This and the ATLAS and CMS pages help to guide mentors and teachers in planning the masterclass.

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• Common Elements
• Table of Institutes

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Additional measurements:    ALICE Raa     ALICE Strange Particles     ATLAS W     CMS J/Psi     LHCb

Find useful general information on International Masterclasses from Local Organisation in the IMC website.

Elements common to all masterclass institutes

Previous to day of the masterclass:

• Orientation for mentors and teachers by QuarkNet staff or fellow (1-3 hr)
• Classroom preparation of students by teacher (~3 hr)

Masterclass day (6-8 hr):

• Registration (sign-in sheet) and gateway activity (e.g. cloud chamber, cosmic ray detector, or e/m apparatus)
• Icebreaker activity
• Mentor presentation (a bit of standard model, a bit of mentor's own research)
• Lab tour
• Teacher presentation on masterclass measurement (ATLAS Z-path, CMS WZH-path, or other)
• Lunch with a physicist
• Masterclass measurement by students with help from mentor, teachers, other physicists 
• Discussion of combined results for Institute
• Videoconference
• Wrap-up

Masterclass 2016 Institutes in Fermilab group (update for 2017 forthcoming)

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This page is to help to guide teachers in preparing students for their masterclass.

Navigation

• Objectives
• Suggested activities
• Additional resources
• Get the word out

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Prior knowledge for masterclasses / Classroom prep objectives

Meeting these objectives will assure that students are well prepared for the masterclass.

• Describe the claim and indirect evidence in Rutherford's or another key experiment.
• Identify the peak in a histogram and explain what it means.
• Describe how quarks combine to form mesons and baryons.
• Apply conservation rules to measurements to provide evidence for unobserved particles.

Suggested activities

Particle physics research requires the use of indirect evidence to support claims.
Rolling with Rutherford
Students will be able to:

• Describe the claim and indirect evidence in Rutherford’s experiment.
• Identify the peak in a histogram and explain what it means.

The Standard Model is the current theoretical framework for our understanding of matter.
Quark Workbench 
Students will be able to:

• Describe how quarks combine to form mesons and baryons.

The behavior of particles is governed by conservation laws and mass-energy conversion.

Choose one or both:

• Mass Calc: Z 
• Top Quark Mass Reconstruction 

Students will be able to:

• Apply conservation rules to measurements to provide evidence for unobserved particles.

Additional resources

• ATLAS Masterclass website
• CMS videos
• ATLAS videos
• The Particle Adventure
• Bubble Chamber Activity
• Hands-on CERN

Get the word out about International Masterclasses!

IMC Poster (PDF) - plain Large (11"x17") Large (A3) Small (8.5"x11") Small (A4)

IMC Poster (PDF) - U.S. logos Large (11"x17") Small (8.5"x11")

IMC Poster (doc) - editable Large (A3) Small (A4)

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This page is to help to guide mentors in preparing their teams, including teachers, for the masterclass.

Navigation

• New Institutes
• Experienced Institutes
• Orientation Schedule
   

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New Institutes: Masterclass Orientation

A masterclass orienation can be done online via Vidyo or in person with a visit from a QuarkNet staff member or fellow. It is intended for teachers and mentors. Here is what is covered:

• Classroom prep for the masterclass
• Try out an ATLAS or CMS masterclass measurement
• Walk-through of masterclass logistics
• Masterclass Library
• Vidyo test
• Q&A

This generally takes 3-6 hours, though it can be trimmed or extended depending on needed. If you are doing a CMS or ATLAS Data Workshop in the masterclass orientation period, it counts as an orientation. If you had one previous to this, you only need an orientation update (below).

Register for Masterclass Orientation on the Google form at least one week prior to your earliest preferred date!

Experienced Institutes: Orientation Updates

An orientation update is to bring teachers and mentors up to speed on the latest in masterclass measurements and procedures. As orientation updates are done online, they also serve as Vidyo tests. Orientation updates take 1-2 hours.

Register for Masterclass Orientation on the Google form at least one week prior to your earliest preferred date!

Orientation Schedule 2017

Orientation Indico pages:

• ATLAS: https://indico.cern.ch/e/atlor17
• CMS: https://indico.cern.ch/e/cmsor17.

Start time in CT and facilitator in parentheses. New registrants: we can accommodate days and times not yet shown on this schedule.

* Site visit.

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This page is to help to guide mentors in preparing their teams, including teachers, for the masterclass.

Navigation

• Key elements
• Resources
• Narrative
• Objectives

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Key elements

• Start early - October is good for a masterclass the following March.
• People - assemble a team of physicists, students, and high school physics teachers.
• Schedule - check your Institution and have teachers check their school for a good masterclass date.
• Ratios - one mentor or tutor per maximum 10 students, one computer per 2 students.
• Preparation - orientation for your team, into activities for students before masterclass.
• Vidyo - arrange what you need for the masterclass videoconference and have a Vidyo test using the same place and equipment.
• Organize - a place for students to work, tours of labs, presentations, lunch together (plus snacks, drinks etc), etc.

Resources

• International Masterclasses website
• IMC Coordinators Uta and Ken

Narrative

"I let myself in."

I looked up. In the waning light of that early October day, I could tell that a particle physicist had just entered my office. 

"Yeah, welcome," I said, "but I have papers to grade."

"Grade them later. Right now, let me tell you a story," replied the CMS genius.

"Okay. Talk." I sat back and dropped the red pen on the desk. I took a long, slow sip of my cold coffee.

"I have a gig with the LHC, and you have high school physics students. We're going to do a masterclass. I'll check my March calendar, you check yours, and let's find a good day to bring your most motivated. We'll sign up on the Doodle poll. After the New Year, we'll prep some. You and I and the team will have an orientation to learn about the masterclass. Then, you'll give your students some activities to familiarize them with particle physics and prepare them for the masterclass, where they'll use actual LHC data. With me so far?"

"Yeah, I'm interested, Doc." 

"Good. On the date we pick, we'll have the students at the Institute the whole day. We'll start them with a cloud chamber and work up to the Standard Model in a presentation I'll give. Then, we'll let them tour a bit (everyone loves the laser lab on the third floor and the Van der Graff in the basement) and have lunch."

"Lunch, good," I said. "Lunch with a physicist will be a great event for the students."

"In the afternoon, you will lead the students and show them how to analyze the LHC data. Yes, you can do it. After that, we turn them loose on data before I lead them in a physics discussion of the results. They will cap it off with a videoconference with other masterclass institutes and with moderators at CERN or Fermilab. Sound like a plan?"

"It's a plan. You had me at LHC. Now let me finish these quizzes."

Keep in mind

Here is what we hope to achieve with a masterclass from an educational point of view . . .

Enduring Understandings from the Masterclass

These are points we want students to remember long after the masterclass.

1. Particle physics research requires the use of indirect evidence to support claims.
2. The Standard Model is the current theoretical framework for our understanding of matter.
3. The behavior of particles is governed by conservation laws and mass-energy conversion.

Learning Objectives

These are things we want students to be able to do as a result of the masterclass.

After the masterclass activity students will be able to:

1. Explain that a general-purpose collider detector is made of a number of subsystems and describe what they are designed to measure.
2. Express an increased appreciation for the nature of scientific investigation.
3. Describe features of the Standard Model—which particles are which and how they relate to one another.
4. Identify specific particles and their decays by their signatures.
5. Give examples of how hadrons or force carriers can decay into different types of leptons.
6. Describe/show how conservation laws, behavior of particles in a magnetic field and energy-mass conversion apply to particle physics.
7. Give examples of conservation of charge in particle decays.

Go to Project Map

The Masterclass Library contains most of the information needed for physicists and teachers to run a masterclass. The Project Map below is arranged in the typical chronological order in which a masterclass prepared and then carried out.  The order is more descriptive than prescriptive.

The Project Map has 6 "metro stops" plus several associated branches. The main metro stops are:

• Planning gives an overview of how to get masterclasses organized and going.
• Orientation explains orienting of teachers and physicsts to run a masterclass and provides schedule information.
• Classroom Preparation details how teachers get their students ready for the masterclass.
• Institute and Videocon with their branches cover the main elements of the masterclass day. These make up the heart of the Project Map.
• Follow on shows what students can do to continue their exploration of particle physics after the masterclass. 

Register:

• for Orientation and Vidyo testing on the Orientation page
• for Masterclass videoconferences on the Videocon page
• or contact Ken Cecire and Uta Bilow.

Get a poster!