A Tale of Two Anomalies: from LHCb to ANITA Speaker: Yicong Sui In - - PowerPoint PPT Presentation

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A Tale of Two Anomalies: from LHCb to ANITA Speaker: Yicong Sui In - - PowerPoint PPT Presentation

Jan 26, 2023 362 likes •1.14k views

A Tale of Two Anomalies: from LHCb to ANITA Speaker: Yicong Sui In collaboration with: Wolfgang Altmannshofer, Bhupal Dev, Amarjit Soni 27th International Conference on Supersymmetry and Unification of Fundamental Interactions May 20-24th,

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SLIDE 1

A Tale of Two Anomalies: from LHCb to ANITA

Speaker: Yicong Sui In collaboration with: Wolfgang Altmannshofer, Bhupal Dev, Amarjit Soni 27th International Conference on Supersymmetry and Unification of Fundamental Interactions May 20-24th, 2019

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Introduction of B-anomaly

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SLIDE 3

Introduction of B-anomaly

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SLIDE 4

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766

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SLIDE 5

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 Florian U. Bernlochner, etl, 1703.05330

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SLIDE 6

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 PDG2018 Florian U. Bernlochner, etl, 1703.05330

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SLIDE 7

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 PDG2018 Florian U. Bernlochner, etl, 1703.05330

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SLIDE 8

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 PDG2018 Florian U. Bernlochner, etl, 1703.05330

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SLIDE 9

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 PDG2018 Florian U. Bernlochner, etl, 1703.05330

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SLIDE 10

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 PDG2018 Florian U. Bernlochner, etl, 1703.05330 Marzia Bordone, Gino Isidori, Andrea Pattori, 1605.07633

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SLIDE 11

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 LHCb collaboration, 1903.09252 PDG2018 Florian U. Bernlochner, etl, 1703.05330 Marzia Bordone, Gino Isidori, Andrea Pattori, 1605.07633 LHCb collaboration, 1705.05802

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SLIDE 12

Introduction of B-anomaly

Gregory Ciezarek, etl, , 1703.01766 LHCb collaboration, 1903.09252 PDG2018 Florian U. Bernlochner, etl, 1703.05330 Marzia Bordone, Gino Isidori, Andrea Pattori, 1605.07633 LHCb collaboration, 1705.05802

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The ANITA detection concepts, figure from Cosmin Deaconu

Introduction of ANITA anomaly

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The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Introduction of ANITA anomaly

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SLIDE 15

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 16

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 17

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 18

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 19

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 20

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

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SLIDE 21

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

l

S M

~ 300 km (in rock)

R ~ 6400 km D = 2R cos(θ) > 5700 km

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SLIDE 22

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

Psurvival ~ 10-6

l

S M

~ 300 km (in rock)

R ~ 6400 km D = 2R cos(θ) > 5700 km

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SLIDE 23

The ANITA detection concepts, figure from Cosmin Deaconu

Table from ANITA, 1803.05088

Properties of the anomalous upward events 1.Large Elevation Angle, going upwards. 2.No Polarity Reverse Relative to Geomagnetic Field. 3.Both have large energy~0.5EeV 4.Both interpreted as tau events by ANITA

Introduction of ANITA anomaly

Psurvival ~ 10-6

= 0.0001% l

S M

~ 300 km (in rock)

R ~ 6400 km D = 2R cos(θ) > 5700 km

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SLIDE 24

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 25

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

Long-lived neutral particle + TeV level mediator particle

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 26

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

Long-lived neutral particle + TeV level mediator particle

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 27

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

λ geff Long-lived neutral particle + TeV level mediator particle

  • M. Carena, D. Choudhury, S. Lola, C. Quigg, Hep-ph/9804380;
  • P. S. Bhupal Dev, Dilip Kumar Ghosh, Werner Rodejohann.1605.09743

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 28

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

λ geff Long-lived neutral particle + TeV level mediator particle

  • M. Carena, D. Choudhury, S. Lola, C. Quigg, Hep-ph/9804380;
  • P. S. Bhupal Dev, Dilip Kumar Ghosh, Werner Rodejohann.1605.09743

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 29

RPV-SUSY

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

λ geff Long-lived neutral particle + TeV level mediator particle

  • M. Carena, D. Choudhury, S. Lola, C. Quigg, Hep-ph/9804380;
  • P. S. Bhupal Dev, Dilip Kumar Ghosh, Werner Rodejohann.1605.09743

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 30

RPV-SUSY

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

λ geff Long-lived neutral particle + TeV level mediator particle

  • M. Carena, D. Choudhury, S. Lola, C. Quigg, Hep-ph/9804380;
  • P. S. Bhupal Dev, Dilip Kumar Ghosh, Werner Rodejohann.1605.09743

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 31

RPV-SUSY

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

λ geff Long-lived neutral particle + TeV level mediator particle

  • M. Carena, D. Choudhury, S. Lola, C. Quigg, Hep-ph/9804380;
  • P. S. Bhupal Dev, Dilip Kumar Ghosh, Werner Rodejohann.1605.09743

New Phyiscs Interpretation to ANITA-anomaly

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SLIDE 32
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LLE senario

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

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LLE senario

Jack Collins and Bhupal Dev, Yicong Sui, 1810.08479

LQD senario

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RPV-SUSY Interpretation to B-anomaly: RD RD*

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RPV-SUSY Interpretation to B-anomaly: RD RD*

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RPV-SUSY Interpretation to B-anomaly: RD RD*

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SLIDE 38

RPV-SUSY Interpretation to B-anomaly: RD RD*

N.G. Deshpande, Xiao-Gang He, 1608.04817

  • W. Altmannshofer, P. S. Bhupal Dev and A. Soni, 1704.06659

Sokratis Trifinopoulos, 1807.01638

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SLIDE 39

RPV-SUSY Interpretation to B-anomaly: RD RD*

N.G. Deshpande, Xiao-Gang He, 1608.04817

  • W. Altmannshofer, P. S. Bhupal Dev and A. Soni, 1704.06659

Sokratis Trifinopoulos, 1807.01638

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SLIDE 40

RPV-SUSY Interpretation to B-anomaly: RD RD*

N.G. Deshpande, Xiao-Gang He, 1608.04817

  • W. Altmannshofer, P. S. Bhupal Dev and A. Soni, 1704.06659

Sokratis Trifinopoulos, 1807.01638

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SLIDE 41

RPV-SUSY Interpretation to B-anomaly: RK RK*

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RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 44

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 45

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 46

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 47

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 48

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343

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SLIDE 49

RPV-SUSY Interpretation to B-anomaly: RK RK*

Diganta Das, Chandan Hati, Girish Kumar, and Namit Mahajan, 1705.09188 Kevin Earla, Thomas Gr´egoirea, 1806.01343 Sokratis Trifinopoulos, 1807.01638

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independents

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independents

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independents parameters

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independents parameters

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independents parameters

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independents parameters

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Possible Constraints

independents parameters

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Possible Constraints

Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 62

Possible Constraints

Heavy Flavor Averaging Group, etl, 1612.07233 Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 63

Possible Constraints

Heavy Flavor Averaging Group, etl, 1612.07233 Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 64

Possible Constraints

Dario Buttazzo, etl, 1706.07808 Heavy Flavor Averaging Group, etl, 1612.07233 Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 65

Possible Constraints

Dario Buttazzo, etl, 1706.07808 Heavy Flavor Averaging Group, etl, 1612.07233 Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 66

Possible Constraints

Dario Buttazzo, etl, 1706.07808 Heavy Flavor Averaging Group, etl, 1612.07233 Sokratis Trifinopoulos, 1807.01638

independents parameters

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SLIDE 67

Conclusion:

1.Under the framework of RPV-SUSY, ANITA anomaly has quite large parameter space, which is in the simlar range demanded by RD and RK. 2.Rk Rk* and RD RD* anomalies could be explained simultaneously after a “fourth term” is included in the traditional RPV-SUSY Rk Rk* expression. 3.Under the simplified parameter setup, we find that there exist parameter spaces that could satisfy RK-RD-ANITA altogether. 4.Relaxing the parameter setup and letting more lambda’ running free could possibly lead to larger preferred region for the parameters. 5.This framework could also be expanded to include muon g-2 anomaly

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B, Anomaly Anita, Anomaly

Hey, B. Are we related?

RPV- SUSY

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BK slides-Constraints

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BK slides-Constraints

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BK slides-Constraints

1706.07808 eq 50

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BK slides-Constraints

1706.07808 eq 50

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BK slides-Constraints

1706.07808 eq 50 1807.01638

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BK slides-Constraints

1706.07808 eq 50 1807.01638

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BK slides-Constraints

1706.07808 eq 50 1807.01638 1807.01638