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flip . tanedo 24ucr . edu@ UCR PHYSICS 288
1
J O I N I N G T H E U C R PA R T I C L E T H E O R Y G R O U P
Flip Tanedo
1 March 2017 Physics 288
UC Riverside Particle Theory
HOW TO HEP-PH
theory.ucr.edu
UCR Physics Department
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
2Andrew Grant, Science News, June 2013
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
3
State of Particle Physics: 2017
“There is nothing new to be discovered in
physics now. All that remains is more and more
precise measurement”
— Kelvin (apocryphal)
1890s 1905
SR
1915
GR
1920s
quantum
relativistic quantum
non-Abelian gauge theory
renormalization
strings
holography
new particles neutrino mass
accelerating expansion
dark matter timeHiggs
Cosmic Microwave BG
conformal bootstrap
B-modes
gravitational waves
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Astro + Cosmo: Dark Matter Exists
5%
27%
68%
Standard Model is not complete
GALACTIC 

ROTATION CURVES
GRAVITATIONAL LENSING COSMIC MICROWAVE BACKGROUND
Images: Jeff Filippini (Berkeley Cosmology 2005), NASA APOD 2006, NASA WMAP
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
5
Prof. Flip Tanedo
INTERESTS:
What is dark matter?

How can we determine its properties?

… terrestrial, astro-particle, cosmological

What else is it good for?
What stabilizes the Higgs mass?

What is strong dynamics good for?
How do we test our hypotheses?
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
6
Particle Phenomenology
MYSTERY
examples:
Theory: what makes W scattering unitary? (Higgs boson)
Experiment: observed excess in 𝛾-rays … dark matter?
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
7
Particle Phenomenology
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Particle Phenomenology
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Particle Phenomenology
PREDICTION MYSTERY
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Where we earn our stripes
HACK
full theory
predictions
interpretation
consistency
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Weakly-Coupled Strong Dynamics
MY THEME:
Room for all sorts
of neat theories in
the dark sector.
… can use past
Higgs sector
creativity as a
launching point
My thesis title and Ph.D. defense flyer, 2013
FLIGHT OF THE WARPED PENGUINS
AND OTHER WEAKLY COUPLED TALES OF STRONG DYNAMICS
10:00AM PSB 301
TUESDAY MAY 21
Flip Tanedo
A DISSERTATION BY
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
12
Currently Thinking About (Part I)
Dark Matter Mediator
Standard ModelU(1)’
Standard
ModelHiggs
Dark Matter Mediator
Standard
Model
⌫R
Kinetic
Mixing
Dark
Matter
Ways to “subvert” ordinary portals to the dark sector
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
13
e.g. Majorino dark matter
Dark Matter
Mediator
Standard
Model
⌫R
supersymmetric
MAJORON
MAJORINO
order parameter for lepton number violation
SUSY
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Currently Thinking About (Part II)
Ways to “subvert” ordinary searches for the dark sector
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Example: Earth capture
Feng, Smolinsky, Tanedo (1509.07525 )
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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What is it like to be a theorist?
• The best qualities to have are: 

depth of understanding & creativity
• You will spend your time:

— Learning and re-learning known physics

— Deriving implications of new ideas

— Interpreting experimental results

— Collaborating with others to generate new ideas

— Communicating these ideas (talks, papers)
• Need to be tenaciously curious
• Humility towards subject, moxie in your ambitions
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
17
Preparation
• quantum field theory
• 2013 BSM lectures arXiv:1602.04228
• useful technical skills
• LaTeX, Python, Mathematica; C++, Root, …
• (Lie) group theory; differential geometry
• useful coursework (we expect top marks)
• E&M, Quantum Mechanics, Statistical Physics
• Statistical Field Theory / all the QFT you can take
• General relativity, cosmology
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
18
Hai-Bo’s Catechism
THE KEY TO SUCCESS IN OUR FIELD:

10 hours per day

6 days a week
… REPEAT FOR 10 YEARS
from Hai-Bo Yu
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
19
What it’s like to work with me
• Start as tightly coupled system: frequent check
ins, first projects will be micro-managed
• Training includes writing/reading papers, how to
give talks, collaborating with peers, …
• Goals: develop good habits, become
independent, well positioned for next job
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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Goals for my students
you
• Work with multiple faculty
• Publications & letters of 

recommendation
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
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world
expert
on this
space of ideas
Light Mediators
dark matter
capture
Supersymmetry
you
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
22
space of ideas
Dark
Matter
Theory of Strong Dynamics
Cosmology
Other funny ideas …
Collider Physics
new
searches
still you, but closer to scale
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
23
Road Map
Excel in courses, be curious about particle physics

Ace the qualifying exam, small summer project
Meet 3x per week, micromanaged

Rapid expertise in a small topic

Drinking from the firehose learning
Projects with faculty, expand bubble of expertise

Give journal club talks, work with other students

Summer schools, conference talks
Projects with faculty outside UCR

Initiate your own projects, invited seminars

Launch towards a top postdoc position
flip . tanedo 24ucr . edu@ UCR PHYSICS 288
24
Your next steps
• Talk to us & to senior graduate students
• Do exceptionally well in relevant
coursework: E&M, QM, field theory
• Pass Ace the qualifying exams
• Do your “homework,” attend seminars
theory.ucr.edu

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How to HEP-PH

  • 1. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 1 J O I N I N G T H E U C R PA R T I C L E T H E O R Y G R O U P Flip Tanedo 1 March 2017 Physics 288 UC Riverside Particle Theory HOW TO HEP-PH theory.ucr.edu UCR Physics Department
  • 2. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 2Andrew Grant, Science News, June 2013
  • 3. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 3 State of Particle Physics: 2017 “There is nothing new to be discovered in physics now. All that remains is more and more precise measurement” — Kelvin (apocryphal) 1890s 1905 SR 1915 GR 1920s quantum relativistic quantum non-Abelian gauge theory renormalization strings holography new particles neutrino mass accelerating expansion dark matter timeHiggs Cosmic Microwave BG conformal bootstrap B-modes gravitational waves
  • 4. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 4 Astro + Cosmo: Dark Matter Exists 5% 27% 68% Standard Model is not complete GALACTIC 
 ROTATION CURVES GRAVITATIONAL LENSING COSMIC MICROWAVE BACKGROUND Images: Jeff Filippini (Berkeley Cosmology 2005), NASA APOD 2006, NASA WMAP
  • 5. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 5 Prof. Flip Tanedo INTERESTS: What is dark matter?
 How can we determine its properties?
 … terrestrial, astro-particle, cosmological
 What else is it good for? What stabilizes the Higgs mass?
 What is strong dynamics good for? How do we test our hypotheses?
  • 6. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 6 Particle Phenomenology MYSTERY examples: Theory: what makes W scattering unitary? (Higgs boson) Experiment: observed excess in 𝛾-rays … dark matter?
  • 7. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 7 Particle Phenomenology
  • 8. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 8 Particle Phenomenology
  • 9. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 9 Particle Phenomenology PREDICTION MYSTERY
  • 10. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 10 Where we earn our stripes HACK full theory predictions interpretation consistency
  • 11. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 11 Weakly-Coupled Strong Dynamics MY THEME: Room for all sorts of neat theories in the dark sector. … can use past Higgs sector creativity as a launching point My thesis title and Ph.D. defense flyer, 2013 FLIGHT OF THE WARPED PENGUINS AND OTHER WEAKLY COUPLED TALES OF STRONG DYNAMICS 10:00AM PSB 301 TUESDAY MAY 21 Flip Tanedo A DISSERTATION BY
  • 12. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 12 Currently Thinking About (Part I) Dark Matter Mediator Standard ModelU(1)’ Standard ModelHiggs Dark Matter Mediator Standard Model ⌫R Kinetic Mixing Dark Matter Ways to “subvert” ordinary portals to the dark sector
  • 13. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 13 e.g. Majorino dark matter Dark Matter Mediator Standard Model ⌫R supersymmetric MAJORON MAJORINO order parameter for lepton number violation SUSY
  • 14. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 14 Currently Thinking About (Part II) Ways to “subvert” ordinary searches for the dark sector
  • 15. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 15 Example: Earth capture Feng, Smolinsky, Tanedo (1509.07525 )
  • 16. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 16 What is it like to be a theorist? • The best qualities to have are: 
 depth of understanding & creativity • You will spend your time:
 — Learning and re-learning known physics
 — Deriving implications of new ideas
 — Interpreting experimental results
 — Collaborating with others to generate new ideas
 — Communicating these ideas (talks, papers) • Need to be tenaciously curious • Humility towards subject, moxie in your ambitions
  • 17. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 17 Preparation • quantum field theory • 2013 BSM lectures arXiv:1602.04228 • useful technical skills • LaTeX, Python, Mathematica; C++, Root, … • (Lie) group theory; differential geometry • useful coursework (we expect top marks) • E&M, Quantum Mechanics, Statistical Physics • Statistical Field Theory / all the QFT you can take • General relativity, cosmology
  • 18. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 18 Hai-Bo’s Catechism THE KEY TO SUCCESS IN OUR FIELD:
 10 hours per day
 6 days a week … REPEAT FOR 10 YEARS from Hai-Bo Yu
  • 19. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 19 What it’s like to work with me • Start as tightly coupled system: frequent check ins, first projects will be micro-managed • Training includes writing/reading papers, how to give talks, collaborating with peers, … • Goals: develop good habits, become independent, well positioned for next job
  • 20. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 20 Goals for my students you • Work with multiple faculty • Publications & letters of 
 recommendation
  • 21. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 21 world expert on this space of ideas Light Mediators dark matter capture Supersymmetry you
  • 22. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 22 space of ideas Dark Matter Theory of Strong Dynamics Cosmology Other funny ideas … Collider Physics new searches still you, but closer to scale
  • 23. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 23 Road Map Excel in courses, be curious about particle physics
 Ace the qualifying exam, small summer project Meet 3x per week, micromanaged
 Rapid expertise in a small topic
 Drinking from the firehose learning Projects with faculty, expand bubble of expertise
 Give journal club talks, work with other students
 Summer schools, conference talks Projects with faculty outside UCR
 Initiate your own projects, invited seminars
 Launch towards a top postdoc position
  • 24. flip . tanedo 24ucr . edu@ UCR PHYSICS 288 24 Your next steps • Talk to us & to senior graduate students • Do exceptionally well in relevant coursework: E&M, QM, field theory • Pass Ace the qualifying exams • Do your “homework,” attend seminars theory.ucr.edu