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Summer outreach programme & Education Initiatives

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Our Team

Samyak Mohanty, Ved Rathi, Arya Rathi, Suchir Divekar

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Our Projects

Hardware design for affordable, deployable muon detector replacing dry ice with gel-compartment.

Design and construct a lower-cost alternative to current models with focus on durability and portability.

DIY Cloud Chamber Kit

Cosmic ray Muon Detector

Video scripts, teacher guides and student worksheets aligned to Indian board curricula. Focused on developing foundational particle physics understanding

Lecture series

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Pitch Decks

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Lecture Series

Cloud Chamber Kit

Administration

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Lecture Series

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Establishing a particle physics lecture series for high school students.

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Addressing Gaps

Special Relativity

  • Explained key concepts: Lorentz Factor, Time Dilation, and Length Contraction.
  • Essential in understanding the arrival of muon at sea level

Conservation laws

  • While charge, energy, and momentum conservation laws were covered, students lacked understanding of lepton number conservation principle.

Ionizing Radiation and Track Formation

  • Explaining the mechanism of ionization along a particle track
  • Introducing the concept of supersaturated vapour and nucleation in ion pairs.

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VIDEO SNAPSHOTS

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Learning Outcomes

  • The scope of the project consists of Tier 1 & 2 cities in india.
  • The Urban-rural resource gap was factored into the
    • Detector kits and
    • Bill of materials.
  • Finally, the deliverables aimed to foster an understanding of basic fundamental particle physics concepts and working of detectors, cloud chambers.

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Cloud Chamber

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Typical Cloud Chamber

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CLOUD CHAMBER - S'Cool LAB - DIY manual on Cloud Chamber

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Basic Components of a cloud chamber

Enclosure

Thermal Insulation

Observation Region

Control heat flow using felt cloth to improve efficiency.

Vapor Source

High-purity isopropyl alcohol (99.9%) or ethanol

Thermal Gradient System

Create a warm-top and cold-bottom environment.

Light Source

Makes tracks visible.

Safety Equipment

Makes tracks visible.

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Our Proposition

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Iterations

Why model was not feasible

  • Minimum Temperature was not achieved by cooling in a normal refrigerator
  • Maintaining and cooling of the gel pack for sufficient time was not operational

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Possible Observations in a Cloud Chamber

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Alpha

Muon

Electron

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Image Source:CERN S’CoolLAB & KIT (via PhysicsOpenLab)

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Cloud Chamber Analysis

Simple experiments and measurements using particle tracks.

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Track Length (Range)

  • Measure total track length of a particle
  • Compare the tracks of various particles
  • Alpha particles stop inside the cloud chamber, whereas most other particles do not
  • The energy of the alpha-particle can be estimated using the range-energy tables.

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Energy Loss

  • Measure track width or brightness along its length.
  • Alpha particles become brighter near the end of their range due to increased ionization.
  • Compare the ionization patterns of different particle types.

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Track end much brighter than the beginning.

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Helping BBLC students with making an actual model of a Muon cloud chamber.

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Cost Breakdown for Dry ice model

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COMPONENT

COSTING IN INR

Clear acrylic / glass / fish tank

₹700

Black felt or velvet cloth

₹200

Isopropyl Alcohol (IPA) 99%

₹200 (for 500 ml)

LED / Torch (side illumination)

₹400

Sponge / foam strip

₹35

Rubber gloves + tongs + safety goggles

₹435

Base tray

₹470

Dry ice

₹150 (per KG)

Instruction booklet (printed)

₹10-20

Transportation and packaging

₹350-400

Total cost estimation

₹3000 (approx)

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Muon Detector Working

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COMPONENT

COSTING IN INR

Plastic scintillator tile

₹3000

Silicon Photomultiplier (SiPM)

₹16,000 (₹4000 for single tile)

Optical coupling grease / wrap

₹1500

Front-end electronics / ASIC

₹5800

Arduino / Raspberry Pi

₹1500

Power supply (battery or USB)

₹950

Enclosure / housing

₹2800

Total cost estimation

₹32,000 (approx)

Cost Breakdown for the Detector

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Photodetector Choice

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  • Our Choice: SiPM over PMT
  • SiPMs (Silicon Photomultipliers) are strongly preferred for portable detectors.
  • They operate at 25–70 V (vs. ~1000 V for PMTs)
  • They are compact, robust.
  • More Cost Effective

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Visiting detector labs at CERN

CERN uses SiPMs and PMTs across multiple experiments, including the LHCb SciFi tracker and detectors in proposed future colliders , but these devices are generally manufactured by specialized external suppliers such as Hamamatsu, SensL, and EXCELITAS rather than in CERN’s GEM laboratory.

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Thank you�Open for questions

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Credits and Sources

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  • https://ppc.web.cern.ch/
  • https://scoollab.web.cern.ch/sites/default/files/documents/20200521_JW_DIYManual_CloudChamber_v7.pdf
  • https://arxiv.org/pdf/2111.10151