Nova: The Fabric of the Cosmos

The Fabric of the Cosmos

Watch a live webcast with Brian Greene November 2 at 10pm - Watch the webcast. Hosted by The World Science Festival, Columbia University, and NOVA, this webcast will allow in-theatre and digital audiences to further explore the program's rich material in direct conversation with Greene and other featured program participants. You can ask questions in advance at the World Science Festival Facebook page.


"The Fabric of the Cosmos," a four-hour series based on the book by renowned physicist and author Brian Greene, takes us to the frontiers of physics to see how scientists are piecing together the most complete picture yet of space, time, and the universe. With each step, audiences will discover that just beneath the surface of our everyday experience lies a world we’d hardly recognize—a startling world far stranger and more wondrous than anyone expected.


Brian Greene is going to let you in on a secret: We've all been deceived. Our perceptions of time and space have led us astray. Much of what we thought we knew about our universe—that the past has already happened and the future is yet to be, that space is just an empty void, that our universe is the only universe that exists—just might be wrong.


Interweaving provocative theories, experiments, and stories with crystal-clear explanations and imaginative metaphors like those that defined the groundbreaking and highly acclaimed series "The Elegant Universe," "The Fabric of the Cosmos" aims to be the most compelling, visual, and comprehensive picture of modern phys

Watch live streaming video from worldsciencefestival at livestream.com

See: Live Forum

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Brian Greene, "The Fabric of the Cosmos: Space, Time, and the Texture of Reality"
Vintage | 2005 | ISBN: 0375727205 | 592 pages

One harmonious possibility is that string enthusiasts and loop quantum gravity aficionados are actually constructing the same theory, but from vastly different starting points. That each theory involves loops-in string theory, these are string loops; in loop quantum gravity, they're harder to describe non mathematically, but. roughly speaking, they're elementary loops of space-suggests there might be a connection. This possibility is further supported by the fact that on a few problems accessible to both, such as blackhole entropy, the two theories agree fully. And on the question of spacetime's constituents, both theories suggest that there is some kind of atomized structure. Page 490, Fabric of the Cosmos by Brian Greene

See Also:

• Liminocentric Structures: Which Circle do you Belong Too?
  

• Proton Collision ->Decay to Muons and Muon Neutrinos ->Tau Neutrino ->

Jet Manifestation: A World Unto Itself.

The Landscape Again and again....

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(September 20, 2010) Leonard Susskind gives a lecture on the string theory and particle physics. He is a world renown theoretical physicist and uses graphs to help demonstrate the theories he is presenting.

String theory (with its close relative, M-theory) is the basis for the most ambitious theories of the physical world. It has profoundly influenced our understanding of gravity, cosmology, and particle physics. In this course we will develop the basic theoretical and mathematical ideas, including the string-theoretic origin of gravity, the theory of extra dimensions of space, the connection between strings and black holes, the "landscape" of string theory, and the holographic principle.

This course was originally presented in Stanford's Continuing Studies program.

Stanford University:
http://www.stanford.edu/

Stanford Continuing Studies Program:
http://csp.stanford.edu/

Stanford University Channel on YouTube:
http://www.youtube.com/stanford

 Playlist

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Quarks, gluons and anti-quarks are the constituents of protons, neutrons and (by definition) other hadrons.  It is a fascinating aspect of the physics of our world that when one of these particles is kicked out of the hadron that contains it, flying out with high motion-energy, it is never observed macroscopically. Instead, a high-energy quark (or gluon or anti-quark) is transformed into a spray of hadrons [particles made from quarks, antiquarks and gluons].  This spray is called a “jet.” [Note this statement applies to the five lighter flavors of quark, and not the top quark, which decays to a W particle and a bottom quark before a jet can form.] See: Jets: The Manifestation of Quarks and Gluons

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 Quark Soup: Applied Superstring Theory- 

See Also:

• Quark Soup: Applied Superstring Theory
•  How Particles Came to be? 
•  
• The First Few Microseconds, by Michael Riordan and Willaim A. Zajc
  

  For the past five years, hundreds of scientists have been using a powerful new atom smasher at Brookhaven National Laboratory on Long Island to mimic conditions that existed at the birth of the universe. Called the Relativistic Heavy Ion Collider (RHIC, pronounced "rick"), it clashes two opposing beams of gold nuclei traveling at nearly the speed of light. The resulting collisions between pairs of these atomic nuclei generate exceedingly hot, dense bursts of matter and energy to simulate what happened during the first few microseconds of the big bang. These brief "mini bangs" give physicists a ringside seat on some of the earliest moments of creation. 

  
  During those early moments, matter was an ultrahot, superdense brew of particles called quarks and gluons rushing hither and thither and crashing willy-nilly into one another. A sprinkling of electrons, photons and other light elementary particles seasoned the soup. This mixture had a temperature in the trillions of degrees, more than 100,000 times hotter than the sun's core.

The Developmental Jet Process

As a layman I have been going through the research of those better educated then I in order to construct a accurate syntactically written developed scientific process as I have become aware of it. This is what I have been doing for the last number of years so as to get some idea of the scientific process experimentally driven to this point.

Theoretical development is important to myself,  as well as,   the underlying quest for a foundational perspective of how we can push back perspective with regard to the timeline of the universe in expression.

This has to be experimentally written in the processes we now use to help formulate an understanding of how the universe came into being by examining local events with the distribution of the cosmological data we are accumulating. A Spherical Cow anyone?

Jets: Article Updated An update here as well, "Two-Photons: Data and Theory Disagree"

I do appreciate all those scientist who have been giving their time to educating the public. This is a big thank you for that devotion to the ideal of bringing society forward as to what we as a public are not privy too. As too, being not part of that 3% of the population who are far removed from the work being done in particle research.

Almost a year ago, I had an e-mail exchange, and planned a phone call, with Maria Spiropulu of CMS. She looked particularly excited about something and the mortals may be learning what the cause was today.

CMS turned out to be much more "aggressive" relatively to the "conservative" ATLAS detector and it has already provided us with some hints. But what they published today, in the paper called: See: CMS: a very large excess of diphotons

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Measurement of the Production Cross Section for Pairs of Isolated Photons in pp collisions at sqrt(s) = 7 TeV

The integrated and differential cross sections for the production of pairs of isolated photons is measured in proton-proton collisions at a centre-of-mass energy of 7 TeV with the CMS detector at the LHC. A data sample corresponding to an integrated luminosity of 36 inverse picobarns is analysed. A next-to-leading-order perturbative QCD calculation is compared to the measurements. A discrepancy is observed for regions of the phase space where the two photons have an azimuthal angle difference, Delta(phi), less than approximately 2.8. 

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Tscan

Tscan ("Trivial Scanner") is an event display, traditionally called a scanner, which I developed. It is a program that shows events graphically on the computer screen.

It was designed to be simple ("trivial") internally, and to have a simple user interface. A lot of importance was given to giving the user a large choice of options to display events in many different ways.

Tscan proved to be a very useful tool for the development of fitters. A particularly useful feature is the ability to show custom data for every photpmultiplier tube (PMT). Instead of the usual time and charge, it can show expected charge, scattered light, likelihood, chi-squared difference, patches, and any other data that can be prepared in a text format.

See:Trivial Scanner

Credit: Super-Kamiokande/Tomasz Barszczak Three (or more?) Cerenkov rings

Multiple rings of Cerenkov light brighten up this display of an event found in the Super-Kamiokande - neutrino detector in Japan. The pattern of rings - produced when electrically charged particles travel faster through the water in the detector than light does - is similar to the result if a proton had decayed into a positron and a neutral pion. The pion would decay immediately to two gamma-ray photons that would produce fuzzy rings, while the positron would shoot off in the opposite direction to produce a clearer ring. Such kinds of decay have been predicted by "grand unified theories" that link three of nature's fundamental forces - the strong, weak and electromagnetic forces. However, there is so far no evidence for such decays; this event, for example, did not stand up to closer scrutiny.

See:

• Picture of the Week

Update

See Also:

• CMS Physics Results
• The Plot Of The Week - Z Plus Jets
• B-Quark Jets: Keys To New Discoveries
• CMS Bosons!
• Two Jets, Two Protons, Nothing Else
• A Short Story Of Dijet Resonances
• New CMS Results On Dijet Resonances

2010 ion run: completed!

What Does the Higgs Jet Energy Sound Like?

Justin Hall-Tipping: Freeing energy from the grid

The grid of tomorrow is no grid, and energy, clean efficient energy, will one day be free. If you do this, you get the last puzzle piece, which is water. Each of us, every day, need just eight glasses of this, because we're human. When we run out of water, as we are in some parts of the world and soon to be in other parts of the world, we're going to have to get this from the sea, and that's going to require us to build desalination plants. 19 trillion dollars is what we're going to have to spend. These also require tremendous amounts of energy. In fact, it's going to require twice the world's supply of oil to run the pumps to generate the water. We're simply not going to do that. But in a world where energy is freed and transmittable easily and cheaply, we can take any water wherever we are and turn it into whatever we need.

VS Ramachandran: The neurons that shaped civilization

VS Ramachandran: The neurons that shaped civilization | Video on TED.com

• Neuroscientist Vilayanur Ramachandran outlines the fascinating functions of mirror neurons. Only recently discovered, these neurons allow us to learn complex social behaviors, some of which formed ...
• http://www.ted.com/talks/lang/en/vs_ramachandran_the_neurons_that_shaped_civilization.html

Gran Sasso and Fermilab

Gran Sasso

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deconstruction: soudan mural

The Soudan mural is next to the 6000-ton MINOS detector. Mural artists: Joseph Giannetti, Leila Giannetti, Mick Pulsifer. Funded by a grant from the University of Minnesota. (Credit: Fermilab Visual Media Services)

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Fermilab experiment weighs in on neutrino mystery

Scientists of the MINOS experiment at the Department of Energy’s Fermi National Accelerator Laboratory announced today (June 24) the results from a search for a rare phenomenon, the transformation of muon neutrinos into electron neutrinos. The result is consistent with and significantly constrains a measurement reported 10 days ago by the Japanese T2K experiment, which announced an indication of this type of transformation.

The results of these two experiments could have implications for our understanding of the role that neutrinos may have played in the evolution of the universe. If muon neutrinos transform into electron neutrinos, neutrinos could be the reason that the big bang produced more matter than antimatter, leading to the universe as it exists today.

The Main Injector Neutrino Oscillation Search (MINOS) at Fermilab recorded a total of 62 electron neutrino-like events. If muon neutrinos do not transform into electron neutrinos, then MINOS should have seen only 49 events. The experiment should have seen 71 events if neutrinos transform as often as suggested by recent results from the Tokai-to-Kamioka (T2K) experiment in Japan. The two experiments use different methods and analysis techniques to look for this rare transformation.

To measure the transformation of muon neutrinos into other neutrinos, the MINOS experiment sends a muon neutrino beam 450 miles (735 kilometers) through the earth from the Main Injector accelerator at Fermilab to a 5,000-ton neutrino detector, located half a mile underground in the Soudan Underground Laboratory in northern Minnesota. The experiment uses two almost identical detectors: the detector at Fermilab is used to check the purity of the muon neutrino beam, and the detector at Soudan looks for electron and muon neutrinos. The neutrinos’ trip from Fermilab to Soudan takes about one four hundredths of a second, giving the neutrinos enough time to change their identities.

For more than a decade, scientists have seen evidence that the three known types of neutrinos can morph into each other. Experiments have found that muon neutrinos disappear, with some of the best measurements provided by the MINOS experiment. Scientists think that a large fraction of these muon neutrinos transform into tau neutrinos, which so far have been very hard to detect, and they suspect that a tiny fraction transform into electron neutrinos.

The observation of electron neutrino-like events in the detector in Soudan allows MINOS scientists to extract information about a quantity called sin² 2θ₁₃ (pronounced sine squared two theta one three). If muon neutrinos don’t transform into electron neutrinos, this quantity is zero. The range allowed by the latest MINOS measurement overlaps with but is narrower than the T2K range. MINOS constrains this quantity to a range between 0 and 0.12, improving on results it obtained with smaller data sets in 2009 and 2010. The T2K range for sin² 2θ₁₃ is between 0.03 and 0.28.

“MINOS is expected to be more sensitive to the transformation with the amount of data that both experiments have,” said Fermilab physicist Robert Plunkett, co-spokesperson for the MINOS experiment. “It seems that nature has chosen a value for sin² 2θ₁₃ that likely is in the lower part of the T2K allowed range. More work and more data are really needed to confirm both these measurements.”
The MINOS measurement is the latest step in a worldwide effort to learn more about neutrinos. MINOS will continue to collect data until February 2012. The T2K experiment was interrupted in March when the severe earth quake in Japan damaged the muon neutrino source for T2K. Scientists expect to resume operations of the experiment at the end of the year. Three nuclear-reactor based neutrino experiments, which use different techniques to measure sin² 2θ₁₃, are in the process of starting up.

“Science usually proceeds in small steps rather than sudden, big discoveries, and this certainly has been true for neutrino research,” said Jenny Thomas from University College London, co-spokesperson for the MINOS experiment. “If the transformation from muon neutrinos to electron neutrinos occurs at a large enough rate, future experiments should find out whether nature has given us two light neutrinos and one heavy neutrino, or vice versa. This is really the next big thing in neutrino physics.”
The MINOS experiment involves more than 140 scientists, engineers, technical specialists and students from 30 institutions, including universities and national laboratories, in five countries: Brazil, Greece, Poland, the United Kingdom and the United States. Funding comes from: the Department of Energy Office of Science and the National Science Foundation in the U.S., the Science and Technology Facilities Council in the U.K; the University of Minnesota in the U.S.; the University of Athens in Greece; and Brazil's Foundation for Research Support of the State of São Paulo (FAPESP) and National Council of Scientific and Technological Development (CNPq).

Fermilab is a national laboratory supported by the Office of Science of the U.S. Department of Energy, operated under contract by Fermi Research Alliance, LLC.
For more information about MINOS and related experiments, visit the Fermilab neutrino website: http://www.fnal.gov/pub/science/experiments/intensity/

See: 

Intensity Frontier

See Also: The Reference Frame: CMS: a very large excess of diphotons

TRIUMF Dragon

ISAC and DRAGON, the Detector of Recoils And Gammas Of Nuclear reactions

TRIUMF has long been addressing big questions about the origins of matter in our universe by studying the interactions among elementary particles or essential nuclei.  The DRAGON experiment at TRIUMF is an apparatus designed to measure the rates of nuclear reactions that are important in astrophysics and the formation of the chemical elements. The big question we are asking is, "Where do the elements around us come from?" and "What happens inside a supernova and what does it produce?"  One new experiments at TRIUMF, S1227, recently looked at a process that creates lithium and neutrinos within ancient stars. See: A New Look Inside Ancient Stars

ICECUBE Neutrinos

Another Big thank you to ICECUBE Blog.

The IceCube project at the South Pole needed a new server cluster to reconstruct raw data, so it selected Dell PowerEdge servers for the HPC solution.

The IceCube Neutrino Observatory has just completed construction in Antarctica as of January 2011, and will help scientists search for elusive neutrinos that can help us map out the universe in new and exciting ways. I traveled to the South Pole in November and December 2009 to participate in this project, and reported back to classrooms across the US. This stop-motion animated video is an introduction to the IceCube Neutrino Observatory, answering basic questions such as: What is a neutrino? how can we detect them? How does IceCube work? See: Dell Powers IceCube Neutrino Observatory in Antartica

XKCD Significant-Speed of Light Issue?

You got to love it when correlations can be made, and a thank you to the ICECUBE Blog

If the histograms and data are exactly right, the paper quotes a one-in-ten-thousand (0.0001) chance that this bump is a fluke. That's pretty small; although bear in mind that lots of distributions like this get plotted. If you plot 100 different distributions, the chances become about one in a hundred (0.01) that you'll see something odd in one of them. The Tevatron goes bump

http://imgs.xkcd.com/comics/significant.png

ICECUBE Blogging Research Material and more

In regards to Cherenkov Light

Thinking outside the box See: A physicist inthe cancer lab

Ackerman became interested in physics in middle school, reading popular science books about quantum mechanics and string theory. As an undergraduate at the Massachusetts Institute of Technology, she traveled to CERN, the European particle physics laboratory near Geneva, to work on one of the detectors at the Large Hadron Collider, the most powerful particle collider in the world. Then she spent a summer at SLAC working on BaBar, an experiment investigating the universe’s puzzling shortage of antimatter, before starting her graduate studies there in 2007.

 Linking Experiments(Majorana, EXO); How do stars create the heavy elements? (DIANA); What role did neutrinos play in the evolution of the universe? (LBNE). In addition, scientists propose to build a generic underground facility (FAARM) ...

 Dialogos of Eide: Neutrinoless Double Beta DecayCOBRA · CUORICINO and CUORE · EXO · GERDA · MAJORANA · MOON · NEMO-3 and SuperNEMO · SNO+. See Also:Direct Dark Matter Detection.

Also From my research:

1. Neutrinoless Double Beta Decay
   
2. A first look at the Earth interior from the Gran Sasso underground laboratory
   
3. Mysterious Behavior of Neutrinos sent Straight through the Earth
   

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ICECUBE Blog put up some links that I wanted to go through to see what is happening there. Their links provided at bottom of blog post here. Each link of theirs I have provided additional information in concert while I explore above.

• Cherenkov light: Not just for physics anymore (Symmetry)
• First planes at the Pole (The Antarctic Sun)
• The magical neutrino (the guardian)
• Computing from the end of the Earth (insideHPC)
• Entertaining with IceCube (Lekue)