This document contains the notes from a talk given by Dr. Flip Tanedo to physics majors. The talk discusses things Dr. Tanedo wishes he knew when he was a beginning physics major, including doing homework, doing research, having a team, and understanding that failure is an important part of learning and growth.
Attending to Diversity in the Physics ClassroomFlip Tanedo
The document discusses a February workshop at UC Riverside aimed at promoting inclusion in physics. It addresses challenges like underrepresentation of certain groups in physics and barriers that can cause students to leave STEM fields. It provides working definitions for terms like minority, self-efficacy, privilege, and impostor syndrome. The workshop sought input from teachers on helping students succeed and discussed frameworks for continuing conversations between high school and college educators to support diversity.
Talk for the 26th Fr. Ciriaco Pedrosa, O.P. Memorial Lecture Series and 8th International Symposium on Mathematics and Physics at the University of Santo Tomas (Manila, Philippines). Presented remotely on Nov 26, 2021
Prof. Flip Tanedo gives a presentation on his work researching dark matter. He studies theoretical particle physics and tries to answer mysteries like what dark matter is made of. Dark matter is invisible but accounts for 80% of the universe's matter. Tanedo also provides life advice for physics students, encouraging them to be curious, do research, and engage in science as a creative endeavor by coming up with new ideas and rigorously testing them.
This document summarizes Prof. Flip Tanedo's presentation to the UCR CAMP General Meeting. It introduces Prof. Tanedo and their background, including graduating from high school in Los Angeles and being the first in their family to attend a four-year college. It then discusses Prof. Tanedo's work in theoretical particle physics, focusing on dark matter research. The presentation provides advice to students, including developing resilience when facing challenges and embracing failure as an opportunity to grow.
The document discusses a model of spin-1 vector dark matter interacting with a light vector mediator particle. It begins by reviewing previous related work on other models of dark matter with vector or spin-1 properties. It then outlines plans to build a new model with a massive spin-1 mediator between the standard model and vector dark matter, and hints at possible new phenomena that could arise from this setup. Figures and equations are included to illustrate concepts like the symmetry structure and interactions between the sectors.
The document discusses dark matter and the search for dark matter particles through theoretical physics. It begins with a cartoon depiction of dark matter and explains that dark matter exists based on evidence from astronomy and cosmology, such as galaxy rotation curves and gravitational lensing. It then presents the search for dark matter as a puzzle for fundamental physicists to determine which particles in their theories could account for dark matter. Several hypothetical dark matter candidates are discussed, as well as ways indirect evidence about dark matter properties could be learned. The talk concludes by drawing an analogy between the theoretical discovery and detection of Neptune and the ongoing search for direct evidence of dark matter particles.
This document contains the notes from a talk given by Dr. Flip Tanedo to physics majors. The talk discusses things Dr. Tanedo wishes he knew when he was a beginning physics major, including doing homework, doing research, having a team, and understanding that failure is an important part of learning and growth.
Attending to Diversity in the Physics ClassroomFlip Tanedo
The document discusses a February workshop at UC Riverside aimed at promoting inclusion in physics. It addresses challenges like underrepresentation of certain groups in physics and barriers that can cause students to leave STEM fields. It provides working definitions for terms like minority, self-efficacy, privilege, and impostor syndrome. The workshop sought input from teachers on helping students succeed and discussed frameworks for continuing conversations between high school and college educators to support diversity.
Talk for the 26th Fr. Ciriaco Pedrosa, O.P. Memorial Lecture Series and 8th International Symposium on Mathematics and Physics at the University of Santo Tomas (Manila, Philippines). Presented remotely on Nov 26, 2021
Prof. Flip Tanedo gives a presentation on his work researching dark matter. He studies theoretical particle physics and tries to answer mysteries like what dark matter is made of. Dark matter is invisible but accounts for 80% of the universe's matter. Tanedo also provides life advice for physics students, encouraging them to be curious, do research, and engage in science as a creative endeavor by coming up with new ideas and rigorously testing them.
This document summarizes Prof. Flip Tanedo's presentation to the UCR CAMP General Meeting. It introduces Prof. Tanedo and their background, including graduating from high school in Los Angeles and being the first in their family to attend a four-year college. It then discusses Prof. Tanedo's work in theoretical particle physics, focusing on dark matter research. The presentation provides advice to students, including developing resilience when facing challenges and embracing failure as an opportunity to grow.
The document discusses a model of spin-1 vector dark matter interacting with a light vector mediator particle. It begins by reviewing previous related work on other models of dark matter with vector or spin-1 properties. It then outlines plans to build a new model with a massive spin-1 mediator between the standard model and vector dark matter, and hints at possible new phenomena that could arise from this setup. Figures and equations are included to illustrate concepts like the symmetry structure and interactions between the sectors.
The document discusses dark matter and the search for dark matter particles through theoretical physics. It begins with a cartoon depiction of dark matter and explains that dark matter exists based on evidence from astronomy and cosmology, such as galaxy rotation curves and gravitational lensing. It then presents the search for dark matter as a puzzle for fundamental physicists to determine which particles in their theories could account for dark matter. Several hypothetical dark matter candidates are discussed, as well as ways indirect evidence about dark matter properties could be learned. The talk concludes by drawing an analogy between the theoretical discovery and detection of Neptune and the ongoing search for direct evidence of dark matter particles.
Slides for my "lightning talk" at Science Hack Day: San Francisco (2015) on open data sets in particle physics. Small discussion of why some data sets are closed (e.g. LHC) while others are open (e.g. Fermi). Includes some suggested open science projects for the engaged public.
Attending to Diversity in the Classroom: AnnotatedFlip Tanedo
Talk to high school physics teachers to initiate a discussion about inclusion and diversity in the classroom. Part of the UCR Summer Physics Teacher Academy program. Annotated version. (Slides with green bars represent content that was discussed verbally but did not appear on the slides explicitly.) Some teacher responses included at the end.
This document provides advice on how to fail as a physics major and a bit about how to succeed. It begins by introducing the author and their background, including failures they have experienced. The document then outlines five main ways to fail: 1) Letting your goals be defined by others' expectations rather than your own, 2) Assuming you already know the rules without learning them, 3) Viewing success as a zero-sum game rather than cooperative, 4) Being antagonistic rather than cooperative, and 5) Avoiding failure at all costs rather than embracing a growth mindset. The document provides examples and counterarguments for avoiding each of these failures and instead focusing on intrinsic goals, cooperation, learning continuously, and embracing challenges.
This document summarizes a presentation given at BNL on using neutron stars to study dark matter interactions. Dark matter passing through the Milky Way halo can scatter off neutrons in neutron stars, transferring some of its kinetic energy and heating the stars up. This would cause the neutron stars to emit infrared radiation that could be detected by future telescopes. The level of heating depends on the dark matter-nucleon scattering cross section, providing a way to probe certain cross sections that are inaccessible to direct detection experiments. Observing infrared emission from cold neutron stars could help reveal properties of dark matter such as its mass and interaction type.
This document appears to be a set of slides from a presentation given by Flip Tanedo on how to succeed and avoid failure in an academic career. Some key points mentioned include the importance of gaining research experience as early as possible, preferably through summer programs; asking for letters of recommendation well in advance of deadlines; and seeking help and guidance from advisors, mentors, and peers rather than trying to do everything alone. The presentation also warns students that graduate school will be challenging and involves overcoming difficulties like imposter syndrome.
electron positron production of dark sector particlesFlip Tanedo
This document discusses potential studies of dark sector particles that could be performed at a future linear collider, such as the International Linear Collider. It begins by noting some advantages of a linear collider compared to the LHC for such searches, including cleaner events and control of beam polarization. It then discusses various portals through which dark sectors could couple to visible matter and characteristics of interest to measure. Examples of specific studies proposed include searches for light mediators, long-lived low-mass particles, distinguishing spin and mass scales of dark particles, and probing axion-like particles and displaced lepton jets from dark sector bound states.
Diving Into The Dark: What The Universe Is Made OfFlip Tanedo
The document is a presentation given by Flip Tanedo to affiliates of UC Riverside on diving into the dark universe and what the universe is made of. It summarizes that dark matter exists based on evidence from astronomy but its true nature remains a puzzle that theorists are trying to solve using particle physics. It discusses how theoretical science works to make predictions about unseen phenomena and gives examples from the history of astronomy.
Whatever Happened to the WIMP of Tomorrow?Flip Tanedo
The document discusses a physics colloquium presentation about dark matter. It begins with an outline comparing the talk to fictional stories of Superman. The talk then reviews evidence that dark matter exists from astronomical observations. Next, it discusses the status of the weakly interacting massive particle (WIMP) as a leading dark matter candidate. The talk provides historical context for the WIMP hypothesis from the 1990s and outlines several open questions in particle physics that a WIMP could potentially address, such as the hierarchy problem. It describes how supersymmetry is a favored theoretical framework that could explain a WIMP through the introduction of superpartner particles.
The document discusses the current understanding of what the universe is made of according to the Standard Model of particle physics. It explains that all matter is made up of fundamental particles like quarks and electrons, which in turn are made up of even smaller particles. The document then introduces string theory as a promising candidate for a unified theory that could provide a quantum description of gravity and a "Theory of Everything". String theory proposes that all fundamental particles are actually different vibrational states of tiny loops of string. While string theory derives the Standard Model, there is currently no direct experimental evidence to confirm it is the correct description of nature.
This document provides information about joining the UCR Particle Theory Group led by Prof. Flip Tanedo. It discusses Tanedo's research interests in topics like dark matter, the Higgs boson, and strongly coupled dynamics. The document outlines the preparation and skills needed to succeed in theoretical particle physics, including mastery of quantum field theory, programming, and group theory. It also maps out a roadmap for graduate students to develop expertise through projects, seminars, and conferences on their way to a successful career.
Whatever happened to the WIMP of tomorrow?Flip Tanedo
The document discusses a physics colloquium presentation about dark matter. It begins with an outline comparing the talk to fictional stories of Superman. The talk then reviews evidence that dark matter exists from astronomical observations. Next, it discusses the status of the weakly interacting massive particle (WIMP) as a leading dark matter candidate. The talk provides historical context for the WIMP hypothesis from the 1990s and outlines several open questions in particle physics that a WIMP could potentially address, such as the hierarchy problem. It describes how supersymmetry is a favored theoretical framework that could explain a WIMP through the introduction of superpartner particles.
The overwhelming observational evidence for the existence of dark matter is only matched by the awkward scarcity of information about what it might actually be. Laboratory searches for dark matter now appear to exclude many of the "weakly interacting massive particle" models that were favored by particle physicists for decades. Where does that leave the hunt for dark matter? If we've left the WIMP behind, what are we looking for? We give a brief, biased, and largely fictional history of the WIMP in order to establish what has and has not been excluded, and why it matters.
This general-interest presentation grew out of discussions with astronomers who wanted to understand why some of their particle physics colleagues are "searching for WIMPs" while the others
have decided to live in a "post-WIMP world."
Space lattice theory a grand unification of physicsslpr2013
Space Lattice Theory presents a radically new theory of the universe that describes how matter, energy, force at a distance, space and time can be explained by one single principle - a Grand Unification. Many cosmic puzzles are finally explained.
This document is a summary of a physics colloquium given by Flip Tanedo at UC Riverside on October 22, 2018 about dark matter theory. The colloquium discussed the history of the weakly interacting massive particle (WIMP) as a leading dark matter candidate, treating it as a piece of historical fiction. It described how the WIMP arose from attempts to solve problems in particle physics in the 1990s, such as the hierarchy problem, and came to predict the correct abundance of dark matter through the "WIMP miracle." However, as WIMPs have yet to be directly detected, the talk suggests it is now more productive to explore non-WIMP dark matter models.
Physicists believe that our universe has more than 4 dimensions--3 s.pdfajithmobiles
Physicists believe that our universe has more than 4 dimensions--3 spatial ones plus a time
dimension--with some theories suggesting 10 dimensions and others 11. The \"extra\"
dimensions are thought to be somehow inside the big ones we can perceive directly. Does the
idea of fractal geometry suggest to you any ways in which this theory might make sense?
Explain your answer
Solution
Quantum Theory just seems too weird to believe. Particles can be in more than one place at a
time.
And they don\'t exist until you measure them. Spookier still, they en stay in touch when they are
separated by great distances.
Einstein thought this was all a bit much, believing it to be evidence of major problems with the
Theory as many critics still suspect today. Quantum enthusiasts point to the theory\'s
extraordinary
success in explaining the behavior of atoms, electrons, and other quantum systems. They insist
we have
to accept the Theory as it is, however strange it may seem.
But what if there were a way to reconcile these 2 opposing views by showing how Quantum
Theory
might emerge from a deeper level of non-weird Physics?
If you listen to physicist Tim Palmer, it begins to sound plausible. What has been missing, he
argues, are some key ideas from an area of science that most quantum physicists have ignored.
Namely
the science of Fractals -- those intricate patterns found in everything from fractured surfaces to
oceanic
flows (see \"What is a Fractal?\").
Take the mathematics of Fractals into account, says Palmer, and the long-standing puzzles of
Quantum Theory may be much easier to understand. They might even dissolve away.
It is an argument that is drawing attention from physicists around the World. \"His approach is
very
interesting and refreshingly different,\" says physicist Robert Spekkens of the Perimeter Institute
for
Theoretical Physics in Waterloo, Canada. \"He\'s not just trying to reinterpret the usual quantum
formalism but actually to derive it from something deeper.\"
That Palmer is making this argument may seem a little odd, given that he is a climate scientist
working at the European Centre for Medium-Range Weather Forecasting in Reading, UK. It
makes
more sense when you learn that Palmer studied General Relativity at the University of Oxford,
working
under the same PhD adviser as Stephen Hawking.
So while Palmer has spent the last 20 years establishing a reputation as a leading mathematical
climatologist, he has also continued to explore the mysteries of his first interest -- Quantum
Theory (see
\"Quantum Ambitions\").
1\"It has taken 20 years of thinking,\" says Palmer. \"But I do think that most of the paradoxes of
Quantum Theory may well have a simple and comprehensible resolution.\"
Arguments over Quantum Theory have raged since the 1920s starting with a series of famous
exchanges between Einstein and the Danish physicist Niels Bohr.
Bohr and his supporters believed that the Theory\'s successful description of atoms and radiation
meant tha.
This document provides an overview of the topics to be covered in a Physics 357/457 course on elementary particle physics. The course will examine the elementary particles like quarks and leptons, the forces that govern their interactions, and theoretical models used to understand particle physics, including the Standard Model. It outlines the course structure, evaluation methods, and provides a list of reference materials for further reading on topics covered during the semester.
FROM UNDERSTANDING BASIC PARTICLE PHYSICS —to exploring the Universe During the first half of 2013, a number of startling advances in astro-particle physics have been announced. In addition to this--the next ultra large cosmic ray experiment is being developed, regions of the world (including southwest Kansas) tested for their suitability to host such an experiment. In this talk you will get a brief introduction of the ideas of particle physics and how they are being transformed into astro-particle measurements to further understand the Universe and the forces within it.
This document provides an overview of dark matter and dark energy from both observational evidence in the universe and theoretical work done at particle accelerators in laboratories. It summarizes that observational evidence shows the universe is made up of 70% dark energy, 25% dark matter, and only 5% ordinary matter. While much is known about the basic features and inventory of the universe, deep puzzles remain about reconciling gravity and quantum mechanics, the nature of dark matter and dark energy, and resolving why observations of dark energy are so much smaller than theoretical predictions. The document discusses how ideas like extra dimensions, supersymmetry, and multiple compactifications in string theory attempt to address these puzzles, but that challenges remain in fully explaining dark energy and connecting theory to
A preponderance of scientific evidence over the last hundred years tells us that our galaxy is filled with an unknown substance called dark matter. In fact, there is five times as much dark matter in the universe than there is ordinary matter: we are swimming in an ocean of dark matter and we have no firm idea what it is. We suspect that dark matter is composed of undiscovered elementary particles whose properties may, in turn, unlock some of the most pressing open questions in fundamental physics. So why haven't we figured out how to study dark matter in the lab, and why should we be optimistic that we may make progress in the coming decades?
How Not to Discover the WIMP (Sam Houston State University)Flip Tanedo
The document discusses theories of dark matter from the 1990s, when supersymmetry was a favored explanation. Supersymmetry posited that each standard model particle has a supersymmetric partner to address problems like the Higgs mass and proton decay. Imposing R-parity conservation made the lightest supersymmetric particle stable and a dark matter candidate. This "neutralino" would be a weakly interacting massive particle with weak-scale mass and couplings that could naturally produce the observed dark matter abundance through thermal freeze-out in the early universe, in what became known as the "WIMP miracle". While promising, direct searches for WIMPs have so far found nothing, and new ideas for dark matter are now being explored.
1) Stephen Hawking summarized his 1980 lecture where he discussed the progress made in theoretical physics over the previous century and questioned if a complete unified theory could be found by the end of the 20th century.
2) In the 1960s, four fundamental forces were known - gravity, electromagnetism, and the strong and weak nuclear forces. Developments in the 1960s and 1970s unified electromagnetism and the weak force, though gravity remained separate.
3) Hawking proposes that like maps of the Earth's curved surface, there may be multiple overlapping theories needed to describe physics in all situations, rather than one single unified theory, though progress continues to be made theoretically through proposals
Slides for my "lightning talk" at Science Hack Day: San Francisco (2015) on open data sets in particle physics. Small discussion of why some data sets are closed (e.g. LHC) while others are open (e.g. Fermi). Includes some suggested open science projects for the engaged public.
Attending to Diversity in the Classroom: AnnotatedFlip Tanedo
Talk to high school physics teachers to initiate a discussion about inclusion and diversity in the classroom. Part of the UCR Summer Physics Teacher Academy program. Annotated version. (Slides with green bars represent content that was discussed verbally but did not appear on the slides explicitly.) Some teacher responses included at the end.
This document provides advice on how to fail as a physics major and a bit about how to succeed. It begins by introducing the author and their background, including failures they have experienced. The document then outlines five main ways to fail: 1) Letting your goals be defined by others' expectations rather than your own, 2) Assuming you already know the rules without learning them, 3) Viewing success as a zero-sum game rather than cooperative, 4) Being antagonistic rather than cooperative, and 5) Avoiding failure at all costs rather than embracing a growth mindset. The document provides examples and counterarguments for avoiding each of these failures and instead focusing on intrinsic goals, cooperation, learning continuously, and embracing challenges.
This document summarizes a presentation given at BNL on using neutron stars to study dark matter interactions. Dark matter passing through the Milky Way halo can scatter off neutrons in neutron stars, transferring some of its kinetic energy and heating the stars up. This would cause the neutron stars to emit infrared radiation that could be detected by future telescopes. The level of heating depends on the dark matter-nucleon scattering cross section, providing a way to probe certain cross sections that are inaccessible to direct detection experiments. Observing infrared emission from cold neutron stars could help reveal properties of dark matter such as its mass and interaction type.
This document appears to be a set of slides from a presentation given by Flip Tanedo on how to succeed and avoid failure in an academic career. Some key points mentioned include the importance of gaining research experience as early as possible, preferably through summer programs; asking for letters of recommendation well in advance of deadlines; and seeking help and guidance from advisors, mentors, and peers rather than trying to do everything alone. The presentation also warns students that graduate school will be challenging and involves overcoming difficulties like imposter syndrome.
electron positron production of dark sector particlesFlip Tanedo
This document discusses potential studies of dark sector particles that could be performed at a future linear collider, such as the International Linear Collider. It begins by noting some advantages of a linear collider compared to the LHC for such searches, including cleaner events and control of beam polarization. It then discusses various portals through which dark sectors could couple to visible matter and characteristics of interest to measure. Examples of specific studies proposed include searches for light mediators, long-lived low-mass particles, distinguishing spin and mass scales of dark particles, and probing axion-like particles and displaced lepton jets from dark sector bound states.
Diving Into The Dark: What The Universe Is Made OfFlip Tanedo
The document is a presentation given by Flip Tanedo to affiliates of UC Riverside on diving into the dark universe and what the universe is made of. It summarizes that dark matter exists based on evidence from astronomy but its true nature remains a puzzle that theorists are trying to solve using particle physics. It discusses how theoretical science works to make predictions about unseen phenomena and gives examples from the history of astronomy.
Whatever Happened to the WIMP of Tomorrow?Flip Tanedo
The document discusses a physics colloquium presentation about dark matter. It begins with an outline comparing the talk to fictional stories of Superman. The talk then reviews evidence that dark matter exists from astronomical observations. Next, it discusses the status of the weakly interacting massive particle (WIMP) as a leading dark matter candidate. The talk provides historical context for the WIMP hypothesis from the 1990s and outlines several open questions in particle physics that a WIMP could potentially address, such as the hierarchy problem. It describes how supersymmetry is a favored theoretical framework that could explain a WIMP through the introduction of superpartner particles.
The document discusses the current understanding of what the universe is made of according to the Standard Model of particle physics. It explains that all matter is made up of fundamental particles like quarks and electrons, which in turn are made up of even smaller particles. The document then introduces string theory as a promising candidate for a unified theory that could provide a quantum description of gravity and a "Theory of Everything". String theory proposes that all fundamental particles are actually different vibrational states of tiny loops of string. While string theory derives the Standard Model, there is currently no direct experimental evidence to confirm it is the correct description of nature.
This document provides information about joining the UCR Particle Theory Group led by Prof. Flip Tanedo. It discusses Tanedo's research interests in topics like dark matter, the Higgs boson, and strongly coupled dynamics. The document outlines the preparation and skills needed to succeed in theoretical particle physics, including mastery of quantum field theory, programming, and group theory. It also maps out a roadmap for graduate students to develop expertise through projects, seminars, and conferences on their way to a successful career.
Whatever happened to the WIMP of tomorrow?Flip Tanedo
The document discusses a physics colloquium presentation about dark matter. It begins with an outline comparing the talk to fictional stories of Superman. The talk then reviews evidence that dark matter exists from astronomical observations. Next, it discusses the status of the weakly interacting massive particle (WIMP) as a leading dark matter candidate. The talk provides historical context for the WIMP hypothesis from the 1990s and outlines several open questions in particle physics that a WIMP could potentially address, such as the hierarchy problem. It describes how supersymmetry is a favored theoretical framework that could explain a WIMP through the introduction of superpartner particles.
The overwhelming observational evidence for the existence of dark matter is only matched by the awkward scarcity of information about what it might actually be. Laboratory searches for dark matter now appear to exclude many of the "weakly interacting massive particle" models that were favored by particle physicists for decades. Where does that leave the hunt for dark matter? If we've left the WIMP behind, what are we looking for? We give a brief, biased, and largely fictional history of the WIMP in order to establish what has and has not been excluded, and why it matters.
This general-interest presentation grew out of discussions with astronomers who wanted to understand why some of their particle physics colleagues are "searching for WIMPs" while the others
have decided to live in a "post-WIMP world."
Space lattice theory a grand unification of physicsslpr2013
Space Lattice Theory presents a radically new theory of the universe that describes how matter, energy, force at a distance, space and time can be explained by one single principle - a Grand Unification. Many cosmic puzzles are finally explained.
This document is a summary of a physics colloquium given by Flip Tanedo at UC Riverside on October 22, 2018 about dark matter theory. The colloquium discussed the history of the weakly interacting massive particle (WIMP) as a leading dark matter candidate, treating it as a piece of historical fiction. It described how the WIMP arose from attempts to solve problems in particle physics in the 1990s, such as the hierarchy problem, and came to predict the correct abundance of dark matter through the "WIMP miracle." However, as WIMPs have yet to be directly detected, the talk suggests it is now more productive to explore non-WIMP dark matter models.
Physicists believe that our universe has more than 4 dimensions--3 s.pdfajithmobiles
Physicists believe that our universe has more than 4 dimensions--3 spatial ones plus a time
dimension--with some theories suggesting 10 dimensions and others 11. The \"extra\"
dimensions are thought to be somehow inside the big ones we can perceive directly. Does the
idea of fractal geometry suggest to you any ways in which this theory might make sense?
Explain your answer
Solution
Quantum Theory just seems too weird to believe. Particles can be in more than one place at a
time.
And they don\'t exist until you measure them. Spookier still, they en stay in touch when they are
separated by great distances.
Einstein thought this was all a bit much, believing it to be evidence of major problems with the
Theory as many critics still suspect today. Quantum enthusiasts point to the theory\'s
extraordinary
success in explaining the behavior of atoms, electrons, and other quantum systems. They insist
we have
to accept the Theory as it is, however strange it may seem.
But what if there were a way to reconcile these 2 opposing views by showing how Quantum
Theory
might emerge from a deeper level of non-weird Physics?
If you listen to physicist Tim Palmer, it begins to sound plausible. What has been missing, he
argues, are some key ideas from an area of science that most quantum physicists have ignored.
Namely
the science of Fractals -- those intricate patterns found in everything from fractured surfaces to
oceanic
flows (see \"What is a Fractal?\").
Take the mathematics of Fractals into account, says Palmer, and the long-standing puzzles of
Quantum Theory may be much easier to understand. They might even dissolve away.
It is an argument that is drawing attention from physicists around the World. \"His approach is
very
interesting and refreshingly different,\" says physicist Robert Spekkens of the Perimeter Institute
for
Theoretical Physics in Waterloo, Canada. \"He\'s not just trying to reinterpret the usual quantum
formalism but actually to derive it from something deeper.\"
That Palmer is making this argument may seem a little odd, given that he is a climate scientist
working at the European Centre for Medium-Range Weather Forecasting in Reading, UK. It
makes
more sense when you learn that Palmer studied General Relativity at the University of Oxford,
working
under the same PhD adviser as Stephen Hawking.
So while Palmer has spent the last 20 years establishing a reputation as a leading mathematical
climatologist, he has also continued to explore the mysteries of his first interest -- Quantum
Theory (see
\"Quantum Ambitions\").
1\"It has taken 20 years of thinking,\" says Palmer. \"But I do think that most of the paradoxes of
Quantum Theory may well have a simple and comprehensible resolution.\"
Arguments over Quantum Theory have raged since the 1920s starting with a series of famous
exchanges between Einstein and the Danish physicist Niels Bohr.
Bohr and his supporters believed that the Theory\'s successful description of atoms and radiation
meant tha.
This document provides an overview of the topics to be covered in a Physics 357/457 course on elementary particle physics. The course will examine the elementary particles like quarks and leptons, the forces that govern their interactions, and theoretical models used to understand particle physics, including the Standard Model. It outlines the course structure, evaluation methods, and provides a list of reference materials for further reading on topics covered during the semester.
FROM UNDERSTANDING BASIC PARTICLE PHYSICS —to exploring the Universe During the first half of 2013, a number of startling advances in astro-particle physics have been announced. In addition to this--the next ultra large cosmic ray experiment is being developed, regions of the world (including southwest Kansas) tested for their suitability to host such an experiment. In this talk you will get a brief introduction of the ideas of particle physics and how they are being transformed into astro-particle measurements to further understand the Universe and the forces within it.
This document provides an overview of dark matter and dark energy from both observational evidence in the universe and theoretical work done at particle accelerators in laboratories. It summarizes that observational evidence shows the universe is made up of 70% dark energy, 25% dark matter, and only 5% ordinary matter. While much is known about the basic features and inventory of the universe, deep puzzles remain about reconciling gravity and quantum mechanics, the nature of dark matter and dark energy, and resolving why observations of dark energy are so much smaller than theoretical predictions. The document discusses how ideas like extra dimensions, supersymmetry, and multiple compactifications in string theory attempt to address these puzzles, but that challenges remain in fully explaining dark energy and connecting theory to
A preponderance of scientific evidence over the last hundred years tells us that our galaxy is filled with an unknown substance called dark matter. In fact, there is five times as much dark matter in the universe than there is ordinary matter: we are swimming in an ocean of dark matter and we have no firm idea what it is. We suspect that dark matter is composed of undiscovered elementary particles whose properties may, in turn, unlock some of the most pressing open questions in fundamental physics. So why haven't we figured out how to study dark matter in the lab, and why should we be optimistic that we may make progress in the coming decades?
How Not to Discover the WIMP (Sam Houston State University)Flip Tanedo
The document discusses theories of dark matter from the 1990s, when supersymmetry was a favored explanation. Supersymmetry posited that each standard model particle has a supersymmetric partner to address problems like the Higgs mass and proton decay. Imposing R-parity conservation made the lightest supersymmetric particle stable and a dark matter candidate. This "neutralino" would be a weakly interacting massive particle with weak-scale mass and couplings that could naturally produce the observed dark matter abundance through thermal freeze-out in the early universe, in what became known as the "WIMP miracle". While promising, direct searches for WIMPs have so far found nothing, and new ideas for dark matter are now being explored.
1) Stephen Hawking summarized his 1980 lecture where he discussed the progress made in theoretical physics over the previous century and questioned if a complete unified theory could be found by the end of the 20th century.
2) In the 1960s, four fundamental forces were known - gravity, electromagnetism, and the strong and weak nuclear forces. Developments in the 1960s and 1970s unified electromagnetism and the weak force, though gravity remained separate.
3) Hawking proposes that like maps of the Earth's curved surface, there may be multiple overlapping theories needed to describe physics in all situations, rather than one single unified theory, though progress continues to be made theoretically through proposals
1) The document discusses CERN, the particle physics laboratory located near Geneva, Switzerland. It describes some of the research being done there, including experiments using the Large Hadron Collider to better understand the universe.
2) The Large Hadron Collider fires beams of protons towards each other at close to the speed of light to simulate the high energy conditions that existed shortly after the Big Bang. Experiments detect the subatomic particles created in these collisions to learn about fundamental forces and particles.
3) One goal is to find the Higgs boson particle, which could help explain how other particles acquire mass. Researchers also hope to gain insights into dark matter, black holes, and theories of everything. The scale of the
The document discusses the scientific method and how it has evolved over time. It begins by defining science as the empirical study of nature. It then discusses three main methodologies in science: reductionism, which explains phenomena in terms of underlying mechanisms; structuralism, which studies complex phenomena as original systems; and "universalism", which makes statistical predictions about classes of similar systems. The document traces how these methodologies have developed from classical physics to modern fields like quantum mechanics and biology. It also explores how mythologies can provide metaphorical insights that inspire scientific hypotheses.
This document provides 10 examples of science fact or fiction questions related to space and sci-fi topics. It summarizes the evidence for whether each statement is factual or fictional. Key findings include that multiple planetary systems have been discovered, some microorganisms can survive in space without protection, and organisms have been found thriving in extremely hot water. However, there is no conclusive evidence of life beyond Earth and we do not currently have the technology for interstellar travel or teleporting people.
Discovery and spectroscopy_of_the_young_jovian_planet_51_eri_b_with_the_gemin...Sérgio Sacani
Indo além da descoberta e imageamento de um jovem Júpiter, os astrônomos usando o novo instrumento do Observatório Gemini, Planet Imager, o GPI, eles pesquisaram um mundo recém-descoberto com detalhes sem precedentes. O que eles encontraram é um planeta com cerca de duas vezes a massa de Júpiter, e o exoplaneta mais parecido com um planeta do Sistema Solar já imageado diretamente ao redor de outra estrela.
O exoplaneta, conhecido como 51 Eridani b, orbita sua estrela hospedeira a uma distância equivalente a 13 vezes a distância da Terra ao Sol (o equivalente a uma distância entre Saturno e Urano no nosso Sistema Solar). O sistema está localizado a cerca de 100 anos-luz de distância. Os dados do Gemini, também forneceram aos cientistas as detecções espectroscópicas de metano já detectadas na atmosfera de um planeta fora do nosso Sistema Solar, adicionando mais similaridades desse exoplaneta com os planetas gigantes do nosso Sistema Solar.
Particle physics aims to determine what matter is made of by searching for elementary particles that cannot be broken down further. Particle accelerators like linear colliders and cyclotrons smash particles together to deduce their structure. Unstable particles decay into more stable configurations with lower energy over time, which is why common matter is composed of protons, neutrons, and electrons.
The paper proposes a model of a unitary quantum field theory where the particle is represented as a wave packet. The frequency dispersion equation is chosen so that the packet periodically appears and disappears without changing its form. The envelope of the process is identified with a conventional wave function. Equation of such a field is nonlinear and relativistically invariant. With proper adjustments, they are reduced to Dirac, Schroedinger and Hamilton-Jacobi equations. A number of new experimental effects are predicted both for high and low energies.
This document contains advice from Flip Tanedo for communicating science effectively to policymakers. It discusses knowing your goals and audience, being aware that your audience may have assumptions about you, and the importance of practice. It also announces an upcoming workshop on improvisational theater exercises led by communication professor Annika Speer, which are meant to help speakers practice responding flexibly to unexpected situations or questions. The exercises include forming scenes or machines with other participants through repetition and responding to prompts.
Presentation about ParticleBites.com efforts in the context of sustainability as part of the Sustainable HEP 2nd ed. workshop. https://indico.cern.ch/event/1160140/timetable/
Presented at the 2022 APS April Meeting, session Z05.00009
Abstract: We present a novel approach for student assessment in large physics lecture courses on student-recorded videos. Students record 5-minute videos teaching how to solve a problem to other students and are partially graded based on peer reviews from other students. After piloting this method during COVID-19 remote teaching over the last year and a half, we have found encouraging indications that it (1) promotes student self-efficacy and metacognition, (2) builds in a deeper engagement with the material, (3) encourages student creativity, (4) develops technical and critical communication ability, and (5) avoids long-standing issues with digital plagiarism. Though the method was developed during pandemic teaching, we propose that aspects can be readily applied to in-person teaching and scales with class size. We comment on the potential to support diverse student retention in physics and outline potential pedagogical trade-offs of this method.
This document summarizes Flip Tanedo's presentation on equity as an early career academic. Tanedo discusses their experience on the tenure track and lessons learned. As a student, the focus is individual survival and support, but as a faculty member the goals shift to lifting others, changing institutions, and stewarding disciplines through mentoring and persistence. Achieving equity requires understanding incentives and compensating equity work. Building trust in institutions is important but fragile, so efforts should reaffirm shared values.
Popular Book Discussions: a platform for equity in physicsFlip Tanedo
The document discusses a framework for book club discussions between high school teachers and university physicists about equity in physics. It proposes using popular science books as a common ground to have discussions across different backgrounds and lived experiences. It provides an example of a pilot program where this was done as part of a physics teacher training with discussions of the book "Women in Physics". The goal is to improve preparation of students for university physics and make undergraduate education more inclusive. It suggests expanding this to a network of coordinated book clubs across districts and connections to broader physics education initiatives.
Non-Traditional Assessment and Inclusivity in Physics TeachingFlip Tanedo
This document discusses non-traditional methods of assessment in physics courses, inspired by remote teaching necessitated by the COVID-19 pandemic. It describes using explainer videos created by students to teach concepts to peers, followed by peer review, as well as one-on-one interviews, as alternatives to exams. The goal is to develop students' physics identity and sense of belonging in physics through assessing in a way that emphasizes creativity, communication, and viewing students as physics experts. Examples from a thermodynamics course are provided.
This document contains a presentation by Prof. Flip Tanedo about their background and work. It discusses Prof. Tanedo's educational and professional experiences, including being the first in their family to attend college. It also describes their research focusing on theoretical particle physics and dark matter. Prof. Tanedo shares their goal of increasing equity in science through teaching and mentoring students from underrepresented groups.
The document discusses building a model of a dark sector with vector dark matter and a light vector mediator particle. It notes some previous related work in this area and outlines that this work will focus on constructing a new model with a massive spin-1 mediator particle and no additional fermions. The presentation will describe the new model but not explore new phenomena or technical naturalness.
This document discusses warped dark sectors, where a dark matter particle interacts with standard model particles through a continuum of mediator states rather than a single particle. Key points:
1) A warped extra dimension with a bulk mediator field can encode a continuum/tower of Kaluza-Klein states that goes beyond the narrow width approximation at high energies.
2) The propagator for a bulk mediator field can be represented as a sum over individual KK modes or using the continuum approximation, both of which reproduce the expected fractional power potential at long distances.
3) Self-interactions in the bulk can cause high-mass KK states to have large widths and cascade decays, suppressing on-shell production but maintaining off
Flip Tanedo presented work on warped dark sectors at the KIAS HEP-PH seminar. The talk reviewed dark sectors and theories with extra dimensions. In a warped dark sector, dark matter interacts with standard model particles through a bulk mediator particle. Having many Kaluza-Klein modes of the mediator leads to qualitatively different behavior compared to a few mediators. On-shell particles produced with high momentum in the UV brane may cascade decay into lower modes through bulk self-interactions, staying below the position-dependent cutoff of the effective field theory. This opacity allows timelike momenta to propagate through the extra dimension without violating EFT validity.
Whatever Happened to the WIMP of Tomorrow?Flip Tanedo
This document discusses dark matter and the potential for new discoveries. It begins by outlining how discovering the particle that makes up dark matter could lead to new fundamental insights or the ability to manipulate regular matter in new ways. It uses an analogy of suddenly learning there are new rules or pieces to a game that has been played one's whole life. The document advocates exploring dark matter further rather than remaining "in the dark" about such a large component of the universe. It notes dark matter may be made of something unfamiliar that could have unexpected properties and interactions.
Physics Investigatory Project on transformers. Class 12thpihuart12
Physics investigatory project on transformers with required details for 12thes. with index, theory, types of transformers (with relevant images), procedure, sources of error, aim n apparatus along with bibliography🗃️📜. Please try to add your own imagination rather than just copy paste... Hope you all guys friends n juniors' like it. peace out✌🏻✌🏻
Presentation of our paper, "Towards Quantitative Evaluation of Explainable AI Methods for Deepfake Detection", by K. Tsigos, E. Apostolidis, S. Baxevanakis, S. Papadopoulos, V. Mezaris. Presented at the ACM Int. Workshop on Multimedia AI against Disinformation (MAD’24) of the ACM Int. Conf. on Multimedia Retrieval (ICMR’24), Thailand, June 2024. https://doi.org/10.1145/3643491.3660292 https://arxiv.org/abs/2404.18649
Software available at https://github.com/IDT-ITI/XAI-Deepfakes
Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...Sérgio Sacani
Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation
Order : Trombidiformes (Acarina) Class : Arachnida
Mites normally feed on the undersurface of the leaves but the symptoms are more easily seen on the uppersurface.
Tetranychids produce blotching (Spots) on the leaf-surface.
Tarsonemids and Eriophyids produce distortion (twist), puckering (Folds) or stunting (Short) of leaves.
Eriophyids produce distinct galls or blisters (fluid-filled sac in the outer layer)
Sexuality - Issues, Attitude and Behaviour - Applied Social Psychology - Psyc...PsychoTech Services
A proprietary approach developed by bringing together the best of learning theories from Psychology, design principles from the world of visualization, and pedagogical methods from over a decade of training experience, that enables you to: Learn better, faster!
Embracing Deep Variability For Reproducibility and Replicability
Abstract: Reproducibility (aka determinism in some cases) constitutes a fundamental aspect in various fields of computer science, such as floating-point computations in numerical analysis and simulation, concurrency models in parallelism, reproducible builds for third parties integration and packaging, and containerization for execution environments. These concepts, while pervasive across diverse concerns, often exhibit intricate inter-dependencies, making it challenging to achieve a comprehensive understanding. In this short and vision paper we delve into the application of software engineering techniques, specifically variability management, to systematically identify and explicit points of variability that may give rise to reproducibility issues (eg language, libraries, compiler, virtual machine, OS, environment variables, etc). The primary objectives are: i) gaining insights into the variability layers and their possible interactions, ii) capturing and documenting configurations for the sake of reproducibility, and iii) exploring diverse configurations to replicate, and hence validate and ensure the robustness of results. By adopting these methodologies, we aim to address the complexities associated with reproducibility and replicability in modern software systems and environments, facilitating a more comprehensive and nuanced perspective on these critical aspects.
https://hal.science/hal-04582287
Evaluation and Identification of J'BaFofi the Giant Spider of Congo and Moke...MrSproy
ABSTRACT
The J'BaFofi, or "Giant Spider," is a mainly legendary arachnid by reportedly inhabiting the dense rain forests of
the Congo. As despite numerous anecdotal accounts and cultural references, the scientific validation remains more elusive.
My study aims to proper evaluate the existence of the J'BaFofi through the analysis of historical reports,indigenous
testimonies and modern exploration efforts.
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...Sérgio Sacani
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
Compositions of iron-meteorite parent bodies constrainthe structure of the pr...Sérgio Sacani
Magmatic iron-meteorite parent bodies are the earliest planetesimals in the Solar System,and they preserve information about conditions and planet-forming processes in thesolar nebula. In this study, we include comprehensive elemental compositions andfractional-crystallization modeling for iron meteorites from the cores of five differenti-ated asteroids from the inner Solar System. Together with previous results of metalliccores from the outer Solar System, we conclude that asteroidal cores from the outerSolar System have smaller sizes, elevated siderophile-element abundances, and simplercrystallization processes than those from the inner Solar System. These differences arerelated to the formation locations of the parent asteroids because the solar protoplane-tary disk varied in redox conditions, elemental distributions, and dynamics at differentheliocentric distances. Using highly siderophile-element data from iron meteorites, wereconstruct the distribution of calcium-aluminum-rich inclusions (CAIs) across theprotoplanetary disk within the first million years of Solar-System history. CAIs, the firstsolids to condense in the Solar System, formed close to the Sun. They were, however,concentrated within the outer disk and depleted within the inner disk. Future modelsof the structure and evolution of the protoplanetary disk should account for this dis-tribution pattern of CAIs.
JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDSSérgio Sacani
The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.
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A B O U T 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
15 January 2020 Physics 288
UC Riverside Particle Theory
HOW TO HEP-PH
theory.ucr.edu
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Faculty
Yanou Haibo Flip Jose
Brian (HMC) Ernest (emeritus)
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So you can imagine life is quite difficult
John Mulaney
The Comeback Kid
Netflix
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What we work on
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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
How do we “do particle physics”
on this stuff?
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Other curious puzzles
Why is the weak scale stable vs. quantum
corrections?
Why is there more matter than antimatter?
Are neutrinos trying to tell us something?
How can other fields tell us about our
theory of matter and forces?
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Particle Phenomenology
MYSTERY
examples:
Theory: what makes W scattering unitary? (Higgs boson)
Experiment: observed excess in 𝛾-rays … dark matter?
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Particle Phenomenology
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Particle Phenomenology
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Particle Phenomenology
PREDICTION MYSTERY
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Where we earn our stripes
HACK
full theory
predictions
interpretation
consistency
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world
expert
on this
space of ideas
Light Mediators
dark matter
capture
Supersymmetry
you
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space of ideas
Dark
Matter
Theory of Strong Dynamics
Cosmology
Other funny ideas …
Collider Physics
new
searches
still you, but closer to scale
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Hai-Bo’s Catechism
THE KEY TO SUCCESS:
10 hours per day
6 days a week
… REPEAT FOR 10 YEARS
from Hai-Bo Yu
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Advice
Find material appropriate to your level and interests, and
read aggressively: lectures, review articles.
Better: keep a notebook and do calculations. Write them
pedagogically, and let yourself be wrong. Aim to be
wrong in every reasonable way and annotate the pitfalls.
Your work