Measurement of the Atmospheric Muon Neutrino Energy Spectrum with IceCube in the 79- and 86-String...

Post on 13-Jan-2016

212 views 0 download

Tags:

transcript

Measurement of the Atmospheric Muon Neutrino Energy Spectrum with IceCube in the 79- and 86-String Configuration

Tim Ruhe, Mathis Börner, Florian Scheriau, Martin Schmitz, TU Dortmund

Flu

x

Energy

2

Outline

IceCube and atmospheric neutrinos Event Selection Spectrum Unfolding Results Summary and Outlook

3

IceCube and atmospheric neutrinos

Tim Ruhe | Statistische Methoden der Datenanalyse

4

Data Preprocessing

Cut on zenith angle > 86°

Redcution of the data volume,

BUT remaining background is significantly harder to reject

Additional cuts:

Lepton velocity Empty Hits Truncated Energy (estimator) Track length

5

Feature Selection Stability

BA

BAJ

Jaccard:

Average over many sets of variables:

Number of Variables

Jacc

ard

Inde

x

6

Training and Validation of a Random Forest

treesn

ii

trees

sn

s0

1

use an ensemble of simple decision trees

Obtain final classification as an average over all trees

7

Random Forest Output

200 trees 5 Random Features per node 120,000 signal events 30,000 background events

Forest Settings:

8

Random Forest Output (IC79)Find a trade-off between background

rejection and signal efficiency

Place a cut at confidence >=0.92

212 neutrino candidates per day 66885 neutrino candidates in total 330±200 background muons

9

Random Forest Output (IC86)

2-dimensional cut

289 neutrino candidates per day 92060 neutrino candidates in total 410±220 background muons

10

Why unfold?

Muon production governed by stochastical processes

Energy losses on the way towards the detector

Finite resolution Limited acceptance of the

detector

Inverse Problem, to be solved with TRUEE.

11

Unfolding Input (1): Energy Correlation

Input variables show good correlation with energy

12

Unfolding Input (2): Background Distributions for IC79

Tim Ruhe | Statistische Methoden der Datenanalyse

Background events are located at lower energies

Therefore, they do not affect the highest energy bins

13

Unfolding Input (3): Background Distributions for IC86

Background events are located at lower energies

Therefore, they do not affect the highest energy bins

14

Unfolding Input (3): Background Distributions for IC86

15

Unfolding the spectrum

TRUEE

3 energy dependent input variables

TRUEE

Clear deviation from an atmospheric only prediction

16

More results

Combining the spectra

Unfolding different zenith bands

17

Summary and Outlook

Random Forest &MRMR

TRUEE

18

Backup

Tim Ruhe | Statistische Methoden der Datenanalyse

19

IC86 Precuts

Tim Ruhe | Statistische Methoden der Datenanalyse

20

IC79 Precuts

Tim Ruhe | Statistische Methoden der Datenanalyse

21

Comparison to other measurements

Tim Ruhe | Statistische Methoden der Datenanalyse

22

Relevance vs. Redundancy: MRMR (continuous case)

Relevance: Redundancy:

MRMR: or

23

IC86 Confidence Distributions

Tim Ruhe | Statistische Methoden der Datenanalyse

24

Unfolding Input for IC86

Tim Ruhe | Statistische Methoden der Datenanalyse

25

IC86 2D Cut

Tim Ruhe | Statistische Methoden der Datenanalyse