jpg)
![Page 60: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/60.jpg)
Scanning of the events inside the green circle reveals some indication of residual cross talk – a classic “string 9/10 event”
![Page 61: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/61.jpg)
![Page 62: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/62.jpg)
New conclusionsNew conclusions
Once the cascade fit is correctly performed using the cross talk filtering selection, the excess of events at nch>50 and positive smoothness moves to the low l.r. / low ldirc corner of the 2D plot - which could be indicative of background However, this is the region where the E-2 signal prediction is expected to cluster We cannot cut this region away!
![Page 63: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/63.jpg)
![Page 64: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/64.jpg)
![Page 65: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/65.jpg)
![Page 66: Update on diffuse extraterrestrial neutrino flux search with 2000 AMANDA-II data](https://reader035.vdocuments.site/reader035/viewer/2022062309/56814f0a550346895dbc9e6e/html5/thumbnails/66.jpg)