tag:blogger.com,1999:blog-78155489725570220502017-04-20T13:45:58.202-07:00Cosmology Symmetry Breaking through Higgs MechanismH Peter Alessonoreply@blogger.comBlogger3125tag:blogger.com,1999:blog-7815548972557022050.post-83355341174220352682017-03-02T13:44:00.000-08:002017-04-16T12:07:53.016-07:00Standard Model LagranianThe Standard Model of Particle Physics has helped unravel the hidden symmetries within the design of the Universe. Here we examine the steps in building the Standard Model.<br /><br /><b>1. The Universe </b>was created out of interacting quantum fields of harmonic oscillating excitation with particle-like eigenfunctions.<br /><br />A field is represented at some space-time point by an amplitude (scalar, vector, complex number, spinor, or tensor) that oscillates in space-time to produce wave-like excitation.<br /><br />Quantum field theory explains why electrons are identical because each electron is an excitation of the electron quantum field with identical properties using Fermi-Dirac statistics.<br /><br />Lagrangian Field Theory formulates the relativistic quantum mechanical theory of interactions. It has dependent variables replaced by values of a field at a point in space-time f (x,y,z,t). The equations of motion are obtained by the Action Principle where S is Action. <span style="text-align: center;">Energy is conserved if the Lagrangian doesn’t change with time. </span><br /><span style="text-align: center;"><br /></span>The Euler-Lagrange Equation produces the model's equation of motion:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://4.bp.blogspot.com/-ovjUFmFdvqc/V8MnKdOsqpI/AAAAAAAAAqg/xbIHFBdxQEEPG5w89kbTJYkN7jGylsUnACPcB/s1600/aa2.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="83" src="https://4.bp.blogspot.com/-ovjUFmFdvqc/V8MnKdOsqpI/AAAAAAAAAqg/xbIHFBdxQEEPG5w89kbTJYkN7jGylsUnACPcB/s320/aa2.png" width="320" /></a></div>The steps to construct the Standard Model of Quantum Field Theory start with the classical Lagrangian, L.<br /><br /><b>2. The Lagrangian density function, L</b><br /><br />Maxwell’s Equations<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://1.bp.blogspot.com/-rS25E9RlXNs/V8MoDA2nl6I/AAAAAAAAAqg/j0Os_a1Z9t0G2J5dZd6C_WVFEsGfo6NqQCPcB/s1600/aa3.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="101" src="https://1.bp.blogspot.com/-rS25E9RlXNs/V8MoDA2nl6I/AAAAAAAAAqg/j0Os_a1Z9t0G2J5dZd6C_WVFEsGfo6NqQCPcB/s320/aa3.png" width="320" /></a></div>The L for Classical Electrodynamics:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://1.bp.blogspot.com/-XNuRVL2JUlI/V8MoMhQDZtI/AAAAAAAAAqg/7Hgy6oBSRVMNSBe7D1w7WmLCWBnX4EwnQCPcB/s1600/aa4.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="253" src="https://1.bp.blogspot.com/-XNuRVL2JUlI/V8MoMhQDZtI/AAAAAAAAAqg/7Hgy6oBSRVMNSBe7D1w7WmLCWBnX4EwnQCPcB/s320/aa4.png" width="320" /></a></div>Next consider, the Lagrangian density function for a massless field:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://2.bp.blogspot.com/-N8owXlClqH0/V8MokmnlN5I/AAAAAAAAAqg/-gjW9dpgp3omK6B3sPM-Z60vcoKAGJHBACPcB/s1600/aa5.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="81" src="https://2.bp.blogspot.com/-N8owXlClqH0/V8MokmnlN5I/AAAAAAAAAqg/-gjW9dpgp3omK6B3sPM-Z60vcoKAGJHBACPcB/s320/aa5.png" width="320" /></a></div>Adding mass creates the scalar (spin j=0) Klein Gordon<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://3.bp.blogspot.com/-oUCeX9Pe208/V8Mop9wBaCI/AAAAAAAAAqg/2cfqBYlzixgeRddpts56_PRszpZ1M-tNgCPcB/s1600/aa6.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="65" src="https://3.bp.blogspot.com/-oUCeX9Pe208/V8Mop9wBaCI/AAAAAAAAAqg/2cfqBYlzixgeRddpts56_PRszpZ1M-tNgCPcB/s320/aa6.png" width="320" /></a></div>The solutions to the Klein Gordon Equation are simple plane waves subject to relativistic constraint:<br /><br /><div style="text-align: center;"><span style="background-color: white; color: #333333; font-family: "symbol"; font-size: 14pt;">f</span><span style="background-color: white; color: #333333; font-family: "arial" , "tahoma" , "helvetica" , "freesans" , sans-serif; font-size: 14pt;">(x)</span><span style="background-color: white; color: #333333; font-family: "arial" , "tahoma" , "helvetica" , "freesans" , sans-serif; font-size: 14pt;"> = e<sup>-+i(<b>p.x</b>-Et)</sup> </span></div><br />Introducing a source term produces J(x)<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://2.bp.blogspot.com/-MIz8nsMDDKI/V8Mo9lu3fhI/AAAAAAAAAqg/VZgtuAd-al4lpHHF5T8Y3Q6O4lQariEQACPcB/s1600/aa8.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="65" src="https://2.bp.blogspot.com/-MIz8nsMDDKI/V8Mo9lu3fhI/AAAAAAAAAqg/VZgtuAd-al4lpHHF5T8Y3Q6O4lQariEQACPcB/s320/aa8.png" width="320" /></a></div>For the case of a field with mass and interaction:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://2.bp.blogspot.com/-53dMRd1v24s/V8MpI5P4WII/AAAAAAAAAqg/HG9PCJA18gI6WW0_bwJAyBCicWtnqY3igCPcB/s1600/aa9.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="65" src="https://2.bp.blogspot.com/-53dMRd1v24s/V8MpI5P4WII/AAAAAAAAAqg/HG9PCJA18gI6WW0_bwJAyBCicWtnqY3igCPcB/s320/aa9.png" width="320" /></a></div>The relativistic quantum mechanical Dirac Lagrangian is<br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="https://3.bp.blogspot.com/-0pRJGLqq4i8/V8MpVg6hUMI/AAAAAAAAAqg/yvL88m6ISEgsPhfrL26UUTQEX7W5GDmOACPcB/s1600/eq11.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="93" src="https://3.bp.blogspot.com/-0pRJGLqq4i8/V8MpVg6hUMI/AAAAAAAAAqg/yvL88m6ISEgsPhfrL26UUTQEX7W5GDmOACPcB/s320/eq11.png" width="320" /></a></div><b>3. The Quantum Electrodynamic U(1):</b><br /><br />Tomonaga, Schwinger, Feynman) is a precise description of electromagnetic interactions.<br /><br />Feynman Diagram:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://4.bp.blogspot.com/-hWGQcfINDuU/VyuF6rYD2zI/AAAAAAAAAnQ/_moJ7po1HBweH2c8WyD0HMtzF7_cQ5CoACPcB/s1600/feynman.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="180" src="https://4.bp.blogspot.com/-hWGQcfINDuU/VyuF6rYD2zI/AAAAAAAAAnQ/_moJ7po1HBweH2c8WyD0HMtzF7_cQ5CoACPcB/s320/feynman.png" width="320" /></a></div>A loop in a Feynman diagram indicts a divergence (infinite integral) that must be renormalized for calculations.<br /><br /><div class="separator" style="clear: both; text-align: center;"></div>The Quantum Electrodynamics (QED) Lagrangian:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://3.bp.blogspot.com/-c-FU2Dgkn0A/V8MqPYs8g6I/AAAAAAAAArs/gqBLd7W7XU4DUm4QALKL9KLZ014uDTJJwCPcB/s1600/aa11.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="100" src="https://3.bp.blogspot.com/-c-FU2Dgkn0A/V8MqPYs8g6I/AAAAAAAAArs/gqBLd7W7XU4DUm4QALKL9KLZ014uDTJJwCPcB/s320/aa11.png" width="320" /></a></div><b>4. Next the Quantum ElectroWeak Theory SU(2):</b><br /><br />Salam and Weinberg developed a gauge theory requiring three gauge bosons (W+-,Z). The Quantum ElectroWeak (QEW) Lagranian:<br /><br /><div class="separator" style="clear: both; text-align: center;"></div><div class="separator" style="clear: both; text-align: center;"><a href="https://3.bp.blogspot.com/-78KrPb6jL8Q/WMbiXaqfqNI/AAAAAAAAAs4/-NnFbj3dGdoeblwhCvQWFMEACQhcj1NWwCLcB/s1600/a16.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="128" src="https://3.bp.blogspot.com/-78KrPb6jL8Q/WMbiXaqfqNI/AAAAAAAAAs4/-NnFbj3dGdoeblwhCvQWFMEACQhcj1NWwCLcB/s320/a16.png" width="320" /></a></div><br /><b>5. Quantum Chromodynamics SU(3):</b><br /><br />Han, Nambu, Greenburg described the strong force mediated by gauge bosons, called gluons, carrying a unique kind of charge called color. The Quantum Chromodynamics (QCD) Lagrangian:<br /><div class="separator" style="clear: both; text-align: center;"><a href="https://2.bp.blogspot.com/-zt6HHpeK9iM/V8Mqw9y37kI/AAAAAAAAArs/gGYAmmV8OngjNi1yFwjvZdWcKoTHjURMwCPcB/s1600/aa13.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="63" src="https://2.bp.blogspot.com/-zt6HHpeK9iM/V8Mqw9y37kI/AAAAAAAAArs/gGYAmmV8OngjNi1yFwjvZdWcKoTHjURMwCPcB/s320/aa13.png" width="320" /></a></div><b>6. The Standard Model SU(3) x SU(2) x U(1):</b><br /><br />The current structure of elementary particle physics is called the Standard Model. The Standard Model (SM) Lagrangian:<br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="https://4.bp.blogspot.com/-Cfp_-auabwM/WMWlcnxHj0I/AAAAAAAAAsg/9kF34QhGkNgEfPX4b-kXNyJz5DfzWeMrQCLcB/s1600/a15.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="157" src="https://4.bp.blogspot.com/-Cfp_-auabwM/WMWlcnxHj0I/AAAAAAAAAsg/9kF34QhGkNgEfPX4b-kXNyJz5DfzWeMrQCLcB/s320/a15.png" width="320" /></a></div><div class="separator" style="clear: both; text-align: center;"></div>The first line represents the kinetic energy carried by W, Z, photon, and gluons. The second line is the interaction terms. The third line contains mass and the fourth line the left right parity interaction.<br /><br /><b>References:</b><br /><br />[1] Cox, B. and Forshaw, J., Why does E=mc2, Da Capo Press, Cambridge, MA 2009.<br /><br />[2] Lancaster, T., and Blundell, S. j., Quantum Field Theory, Oxford, UK, 2014.<br /><br />[3] Robinson, M., Symmetry and the Standard Model, Springer, London, 2011.H Peter Alessohttps://plus.google.com/103789440897695412834noreply@blogger.com0tag:blogger.com,1999:blog-7815548972557022050.post-5721052005989543332017-02-28T13:41:00.004-08:002017-04-14T18:15:39.555-07:00Thinking on the Web: Berners-Lee, Gödel and TuringWhen the philosopher René Descartes proclaimed his famous observation "Cogito, ergo sum," he demonstrated the power of thought at the most basic level by deriving an important fact (i.e., the reality of his own existence) from the act of thinking and self awareness.<br /><br />The boldest attempt to apply logic to mathematics was pioneered by philosopher-logician Bertrand Russell, in<i> Principia Mathematia</i>. The idea was that mathematical theories were logical tautologies, and his program was to show this by means to a reduction of mathematics to logic. The various attempts to carry this out met with a series of failures, such as Russell's Paradox, and the defeat of Hilbert's Program by Gödel's incompleteness theorems.<br /><br />Russell's paradox represents either of two interrelated logical contradictions. The first is a contradiction arising in the logic of sets or classes. Some sets can be members of themselves, while others can not. The set of all sets is itself a set, and so it seems to be a member of itself. The null or empty set, however, must not be a member of itself. However, suppose that we can form a set of all sets that, like the null set, are not included in themselves. The paradox arises from asking the question of whether this set is a member of itself. It is, if and only if, it is not!<br /><br />While it was shown that non-Euclidean geometries were consistent relative to Euclidean geometry, proving the consistency of Euclidean geometry has not been achieved by mathematics. It was only found to be consistent as long as mathematics was consistent.<br /><br /><b>What is undefined?</b><br /><br />When students first envision the extensive mathematical landscape, they assume that it is a pristine smooth surface holding all the answers to every mathematical question - just waiting to be unearthed - point to the right spot and there's the answer. They soon discover, however, that the landscape is littered with irregularities, obstructions, and, in some spots, gaping holes.<br /><br /><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">Math and physics have a lot in common. For example, Infinity and c cannot be treated as ordinary numbers.<o:p></o:p></div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">Infinity seems to suffer from the contradiction: infinity + 1 = infinity <o:p></o:p></div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">which reduces to 1 = 0.<o:p></o:p></div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">The speed of light (c) seems to suffer a similar contradiction: c + 1 = c <o:p></o:p></div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">which reduces to 1 = 0.<o:p></o:p></div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">But, Special Relativity put time on the same level as spatial dimensions with the Lorentz transform superseding Newton’s Galilean transform and Einstein redefined how c was understood.</div><div class="MsoNormal" style="line-height: 107%; margin-bottom: 8.0pt;">Similarly, Cantor created aleph to redefined infinity through Cardinal and the Continuum Hypotheses so that infinity was no longer treated as an ordinary Real number. </div>Of particular importance is the fact that division by zero is literally undefined. Nevertheless, it repeatedly pops-up in the most important problems in science from nonlinear equations to Quantum Field Theory where it is finessed by renormalization (removing/cancelling singularities). When trying to reconcile the mathematical models of physical theories it is necessary to consider the failings of math itself.<br /><b><br /></b><b>What is decidable?</b><br /><br />In the 1930s, the logician, Kurt Gödel, established that, in certain important mathematical domains, there are problems that cannot be solved, or propositions that cannot be proved or disproved, and are therefore undecidable. In particular, the work of Kurt Gödel identified the concept of undecidability where the truth, or falsity, of some statements may not be determined. This is relevant to the field of artificial intelligence because of the limits and boundaries that can be inferred from Gödel's insights.<br /><b><br /></b><b>What is machine intelligence?</b><br /><br />In 1947, mathematician Alan Turing first started to seriously explore the concept of intelligent machines. He determined that a computing machine can be called intelligent if it could deceive a human into believing that it was human. His test — called the Turing Test — consists of a person asking a series of questions to both a human subject and a machine. The questioning is done via a keyboard so that the questioner has no direct interaction between subjects; man, or machine. A machine with true intelligence will pass the Turing Test by providing responses that are sufficiently human-like that the questioner cannot determine which responder is human and which is not.<br /><br />Recursion is the process a procedure goes through when one of the steps of the procedure involves rerunning a complete set of identical steps. In mathematics and computer science, recursion is a particular way of specifying a class of objects with the help of a reference to other objects of the class: a recursive definition defines objects in terms of the already defined objects of the class.<br /><br /><b>Is there art in mathematics?</b><br /><br />How much of math is reality-based and how much is art (avoiding irregularities and undefined features in math in order to reach an answer without running into a hole)?<br /><br />Consider:<br /><br /><div class="MsoNormal">e<sup>x</sup> = -1 was considered unsolvable until Euler discovered one solution:<o:p></o:p></div><div class="MsoNormal"><br /></div><div class="MsoNormal">e<sup>i</sup><sup>π</sup>= cos π + i(sin π) = -1 + 1*0 = -1<o:p></o:p></div><div class="MsoNormal"><br /></div><div class="MsoNormal">or rewritten as<o:p></o:p></div><div class="MsoNormal"><br /></div><div class="MsoNormal">Euler’s Equation e<sup>i</sup><sup>π</sup>+1 = 0<o:p></o:p></div><div class="MsoNormal"><br /></div><div class="MsoNormal">Where this one equation equates five fundamental elements of math:<o:p></o:p></div><div class="MsoNormal"><br /></div><div class="MsoNormal">0 = additive identity - a finite real number<o:p></o:p></div><div class="MsoNormal">1 = multiplicative identity - an integer real number<o:p></o:p></div><div class="MsoNormal">π = circular constant pi - a number with unending decimal places<o:p></o:p></div><div class="MsoNormal">e = the base of natural logarithms - an infinite series<o:p></o:p></div><div class="MsoNormal">i = imaginary unit<o:p></o:p></div><br /><div class="MsoNormal"><b>Question:</b>What does it 'mean' when we seek an ‘exact’ value to an infinite series? If it's true in the limit (approaching infinite) then Euler's Equation is an approximation - not an exact solution. </div>_______________________________________________<br /><br />The following excerpts from Alesso [<a href="https://www.amazon.com/Thinking-Web-Berners-Lee-G%C3%B6del-Turing/dp/0471768669/ref=sr_1_10?s=books&amp;ie=UTF8&amp;qid=1488313073&amp;sr=1-10&amp;keywords=alesso" target="_blank">1</a>] illustrate some of these fundamental concepts:<br /><br /><b>Interlude #1: Thinking about Thinking </b><br /><br />John picked up the two double Latte Grandes and walked over to the corner table near the fireplace where Mary was setting up the chess game. She took a pawn of each color and concealed them in her hands before offering two fists to John.<br /><br />Putting the cups down, he tapped Mary’s left hand and was pleased to see the white piece as he took his chair. <br /><br />John said “Playing chess always reminds me of the game between IBM’s Deep Blue Supercomputer and the reigning World Chess Champion at the time, Garry Kasparov.” He glanced at the board, “d4, I think” as he moved his pawn.<br /><br />Mary said, “Me too.” Mary smiled to herself as she moved her own queen’s pawn forward to d5. She knew that John had strong feelings about the limits of true Artificial Intelligence and she hoped to gain an advantage by baiting him. “That was the first time a computer won a complete match against the world’s best human player. It took almost 50 years of research in the field, but a computer finally was thinking like a human.”<br /><br />John bristled slightly, but then realized that Mary was just poking a little fun. Taking his next move, c4, he said “You can guess my position on that subject. The basic approach of Deep Blue was to decide on a chess move by assessing all possible moves and responses. It could identify up to a depth of about 14 moves and value-rank the resulting game positions using an algorithm developed in advance by a team of grand masters. Deep Blue did not think in any real sense. It was merely computational brute force.”<br /><br />Mary reached over and took John’s pawn, accepting the gambit. “You must admit,” she replied, “although Kasparov’s ‘thought’ processes were without a doubt something very different than Deep Blue’s, their performances were very similar. After all, it was a team of grand masters that designed Deep Blue’s decision-making ability to think like them.”<br /><br />John played his usual Nc3, continuing the main line of the Queen’s Pawn Gambit. “You’ve made my point,” he exclaimed, “Deep Blue did not make its own decisions before it moved. All it did was accurately execute, the very sophisticated judgments that had been pre-programmed by the human experts.”<br /><br />“Let’s look at it from another angle.” Mary said as she moved Nf6. “Much like a computer, Kasparov’s brain used its billions of neurons to carry out hundreds of tiny operations per second, none of which, in isolation, demonstrates intelligence. In totality, though, we call his play ‘brilliant.’ Kasparov was processing information very much like a computer does. Over the years, he had memorized and pre-analyzed thousands of positions and strategies."<br /><br />“I disagree,” said John quickly moving e3. “Deep Blue’s behavior was merely logic algebra – expertly and quickly calculated, I admit. However, logic established the rules between positional relationships and sets of value-data. A fundamental set of instructions allowed operations including sequencing, branching and recursion within an accepted hierarchy.”<br /><br />Mary grimaced and held up her hands, "No lectures please." Moving to e6 she added, "A perfectly reasonable alternative explanation to logic methods is to use heuristics methods, which observe and mimic the human brain. In particular, pattern recognition seems intimately related to a sequence of unique images connected by special relationships. Heuristic methods seem as effective in producing AI as logic methods. The success of Deep Blue in chess programming is important because it employed both logic and heuristic AI methods."<br /><br />"Now who’s lecturing," responded John, taking Mary’s pawn with his bishop. “In my opinion, human Grandmasters, do not examine 200,000,000 move sequences per second.”<br /><br />Without hesitation Mary moved c5 and said, "How do we know? Just because human grandmasters are not aware of searching such a number of positions doesn’t prove it. Individuals are generally unaware of what actually does go on in their minds. Patterns in the position suggest what lines of play to look at, and the pattern recognition processes in the human mind seem to be invisible to the mind."<br /><br />John said, "You mean like your playing the same Queen’s Gambit Accepted line over and over again?" as he castled.<br /><br />Ignoring him, Mary moved a6 and said, "Suppose most of the chess player’s skill actually comes from an ability to compare the current position against images of thousands of positions already studied. We would call selecting the best position (or image) insightful. Still, if the unconscious human version yields intelligent results, and the explicit algorithmic Deep Blue version yields essentially the same results, then why can't I call Deep Blue intelligent too?"<br /><br />John said, "I’m sorry, but for me you’ve overstated your case by calling Deep Blue intelligent,” moving Qe2. He continued, “ Would you like to reconsider your position?”<br /><br />Mary moved Nc3 and said, "Of course not, I still have plenty of options to think about, alone this line.”<br />_______________________________________________<br /><br /><b>Interlude #2: The Truth and Beauty of Math</b><br /><br />As John passed with a sour look on his face, Mary looked up from her text book and asked, “Didn’t you enjoy the soccer game?”<br /><br />“How can you even ask that when we lost?” asked John gloomily.<br /><br />“I think the team performed beautifully, despite the score” said Mary.<br /><br />This instantly frustrated John and he said, "Do you know Mary that sometimes I find it disarming the way you express objects in terms of beauty. I find that simply accepting something on the basis of its beauty can lead to false conclusions?"<br /><br />Mary reflected upon this before offering a gambit of her own, "Well John, do you know that sometimes I find that relying on objective truth alone can lead to unattractive conclusions."<br /><br />John became flustered and reflected his dismay by demanding, "Give me an example."<br /><br />Without hesitation, Mary said, "Perhaps you will recall that in the late 1920's, mathematicians were quite certain that every well-posed mathematical question had to have a definite answer ─ either true or false. For example, suppose they claimed that every even number was the sum of two prime numbers,” referring to Goldbach's Conjecture which she had just been studying in her text book. Mary continued, “Mathematicians would seek the truth or falsity of the claim by examining a chain of logical reasoning that would lead in a finite number of steps to prove if the claim were either true or false."<br /><br />"So mathematicians thought at the time," said John. "Even today most people still do."<br /><br />"Indeed," said Mary. "But in 1931, logician Kurt Gödel proved that the mathematicians were wrong. He showed that every sufficiently expressive logical system must contain at least one statement that can be neither proved nor disproved following the logical rules of that system. Gödel proved that not every mathematical question has to have a yes or no answer. Even a simple question about numbers may be undecidable. In fact, Gödel proved that there exist questions that while being undecidable by the rules of logical system can be seen to be actually true if we jump outside that system. But they cannot be proven to be true.”<br /><br />“Thank you for that clear explanation,” said John. “But isn’t such a fact simply a translation into mathematical terms of the famous Liar’s Paradox: ‘This statement is false.’”<br /><br />“Well, I think it's a little more complicated than that,” said Mary. “But Gödel did identify the problem of self-reference that occurs in the Liar’s Paradox. Nevertheless, Gödel’s theorem contradicted the thinking of most of the great mathematicians of his time. The result is that one can not be as certain as the mathematician had desired. See what I mean, Gödel may have found an important truth, but it was – well to be frank – rather disappointingly unattractive," concluded Mary.<br /><br />"On the contrary,” countered John, “from my perspective it was the beauty of the well-posed mathematical question offered by the mathematicians that was proven to be false.<br /><br />Mary replied, “I’ll have to think about that.”<br />_______________________________________________<br /><b><br /></b><b>Interlude #3: Computing Machines</b><br /><br />Having had the final word in their last discussion, John was feeling a little smug as he listened to his ipod. Mary sat down next to him on the library steps. Their last class had been on computer design and they were both thinking about just how far the new technology could evolve.<br /><br />John said, “As you suggested earlier, Gödel was concerned that a logic system had to be consistent and then he determined that no logic system can prove itself to be consistent.”<br /><br />“True,” replied Mary. “But it was Turing who built on Gödel’s findings. Shortly before WWII, Turing found a way to translate Gödel’s logic results about numbers and mathematics into analogous results about calculations and computing machines.”<br /><br />John interrupted, “Yes, Turing was convinced that mathematical problem solving could be reduced to simple steps that could be used to program computer actions."<br /><br />Mary said, “True. Turing considered the logical steps one goes through in constructing a proof as being the same steps that a human mind follows in a computation.” Mary gave John a sideways glance before continuing, “Turing was convinced that the ability to solve this type of mathematical problem is a significant indication of the ability of machines to duplicate human thought.”<br /><br />John dissented, “Wait a minute. We’ve been here before. Just because machines follow the same logical steps a human uses to solve a calculation doesn’t mean that they actually think. Since calculating machines are not biological, it seems unreasonable to me to suggest that machines are capable of actual creative thought. They may be mimicking the logical steps, but are they actually thinking? I think not.”<br /><br />“Therefore, you are not,” Mary said with a grin.<br /><br />John relied, “Hey.”<br /><br />Mary said, “OK. Seriously, if it were even remotely possible that machines could independently mimic thought that would be significant.”<br /><br />She continued, “Consider Turing’s Machine. Turing held that a mechanical computer is basically a large number of address locations acting as a memory, together with an executive unit that carries out individual operations of a calculation. These operations represent a program. Let’s imagine that I want to use the machine to add two numbers 1 and 2 together. The computing machine would begin with placing a ‘1’ in the first location and a ‘2’ in the second location and then the computer consults a program for how to do addition. The instructions would say gather the numbers from the two locations and perform a summing operation to yield the sum of the two numbers and place the resultant number ‘3’ in the third location. This process could be considered to mimic the operations a human would perform.”<br /><br />John replied solemnly, “Simple rote actions.”<br /><br />Mary added, “Turing’s computer consists of two basic elements: an infinitely long tape ruled off into squares, each capable of being inscribed with the symbol ‘0’ or ‘1,’ and a scanning head that can move forward or back one square at a time reading the symbol on that square, either leaving it alone or writing a new symbol on that square. At any step of the operation, the scanning head can be in one of an infinite number of states. The machine has a pointer that is set at one of the letters ‘A’ ‘B’ ‘C,’ and this letter represents the state of the machine. Part of the program tells the machine how to change the pointer setting, depending on what state the machine is currently in and what symbol is on the square of the tape that the head is currently reading.”<br /><br />John nodded slowly as he visualized the machine.<br /><br />Mary continued, “The action of a Turing machine is determined completely by; (1) the current state of the machine, (2) the symbol in the cell currently being scanned by the head, and (3) a table of transition rules, which serves as the “program” for the machine. If the machine reaches a situation in which there is not exactly one transition rule specified, then the machine halts. While it may take a long tape and many steps to carry out sophisticated calculations, anything at all that can be thought of as following from a set of rules, can be calculated in the step by step fashion.”<br /><br />John said, “It is easy to appreciate that Turing Machine is the foundation of the modern computer.”<br /><br />Mary said, “And that leads us to your earlier question about whether a computing machine can have human-like intelligence.”<br /><br />John said, “In general, I would consider ‘thinking’ to be a complex process that uses concepts and relationships to infer new knowledge. Thinking would involve acts such as memory recall, arithmetic calculations, puzzle solving, and so on. By extension the performance of these acts would indicate ‘intelligence’.” For example, a child who can perform difficult arithmetic calculations quickly would display intelligence. Likewise an individual who has rapid memory recall and who has accumulated sufficient amounts of information to consistently win games such as Scrabble, or Trivial Pursuit, might also be considered to be intelligent.”<br /><br />“Well then,” responded Mary, “Why wouldn’t a computer that could perform the same calculations as that child, but faster and with greater accuracy be considered intelligent. Or consider a computer with substantial memory storage that is able to answer all those Trivial Pursuit questions. Why can’t that computer, be considered intelligent.”<br /><br />John said, “Well human thinking involves complicated interactions within the biological components of the brain. In addition, the processes of communication and learning are also important elements of human intelligence.”<br /><br />Mary replied, “By mentioning intelligent communication you have led us to Turing’s Test for machine intelligence.”<br /><br />John said, “OK, but please, let’s talk about that tomorrow.”<br /><br />___________________________________________________________<br /><br />REFERENCE:<br /><br />[1] <a href="https://www.amazon.com/Thinking-Web-Berners-Lee-G%C3%B6del-Turing/dp/0471768669/ref=sr_1_10?s=books&ie=UTF8&qid=1488313073&sr=1-10&keywords=alesso" target="_blank">Thinking on the Web: Berners-Lee, Gödel and Turing</a>, H. Peter Alesso and Craig F. Smith,<br />Wiley-Interscience , November 24, 2008, ISBN-13: 978-0471768661.<br /><br /><div><br /></div>H Peter Alessohttps://plus.google.com/103789440897695412834noreply@blogger.com0tag:blogger.com,1999:blog-7815548972557022050.post-7036277698866781092013-10-16T14:51:00.003-07:002016-04-27T11:34:33.630-07:00<div style="text-align: center;"><b>Cosmology Spontaneous Symmetry Breaking through the Higgs Mechanism</b></div><br />The quantum uncertainty of spontaneous symmetry breaking during the Big Bang was completely indifferent to the birth of the universe and life on Earth. However, this event produced inquiring minds with many questions, such as "what is mass?"<br /><br />Understanding the origin of mass is one of the greatest challenges of science. Going back to a tiny fraction of a second after the Big Bang, the four forces of nature began to split apart and an inflationary expansion took place that increased the size of the universe exponentially. Under these extremely hot conditions the fundamental particles began to form and travel at the speed of light. A tiny fraction of a second later, these particles acquired mass through the Higgs Mechanism, thereby creating the Standard Model of elementary particles ( leptons, quarks, and bosons). The moment when the Higgs field went from zero to an average nonzero value is known as the "electroweak phase transition." The transition was similar to liquid water turning into ice.<br /><br /><div style="text-align: center;"><b>The Big Bang</b></div><br />Today, we know that the 2.725 degree K cosmic microwave background radiation firmly established the existence Big Bang.<br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://4.bp.blogspot.com/-cUMpKMGMubg/UlR8UAXzXuI/AAAAAAAAAQM/IXMn6tVy_WY/s1600/pic9.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="200" src="https://4.bp.blogspot.com/-cUMpKMGMubg/UlR8UAXzXuI/AAAAAAAAAQM/IXMn6tVy_WY/s1600/pic9.jpg" width="320" /></a></div><br /><br />An instant after the Big Bang, the Universe was more symmetric than it is today and during this period, it underwent several symmetry breaking phase changes in very rapid succession.<br /><br />Ultimately, our ability to find cosmological answers rests on how far back in time we can observe (<a href="http://www.amazon.com/First-Three-Minutes-Modern-Universe/dp/0465024378/ref=sr_1_1?s=books&ie=UTF8&qid=1381273285&sr=1-1&keywords=The+First+Three+Minutes%2C" target="_blank">Weinberg</a><u> </u>[1]). By measuring material compositions and using General Relativity to determine expansion rates, scientists were able to determine how long it took from the Big Bang to the recombination era. When atoms began to form during the recombination era, 380,000 years after the Big Bang, it produced the first time that light was able to travel freely. Now when we look at a star one light-year away, we are actually seeing it as it existed one year ago.<br /><br /><div style="text-align: center;"><b>The Universe</b></div><b><br /></b><b>Time Temp Energy Phenomena</b><br />sec. K GEV<br />_________________________________________________________________<br /><br />10 E-43 10 E32 10 E19 Single force divides into gravity and GUT.<br /><br />10 E-37 10 E29 10 E16 Inflation starts.<br /><br />10 E-35 10 E29 10 E16 Strong force splits from electro-weak force.<br /><br />10 E-33 10 E27 10 E14 Heavy bosons freeze. Matter dominates anti-matter.<br /><br />10 E-9 10 E15 10 E2 Weak interaction splits from electromagnetism.<br /><br />10 E-2 10 E13 1 Color quarks and gluons produce protons, neutrons.<br /><br />100 10 E9 1 E-4 Nucleosynthesis creates Helium and Hydrogen.<br /><br />4 E6 10 E3 1 E-10 Photons decouple from matter.<br />years<br /><br />10 E10 3 1 E-12 Today. Black body radiation.<br />years<br />________________________________________________________________<br /><br />Only 4 to 5% of the universe is composed of ordinary matter. Another 23% is dark matter (exotic non-baryonic matter that weakly interacts with ordinary matter). The 1998 recognition that the universe's expansion is accelerating led to the discovery of dark energy. Dark energy is a property of the vacuum itself (the cosmological constant) characterized by negative pressure (repelling force) causing the expansion of the universe to accelerate.<br /><br />To solve the cosmological flatness, horizon, and monopole problems, <a href="http://www.amazon.com/Inflationary-Universe-Alan-Guth/dp/0201328402/ref=sr_1_1?s=books&ie=UTF8&qid=1381273251&sr=1-1&keywords=The+Inflationary+Universe" target="_blank">Guth [</a>2] proposed an early era of exponential expansion called the Inflation Epoch where a tiny bit of space was stretched into a far larger region.<br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://1.bp.blogspot.com/-HSUhwcjaWR0/UlR8S6-cFsI/AAAAAAAAAQQ/UjmoXgwqu0o/s1600/pic2.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="200" src="https://1.bp.blogspot.com/-HSUhwcjaWR0/UlR8S6-cFsI/AAAAAAAAAQQ/UjmoXgwqu0o/s1600/pic2.jpg" width="320" /></a></div><br />Inflation required a supercooling phase transition that would have started from the state of symmetry of the Grand Unified Theory (GUT)/Standard Model (SM) - before it broke into individual forces.<br /><div class="separator" style="clear: both; text-align: center;"><br /></div><div class="separator" style="clear: both; text-align: center;"><a href="http://1.bp.blogspot.com/-IB-PRIBsOEI/UlR9J1naWWI/AAAAAAAAAQY/DU1kEAASzK4/s1600/bigbang1a.tif" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="247" src="https://1.bp.blogspot.com/-IB-PRIBsOEI/UlR9J1naWWI/AAAAAAAAAQY/DU1kEAASzK4/s1600/bigbang1a.tif" width="320" /></a></div>In 1976, particle physics developed the Standard Model of Quantum Mechanics representing the three forces (electromagnetic, weak and strong) as SU(3)C ⊗ SU(2)L ⊗ U(1)Y with exceptional accuracy. Each of the forces in the Standard Model (SM) is a product of gauge theories with complex charges that mutually interact in a highly symmetric way.<br /><br /><div class="separator" style="clear: both; text-align: left;">The development of GUT was intended to unify electromagnetic, weak and strong interactions of the Standard Model in terms of a single fully unified interaction. While this still left out gravity, it was an excellent approximation to nature.</div><div class="separator" style="clear: both; text-align: left;"><br /></div><div class="separator" style="clear: both; text-align: left;">The SM shows the three forces (weak, strong, and electromagnetic) coupling constants splitting at the point of symmetry breaking. In July 2012, the Higgs Boson (125 Gev) was confirmed.</div><div class="separator" style="clear: both; text-align: left;"><br /></div><div class="separator" style="clear: both; text-align: center;"><a href="http://1.bp.blogspot.com/-L4APpu2phrQ/UlR8TbWhveI/AAAAAAAAAP4/KPFOSqJgHp8/s1600/pic3.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="200" src="https://1.bp.blogspot.com/-L4APpu2phrQ/UlR8TbWhveI/AAAAAAAAAP4/KPFOSqJgHp8/s1600/pic3.jpg" width="320" /></a></div><div class="separator" style="clear: both; text-align: center;"><br /></div><div class="separator" style="clear: both;">GUT theories gave specific reasons for the charge symmetry of electrons and protons. Also super-symmetry gave an intersecting point where all three force’s coupling constants merged at 10 E16 Gev. </div><br />An SU(5) GUT (no longer in favor) could for example break the pattern of SU(5) → SU(3)C ⊗ SU(2)L ⊗ U(1)Y to obtain the standard model (SM). The Higgs mechanism for spontaneously symmetry breaking must include massless Goldstone bosons.<br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://3.bp.blogspot.com/-MmkJR8ofHL8/UlR8TBF-lOI/AAAAAAAAAPo/V3APZ0smfrE/s1600/pic10.jpg" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="200" src="https://3.bp.blogspot.com/-MmkJR8ofHL8/UlR8TBF-lOI/AAAAAAAAAPo/V3APZ0smfrE/s1600/pic10.jpg" width="320" /></a></div><div class="separator" style="clear: both; text-align: center;"><br /></div><b><br /></b>Noteworthy is the fact that not only does inflation smooth out the large scale observables of the universe, it also explains its homogeneity.<br /><b><br /></b><br /><div style="text-align: center;"><b>Spontaneous Symmetry Breaking and the Higgs Mechanism</b> </div><br />The Noether’s theorem correlates conservation laws to symmetries that leave the Lagrangian (L) invariant. <br /><br /><div style="text-align: center;">L = T – V </div><br />The classical path taken by a particle is one that minimizes the action S which is equal to the integral of the Lagrangian over time.<br /><div style="text-align: center;"><br /></div>In quantum theory symmetries can take the form of invariance under a unitary transformation. Local symmetries are very important in relativistic physics because they represent quantities like charge and lepton number that are conserved locally. Local symmetries preserve causality if the Lagrangian is invariant under<br /><br /><div style="text-align: center;">L -> -L<br /><br /><div style="text-align: left;">The Lagrangian for the Standard Model is:</div><div style="text-align: left;"><div class="separator" style="clear: both; text-align: center;"><a href="http://4.bp.blogspot.com/-BpWFm5os1jg/U5OK2eNo6PI/AAAAAAAAAUo/OjYQ5Nh24eI/s1600/pic35.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="180" src="https://4.bp.blogspot.com/-BpWFm5os1jg/U5OK2eNo6PI/AAAAAAAAAUo/OjYQ5Nh24eI/s1600/pic35.png" width="320" /></a></div></div></div>This type of symmetry introduces the concept of spontaneous symmetry breaking. The vacuum state that is the apparent ground state may not be the true ground state. The nonlinear jumping from one state to another state can result from symmetry breaking. For example, if we place a marble on top, right in the center, of an over turned bowl, the symmetry is broken when the marble falls in one direction. The marble may start out semi-stable, but the slightest perturbation, or disturbance, will cause it to roll off. This is because the system is basically unstable.<br /><br />A massless gauge field A undergoing symmetry breaking results in a massive vector field. In electroweak theory, SU(2) x U(1), this gives rise to massive vector bosons W+-,Z. The mechanism for spontaneous symmetry breaking with a gauge field and local U(1) invariance is called the Higgs mechanism, after Peter Higgs, 1964. A spontaneous broken symmetry is one that is present in theory but hidden in the equilibrium state. The symmetry is unbroken when all Higgs fields have a value of zero, but the symmetry is broken when all the Higgs fields acquire a nonzero value.<br /><br />Big Bang cosmology depends on special early conditions leading to GUT predictions that there were two early universe phase transitions. A first order phase transition in a special class of grand unification theory is exemplary of a symmetry breaking potential function V(x).<br /><br />The singularity that broke symmetry and changed one force into four (gravity and SM forces) occurred in stages starting at 10 E16 Gev (10 E-39 seconds) after the Big Bang. The original single force coupling constant changed into four coupling constants that began to diverge in value.<br /><br />The first phase transition was at a high temperature phase transition that broke symmetry and split gravity away from the SM forces - generating a large amount of supercooling that delayed the second phase transition and suppressed monopole production. The supercooling caused the second phase transition to occur at a temperature well below the normal phase transition temperature. (For example, ordinary water can be supercooled to 20 degrees below freezing before it turns to ice.)<br /><br />With the second phase transition postponed until after supercooling, a false vacuum was created. The false vacuum would be the result of twenty four Higgs fields intersecting (representing 12 Leptons, Fermions and their anti-particles, and 12 force particles (photon, +-W, Z, and 8 gluons)). Exactly when the various Higgs field come into existence during the symmetry breaking process is not known. This phase transition was a 1st Order Phase Transition (like boiling water with supercooling) which occurred from 10 E-37 to 10 E-35 seconds. The expansion doubling time was 10 E-37 seconds. The false vacuum produced a neg. pressure repulsing gravitons to make the cosmological constant increase the size of the universe by a factor of 10 E30. The supercooling phase transition that followed caused Inflationary expansion of the universe. Inflationary expansion proceeded at faster than the speed of light. During this time the universe grew from the size of a proton to the size of a baseball in a flash. (Today, the observable physical universe is 93 billion light-years in diameter.)<br /><br /> The matter-antimatter ratio became slightly imbalanced and matter became slightly dominate due to cooling shutting off prior to baryon neucleogenesis reaching equilibrium (10 E78 baryons now in the universe).<br /><br />To help visualize the elements of the Standard Model, it is useful to think of an electron as a matter wave - (a Fermion with spin 1/2) and a photon as an energy wave (a Boson with spin 1). A photon, even though it is massless, feels gravity by E/c^2 and it is the only particle that is an exception to relative motion - always travels at the speed of light, c.<br /><br />General Relativity is an extremely accurate theory for gravity but is classical and does not include quantum effects. As a result, the inability to reconcile it with the Standard Model is due to the appearance of infinity expressions that cannot be renormalized.<br /><br />Three constants play a profound role in physics: (1) the speed of light, c, converts between space and time (ie. the Lorentz transform); (2) Planck's constant, h, converts between frequency and energy (E=hv); and (3) Newton's gravitation constant, G, converts between space-time curvature and energy-density.<br /><br />So then what can we say about mass?<br /><br />Mass is the differential energy left over when disturbed fields attempt to cancel out the disturbance to get to the minimum energy state. For example, The disturbance of quark's color charge can be nullified by an antiquark of opposite charge nearby (or by complementary colors in a proton) however due to quantum effects the cancellation is incomplete and the residue constitutes the resulting mass.<br /><br /><div style="text-align: center;"><b>Elementary Catastrophe Theory </b><b>Modeling of the Big Bang Inflation</b></div><br /><div>A ‘singularity’ is a point where mathematical models are no longer valid ‒ for example: a point divided by zero is undefined. The theory of singularities examines mathematical manifolds in an abstract space to gain a topological representation of the region near a singularity.<br /><br />In the 1960’s Rene’ Thom proposed a nonlinear mathematics approach to describe singularities called Catastrophe Theory. Thom classified the bifurcations based upon their potential function and its derivatives. The morphology of solutions is determined by values of the potential’s parameters. In the special case of gradient vector fields, the mathematics results are called Elementary Catastrophe Theory (ECT) Gilmore [3]. <br /><br />Gradient vector fields are interesting because nearly all trajectories on the behavior surface tend toward a point attractor and the attractor minimizes the potential function V of the system. The parameters determine the locations of the relative minima. A smooth change in the parameters can give rise to a discontinuous jump on the behavior surface. <br /><br />Thom found that under stable conditions there are exactly seven elementary catastrophes if the potential function has no more than two parameters. The most illustrative is the Cusp Catastrophe with a potential of: <br /><br /><div style="text-align: center;">V(x, a, b) = (x^4)/4 + a(x^2)/2 + bx. </div><br />The Cusp has two control variables a and b where x satisfies <br /><br /><div style="text-align: center;">dV/dx = 0, </div><br />shown in figure: <br /><br /><div class="separator" style="clear: both; text-align: center;"><a href="http://2.bp.blogspot.com/-QcEU8uQnAsk/UlSJ74ameeI/AAAAAAAAAQo/HIFt6k9s_lo/s1600/ect1.gif" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" src="https://2.bp.blogspot.com/-QcEU8uQnAsk/UlSJ74ameeI/AAAAAAAAAQo/HIFt6k9s_lo/s1600/ect1.gif" /></a></div>Outside the cusp region there is only one extrema value for x. Inside the cusp, there are two different values of x giving local minima of V(x) for each. Nonlinear variable discontinuous jumps occur at the cusp boundary.<br /><br />Cusp shape in parameter space (a,b) near the catastrophe point shows the locus of fold bifurcations separating the region with two stable solutions from the region with one. <br /><br />But the bifurcation curve loops back on itself, giving a second branch where the alternate solution loses stability and jumps back to the original solution space. You can observe hysteresis loops as the system follows one solution and jumps to the other.<br /><br />Consider if one holds b constant and varies a to follow path 1 or 2. In the symmetrical case b = 0, a pitchfork bifurcation occurs as a is reduced. One stable solution suddenly splitting into two stable solutions and one unstable solution as the physical system passes to a < 0 through the cusp point (0,0) (spontaneous symmetry breaking). Away from the cusp point, there are no sudden changes. <br /><br />(For illustrations of Elementary Catastrophe Theory applications see Alesso [4-5]).<br /><br />Classical phase transition theory is naturally modeled in Elementary Catastrophe Theory ECT. The general family of potential functions depending on state variables, or parameters. The first series of applications of ECT deals with thermodynamics phase transition. Ginzburg Landau second order phase transition relate the critical point of the fluid to the cusp catastrophe. We will show it similarly relates to Big Bang Inflationary Theory universe.<br /><br /><div>We let the state of the physical system be described by the value x that minimizes the potential locally. The physical system is then reduced to a study of equilibrium and stability properties of the potential function V(x,c). The first derivative of the function is equal to zero at equilibrium and the second are shown greater than zero indicating a local stability as well as the critical values of the stable equilibrium branches.<br /><br />In general the potential function the will have only isolated critical points. A phase transition occurs when the point reaches this state of the physical system jumps from one critical branch to another.<br /><br />Phase transitions can occur when the control parameters are varied. The control parameters are assumed to depend upon a single time parameter. A phase transition will occur when the curve crosses and appropriate point. The bifurcation set on which the local minimum are created or destroyed for this curve the transition is of order and if the limits of the derivative goes to zero. Phase transitions in nature usually are zero, first, or second order.<br /><br />The potential function V(x) for the standard GUT with finite-temperature effective scalar potential <a href="http://www.amazon.com/The-Particle-End-Universe-Higgs/dp/0142180300/ref=pd_sim_sbs_b_1" target="_blank">Carroll</a> [6] and <a href="http://prl.aps.org/abstract/PRL/v48/i17/p1220_1" target="_blank">Albrecht</a> [7]:<br /><div class="separator" style="clear: both; text-align: center;"><a href="http://1.bp.blogspot.com/-LfNQUADIvqY/VKn9_A4G7PI/AAAAAAAAAeM/xIj1gjJwgy0/s1600/pic34.png" imageanchor="1" style="margin-left: 1em; margin-right: 1em;"><img border="0" height="180" src="https://1.bp.blogspot.com/-LfNQUADIvqY/VKn9_A4G7PI/AAAAAAAAAeM/xIj1gjJwgy0/s1600/pic34.png" width="320" /></a></div><div class="separator" style="clear: both; text-align: left;">where this potential can be mapped into a Cusp catastrophe by first taking the Taylor series expansion of the natural logarithm terms, then gathering Higgs fields terms according to their exponent and grouping like terms. Then following renormalization rules, create counter terms and eliminate divergences. The result is a Cusp x^4 theory.</div><br /><div style="text-align: center;">V(x, a, b) = (x^4)/4 + a(x^2)/2 + bx.</div><div style="text-align: center;"><br /></div><div style="text-align: center;">where x represents the Higgs field, and</div><div style="text-align: center;"><br /></div><div style="text-align: center;">a and b are combinations of A,B, g. </div><div style="text-align: left;"><br /></div><div style="text-align: left;">The value of the Cusp catastrophe transformation is the clarity of an illustrative image of the non-linear behavior of the phase change and the potential of refining the vacuum value based upon the new parameters. The characteristics of a nonlinear <b>JUMP</b> from one solution space to another within the bifurcation cusp show alternative to quantum tunneling.<br /><br />The S-shaped nonlinear jump of the ECT Cusp is characteristic of the S-shaped jump we find in Inflation Theory .<br /><br /></div></div>The concepts expressed in this blog are further illustrated in the app: <a href="https://play.google.com/store/apps/details?id=com.videosoftwarelab.cosmology" target="_blank">Cosmology App.</a><br /><br /><b>REFERENCES: </b><br /><br />[1] Weinberg, S., "<a href="http://www.amazon.com/First-Three-Minutes-Modern-Universe/dp/0465024378/ref=sr_1_1?s=books&ie=UTF8&qid=1381273285&sr=1-1&keywords=The+First+Three+Minutes%2C">The First Three Minutes,</a>" Basic Books, NY, NY, 1977. <br /><br />[2] Guth, A. H., "<a href="http://www.amazon.com/Inflationary-Universe-Alan-Guth/dp/0201328402/ref=sr_1_1?s=books&ie=UTF8&qid=1381273251&sr=1-1&keywords=The+Inflationary+Universe">The Inflationary Universe</a>," Basic Books, NY, NY, 1997. <br /><br />[3] Gilmore, R., <a href="http://www.amazon.com/Catastrophe-Theory-Scientists-Engineers-Gilmore/dp/0486675394/ref=sr_1_1?ie=UTF8&qid=1381281905&sr=8-1&keywords=catastrophe+theory+for+scientists+and+engineers">Catastrophe Theory for Scientists and Engineers</a>, NY, NY, 1981.<br /><br />[4] Alesso, H. P., “<a href="http://www.sciencedirect.com/science/article/pii/0020746282900415">On the Instabilities of an Externally Loaded Shell</a>” INTERNATIONAL JOURNAL OF NONLINEAR MECHANICS, Vol. 17, No. 2, pp-85-103,1982. <br /><br />[5] Alesso, H. P., and Smith, C. F., “<a href="http://link.springer.com/article/10.1007/BF02731688#page-1">On the Classifying the Deformation Shape of the Liquid Drop Model</a>” IL NUOVO CIMENTO, Vol. 66, pp 272-282, 1981. <br /><br />[6] Carroll, S., <a href="http://www.amazon.com/The-Particle-End-Universe-Higgs/dp/0142180300/ref=pd_sim_sbs_b_1">The Particle at the End of the Universe</a>, NY, NY 2012.<br /><br />[7] Albrecht, A., Steinhardt, P., <a href="http://prl.aps.org/abstract/PRL/v48/i17/p1220_1">Cosmology for Grand Unified Theories with Radiatively</a><br /><a href="http://prl.aps.org/abstract/PRL/v48/i17/p1220_1">Induced Symmetry Breaking</a>, Phys. Rev. Lett. 48, 1220 (1982).<br /><br /></div>H Peter Alessohttps://plus.google.com/103789440897695412834noreply@blogger.com0