Resource Type
Lesson
Region
Antarctic
Completion Time
About 1 period
Grade
High school and Up
Permission
Download, Share, and Remix
Related Members
Materials
Worksheet: Build a Particle
Worksheet: Particle Flashcards
Scissors
Markers (Optional)
Quiz
Access to a computer (with internet)
Topic
Physical Science

Overview

In this lesson, students will be introduced to the Standard Model, learning key vocabulary such as Fermions, Hadrons, Mesons, Baryons, Quarks, Leptons, particles, and anti-particles. In particular, students will come to understand what a neutrino is and why it is such a unique particle. This understanding connects to the IceCube Neutrino Observatory’s search for neutrinos in an effort to learn something new and different about the universe. (This lesson is ideal for an upper-level, i.e. AP or IB, Physics or Chemistry class)

Objectives

  1. Understand the organization of the Standard Model.
  2. Correctly use relevant vocabulary such as fermion, hadron, lepton, quark, baryon, meson, particle, and anti-particle.
  3. Discuss why neutrinos are unique and how this serves as an advantage and disadvantage to the IceCube Neutrino Observatory.
    (Note: This lesson is particularly relevant to the IB Physics curriculum, Subtopic 7.3)

Lesson Preparation

Students should go to www.particleadventure.org and read the section on “The Standard Model” before coming to class. This will give students preview of the content.

Procedure

  1. Review relevant vocabulary from the pre-reading, including fermions, hadrons, leptons, quarks, particles and anti-particles.
  2. Discuss how quarks can combine in certain ways to form new, more complex particles.
  3. Students explore ways of combining quarks using bit.ly/BuildaParticle. They should record their findings (combination of quarks, was a particle created?, and, if so, the name of the particle) on the provided worksheet. This will help students begin to look for patterns as well become familiar with the names of various baryons and mesons. (see Worksheet: Build a Particle)
  4. After giving students time to explore, ask them to pull out patterns they see for mesons and baryons and record at the bottom of the provided worksheet.
  5. Discuss these patterns as a class. Students should have discovered that three particles or anti-particles can combined to form a baryon and a particle/anti-particle pair can combine to form a meson.
  6. Discuss how each particle has specific properties. Pull on prior knowledge of charge, and add new properties such as lepton number (leptons=+1, anti-leptons=-1, non-leptons=0), baryon number (baryons=+1, anti-baryons=-1, non-baryons=0), and strangeness (strange quark=-1, anti-strange quark=+1).
  7. Using the IB Physics Data Booklet (or other online resources if not an IB course), students should create flashcards recording the name, category, charge, lepton #, baryon #, and strangeness of common particles. Option: have students color/decorate the flashcards (see Worksheet: Particle Flashcards) (note to teacher: print the worksheet front-to-back in order to line up the particle with the properties on the back)
    (note to teacher: although students will likely not fully understand lepton #, baryon #, or strangeness at this point in time, later lessons could focus on conservation of these quantitates to further understanding)
  8. Discuss what makes neutrinos so special: Students should notice from their flashcards that neutrinos have a charge of 0. Connect this to prior knowledge about about electric and magnetic fields – neutrinos would not change their direction when traveling through electric or magnetic fields. Ask students to look up to the mass of neutrinos – they’ll find it’s nearly zero. Connect this to prior knowledge about gravitational fields – neutrinos would not change their direction when traveling through gravitational fields.
  9. Discuss: Why might these two properties of neutrinos, chargeless and nearly massless, be helpful when trying to study the universe? Why might IceCube be interested in neutrinos in particular? Answer: wherever these neutrinos are coming from, they’ll travel in a straight path, unobstructed by fields, to earth. This makes it really easy to trace a detected neutrino back to its source.
  10. Discuss: Why might these two properties of neutrinos, chargeless and nearly massless, pose a problem to scientists? Answer: hard to detect!
  11. Next, students should cut out the labels on the last page of the worksheet. Using these labels, ask students to organize the flashcards in a way that makes sense to them. (Formative assessment: check that students are correctly using the vocabulary words.)
  12. How do physicists organize these particles? Present students with various different Standard Model representations. (suggested links: Table, Web, Traditional table, Traditional Chart). Discuss the pros and cons of each type of representation. What is your favorite? Why?
  13. Present alternative way of discussing the standard model by playing the Quark Song.

Extension

Students create another representation that includes the vocabulary fermions, leptons, quarks, mesons, baryons, and hadrons. Encourage creativity! (ideas could include a family album, baseball cards, etc.)

Resources

Assessment

  • Formative Assessment (in #10 in above lesson plan): check that students are correctly using the vocabulary words as they sort their flashcards using the labels
  • Formative Assessment: mini-quiz (download entire lesson PDF) given the following class to assess student’s knowledge of the Standard Model as well as their use of vocabulary.

Author/Credits

This lesson was modified by Kate Miller (contact: kate.miller [at] polartrec.com) from resources produced by the KSTF IB Physics Collaboration (including Heather Hotchkiss, Mark Hartman, Jennifer Goetz, Nick Guendel, Christine Scott, and Katelyn Warner)

Standards Other

IB Curriculum

IB Physics SL / HL curriculum, Sub-Topic 7.3: The Structure of Matter

Aim 1: the research that deals with the fundamental structure of matter is international in nature and is a challenging and stimulating adventure for those who take part
Aim 4: particle physics involves the analysis and evaluation of very large amounts of data
Aim 6: students could investigate the scattering angle of alpha particles as a function of the aiming error, or the minimum distance of approach as a function of the initial kinetic energy of the alpha particle
Aim 8: scientific and government organizations are asked if the funding for particle physics research could be spent on other research or social needs


This program is supported by the National Science Foundation. Any opinions, findings, and conclusions or recommendations expressed by this program are those of the PIs and coordinating team, and do not necessarily reflect the views of the National Science Foundation.