Workshop implementation Robert F Preston, ID High School

Workshop Location:  Preston, ID

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.):  This is an AP Statistics course. The student should have already been introduced to presenting numbers in a variety of formats, including equations and graphs. In this lesson, which is expected to last approximately 4 class periods, the student will work in groups of 4-5 to not only plot data using a histogram, but they will interpret their results and present the results to the class by poster and presentation software (e.g. powerpoint).

Grade(s)/Context:  11/12 Stats Class

Challenges:  Giving enough science background to make the data meaningful, yet not too much to digress from course outline

When/Where: 2nd semester 2011/12

Learning Objectives:The student will plot a histogram of cms data.

The student will interpret the plotted data.

While plotting the histogram is a worthwhile endeavor, a goal of the course is to discriminate the appropriate data within the appropriate headings. If necessary the student should perform calculations using measured data. The student will describe the calculations and present the results as a poster and in a 5 minute group presentation.

Standards:

The state standards (emphasis added)

I. Exploring Data: Describing patterns and departures from patterns.

A. Constructing and interpreting graphical displays of distributions of univariate data (dotplot, stemplot, histogram, cumulative frequency plot)

II. Sampling and Experimentation: Planning and conducting a study.

A. Overview of methods of data collection

B. Planning and conducting surveys

C. Planning and conducting experiments

D. Generalizability of results and types of conclusions that can be drawn from observational studies, experiments, and surveys

As stated in the Learner Objectives the student will construct a histogram(s). The design of the histogram and preparation of the poster will include the information of the method of data collection and the conclusions that can be acquired.

Steps:  

The student will use data assigned to determine: first, what is the data; second is the data categorical or quantitative; third, when, where and how the data was collected. The student should come to understand the answers to the previous questions to determine if additional results are needed to be tabulated. As each group makes conclusions regarding their data, they will submit a proposal to begin the analysis phase of the project.

The student, following their proposal, will calculate the additional information if necessary and create histograms of varying bin widths of the data. Using the histograms showing what was measured, the groups will infer reasonable conclusions and submit a draft of the poster.

Once approved, the groups will be allowed to continue work on the poster and preparing for the presentation portion of the project. The time of their presentation was selected when the data was first disbursed.


Follow-Up Date:

6 Apr 2012

 

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Watching…

08:09 ET…I’m at Notre Dame on the 4th floor of the Nieuwland Science Hall where the particle physics group has gathered to watch the CERN webcast of the ATLAS-CMS seminar. Fabiola Giannoti, ATLAS spokesperson, is giving the ATLAS part of the presentation, showing agreement with the Standard Model at 7 TeV…

08:25 ET…talking about Higgs —> gamma gamma possibilities. Something at 126 GeV?

08:47 ET…ATLAS talk ending. Higgs mass restricted to 115.5-131 GeV with a possible bumo at 126 GeV. More data in the coming year will tell if we really have a Higgs in this range.

08:49 ET…Guido Tonnelli, CMS spokesperson, has just greeted Fabiola and taken the floor.

09:07 ET…talk well underway. CMS really looked at every possible signal, even ZZ to 3 electrons and a tau. That signal is one tough hombre.

09:10 ET…looking at low mass Higgs possibilities now…

09:16 ET…H–>ZZ, the Golden Channel.

09:18 ET…small excess there.

09:35 ET…Combined data: modest excess at 115-127 GeV, cannot exclude Higgs.

09:43 ET…Questions have begun. One comment from the audience at CERN: “Thank you for your very nice Christmas gift and I hope you will not take it back.”

09:50 ET…Conclusion by CERN DG Rolf Heuer: great work but be careful as we do not have discovery or exclusion yet.

09:53 ET…There is lots of discussion now here at Notre Dame. Stay tuned.

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Preparing to discuss the Higgs

a Higgs to ZZ event candidate
As we look forward to Tuesday’s upcoming discussion at CERN of the state of the investigation into the Higgs, it is interesting to read a theorist’s view of the matter. Joe Lykken is not just any theorist, but one of a handful who are part of the CMS collaboration. This interview sheds light not only on Higgs and the upcoming announcement, but also on the nature of science. Consider reading it before Tuesday. If you have time for another, this NY Times article features Lisa Randall’s comments.

Also, CMS member and blogger Tommaso Dorigo offers this glossary of terms to prepare for Tuesday’s announcement. The glossary is pretty technical, appropriate for someone already fairly familiar with the material in the CMS e-Lab. See this Scottish news report (with 7:24 minute video) for a more basic introduction to the Higgs.

Then tune in, if you can–from 8:00 to 10:00 AM Eastern Standard Time on Tuesday, December 13–to watch the action live. You can also follow the action on twitter: search the hashtag #Higgsupdate.

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Curious cosmic ray behavior?

Has anyone else noticed increased cosmic ray activity? I have seen drastic changes to flux counts the past two weeks.
Kevin

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DGCMSelab follow up classroom plan

Workshop Location:  UPR

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.): CMS

Grade(s)/Context:  9th grade, average ability students

Challenges:  low math ability

When/Where:  Introductory Physics/Parkway School District

Learning Objectives:  During unit on energy and momentum, learn about sub-atomic particles and evaluate energy of sub-atomic particles.

Standards:  Energy and conservation

Steps: 1. sub-atomic particle information appropriate for students can be obtained from current physical science text which also includes chemistry.

2.  Break students into research groups of 2 for different particles, they may develop a short (5 slide) power point for their particle.  They may use text, CMS website and particle adventure website.

3.  Supplemental materials on very simple nuclear equation balancing.  Will only use the beginning of Uranium 238 decay and particles produced.

4.  Presentation of these power points will be the introduction to extending the normal energy discussion to energy of a few of the particles presented by students. 

Follow-Up Date:  May 2012

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Fisica de particulas-Sahilis

Workshop Location: UPRM

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.):

Grade(s)/Context:12

Challenges:

When/Where: February 2012,  Loaiza Cordero del Rosario, Yauco

Learning Objectives: 1. Definir y describir las sub-particulas del atomo.  2.  Identificar los quarks (up, down), del cual esta compuesto los protones.

Standards: Estructura y niveles de organizacion de la materia

Steps:  1. Se le presentara al estudiante la estructura del atomo.  2.  A traves de una presentacion de power point se le presentara la estructura de los leptones y los quarks.  3.  Se le dara a el estudiante unos rompecabezas para que, al unirlos, formen los protones.  4.  Se le presentara un desconocido para que el estudiante pueda identificar o reconocer el componente del proton.

 

Follow-Up Date:februar

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Frances Implementation Plan

Workshop Location:UPRMPR

 Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.):   Integrate e-Lab in the Physics Class  Relate students with the 21st Century Particle PhysicsT

 Grade(s)/Context:  12

 Challenges:   Lack of internet access within my classroom so I would have to coordinate with the school librarian and move with my students to the Library.  We have a 50minutes class period.  Alingment of the current Puertorrican Science Standards  and Expectations with this project    Science Standards: Example:   Interactions (In the Chemistry class curriculum it provides only for interactions at electron level not at nuclear particles like protons-protons collisions)

When/Where:  At school. During this semester or the next

Learning Objectives:  Relate my students with the 21st Century Physics. 

Standards:  Interactions,  Energy,  Change and Conservation,  Structure and Organization of Matter, Science Nature and Technology

 Steps:  Talk to the students about the e-Lab Project, its goals, its importance Tell them that this will be a Physics Research Project in which they will be involved.  Visit UPRM for a workshop 

Follow-Up Date:

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Plan de implementation

Workshop Location:Uprm-prm 

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the cósmico Ray you can live section out.):Integrar E lab en la class de Quimica de escuela superior mediante una propuesta de investigation

Grade(s)/Context: 10,11,and 12

Challenges:llevar a Los estudiantes a la par con Los ultimos advances en el conocimiento del atomo y sus aplicaciones

When/Where:
En la escuela donde trabajo

Learning Objectives:

Standards:
Las interactions
Espectativa
Reconoce que la estructura de los atomos es Consecuencia de las interactions entre las particles subatomic as electron,protons and neutron.

Steps:

Follow-Up Date:

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Implementation Plan – Elba

Workshop Location: UPRM – PR

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.): Research Project using eLab

Grade(s)/Context: 10-12

Challenges:

1. To explain particle interactions and describe interactions.

2. To align the standard to the activities

3. To have computers with Internet Access

 

When%2

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Decaimientos Cosmicos

Workshop Location:

MAYAGUEZ

Goals of the Science Experiment (e.g., CMS, LIGO) (If you are working on the Cosmic Ray e-Lab, you can leave this section out.):

entender los decaimientos que se realizan y las particulas que debienen de losdecaimientos

Grade(s)/Context:

Graduate Students

Challenges:

When/Where:

Puerto Rico

Learning Objectives:

Standards:

Steps:

Follow-Up Date:

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