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	<title>Beyond Standard Model Pub</title>
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		<title>Beyond Standard Model Pub</title>
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		<title>Recharge a 9V NiMh battery with a Solar Panel / Constant Current Generator</title>
		<link>http://disipio.wordpress.com/2009/08/11/recharge-a-9v-nimh-battery-with-a-solar-panel-constant-current-generator/</link>
		<comments>http://disipio.wordpress.com/2009/08/11/recharge-a-9v-nimh-battery-with-a-solar-panel-constant-current-generator/#comments</comments>
		<pubDate>Tue, 11 Aug 2009 12:37:29 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Experimentals Pints]]></category>
		<category><![CDATA[Arduino]]></category>
		<category><![CDATA[lm317]]></category>
		<category><![CDATA[NiMh]]></category>
		<category><![CDATA[rechargeable battery]]></category>
		<category><![CDATA[solar energy]]></category>
		<category><![CDATA[Solar Panel]]></category>
		<category><![CDATA[trimmer]]></category>

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		<description><![CDATA[Hi guys,
if you enjoyed the previous post solar-powered Arduino board, you should keep reading this one as well to improve your solar power generator. In fact, with that setup the 9V battery would decay too soon: A NiMh (Nichel &#8211; metal hydroxide) battery must be recharged with a constant current generator, a solar panel alone [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=32&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Hi guys,</p>
<p>if you enjoyed the previous post <a href="http://disipio.wordpress.com/2009/07/17/solar-powered-arduino-board/">solar-powered Arduino board</a>, you should keep reading this one as well to improve your solar power generator. In fact, with that setup the 9V battery would decay too soon: A NiMh (Nichel &#8211; metal hydroxide) battery must be recharged with a constant current generator, a solar panel alone is not.</p>
<p>In order to do so, we can assemble a quite simple circuit using the following components:</p>
<ul>
<li>LM317M or LM317LZ</li>
<li>A 200Ohm trimmer</li>
<li>10Ohm resistance</li>
<li>A LED to check if the current is actually flowing</li>
</ul>
<p>The core of this circuit is the integrated three-terminal adjustable <a title="Linear regulator" href="http://en.wikipedia.org/wiki/Linear_regulator">linear voltage regulator</a> LM317. The &#8216;adj&#8217; pin is a control terminal that is used to adjust the output current. So, the trick is to use a variable resistor (in our case, a trimmer with a small resistance put in front of it) to set the current at a definite value.</p>
<div id="attachment_35" class="wp-caption alignright" style="width: 310px"><img class="size-medium wp-image-35" title="const_curr_gen" src="http://disipio.files.wordpress.com/2009/08/const_curr_gen.png?w=300&#038;h=230" alt="Constant current generator with a LM317" width="300" height="230" /><p class="wp-caption-text">Constant current generator with a LM317</p></div>
<p>With an input DC voltage of max 24V, and the resistances shown in the diagram, one can obtain an output current of:</p>
<p>I_out = 1.2/(10 + R_trim) [A]</p>
<p>This current <em>must</em> be less than 1/10 of the battery output, e.g. for a 750mAh battery the output current must be less than 75mA. As usual, it is customary to insert a capacitor (100uF should be ok) in parallel at the input node to smooth out fast-varying voltages.</p>
<div id="attachment_33" class="wp-caption alignright" style="width: 217px"><img class="size-medium wp-image-33" title="LM317LZ" src="http://disipio.files.wordpress.com/2009/08/lm317lz.gif?w=207&#038;h=133" alt="Pin diagram of a LM317LZ" width="207" height="133" /><p class="wp-caption-text">Pin diagram of a LM317LZ</p></div>
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		<title>Temperature Measurement using Arduino and a Thermistor</title>
		<link>http://disipio.wordpress.com/2009/07/17/temperature-measurement-using-arduino-and-a-thermistor/</link>
		<comments>http://disipio.wordpress.com/2009/07/17/temperature-measurement-using-arduino-and-a-thermistor/#comments</comments>
		<pubDate>Fri, 17 Jul 2009 19:08:12 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Electronics]]></category>
		<category><![CDATA[Experimentals Pints]]></category>
		<category><![CDATA[Hardware]]></category>
		<category><![CDATA[Arduino]]></category>
		<category><![CDATA[monitor]]></category>
		<category><![CDATA[Steinhart-Hart equation]]></category>
		<category><![CDATA[temperature]]></category>
		<category><![CDATA[thermistor]]></category>

		<guid isPermaLink="false">http://disipio.wordpress.com/?p=27</guid>
		<description><![CDATA[Components

Arduino Duemilanove Board, a USB cable and of course a PC/Mac
A 10kOhm thermistor
A 10kOhm resistor
A breadboard wires

Hot topic
It&#8217;g getting hotter and hotter. Is it due to global warming? Who knows, but in the meanwhile we can measure the temperature with our Arduino board and a thermistor. A thermistor is simply a type of resistor whose [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=27&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h2>Components</h2>
<ul>
<li>Arduino Duemilanove Board, a USB cable and of course a PC/Mac</li>
<li>A 10kOhm thermistor</li>
<li>A 10kOhm resistor</li>
<li>A breadboard wires</li>
</ul>
<h2>Hot topic</h2>
<p>It&#8217;g getting hotter and hotter. Is it due to global warming? Who knows, but in the meanwhile we can measure the temperature with our Arduino board and a thermistor. A thermistor is simply a type of resistor whose resistance varies with temperature. If we knew <em>how</em> it varies, we could extract the temperature from the measurement of the resistance (or, better, the voltage across its ends).</p>
<h2>The Steinhart-Hart equation</h2>
<p>In first approximation, the resistance is proportional to the temperature:</p>
<p>R = k(T-T0)</p>
<p>This can work for a narrow temperature range, but we can figure out something more accurate, up to the third order:</p>
<p>1/<em>T</em> = <em>A</em> + <em>B</em> <em>log</em>R + <em>C</em> ( <em>log</em>R )^3</p>
<p>The temperature <em>T</em> is expressed in <em>Kelvin</em>, the resistance <em>R</em> in <em>Ohm</em> and the parameters <em>A</em>, <em>B</em> and <em>C</em> must be determined experimentally, or taken from the datasheet.</p>
<p>If you want to be even more rigorous, you have to include a self-heating effect in the picture. I&#8217;ll give it as a black-box formula:</p>
<p><em>T</em> = <em>T</em>(steinhart-hart) &#8211; <em>V</em>^2 / <em>k</em>*<em>R</em></p>
<p>Where <em>k</em> is the dissipation constant, usually given in units of mW/degree C.</p>
<h2>Setting things up</h2>
<p>In this case the setup is really simple. First of all, connect the Arduino board to the computer (in my case, it&#8217;s a Mac) via the USB cable. Now, connect the GND terminal to the <em>B</em> line of the breadbord (use a <em>black</em> wire), and Arduino&#8217;s +5V output to the <em>A</em> line (use a <em>red</em> wire). Now, put the 10kOhm resistance between the (+) bus and a horizontal line. Now, connect the thermistor between the horizontal line you chose and the (-) bus, the common ground. Last but not least, connect Arduino&#8217;s Analog Input #0 to the horizontal line (X).</p>
<p>(+5V) &#8212;- R &#8212;- X &#8212;- Th &#8212; GND</p>
<h2>Programme Arduino</h2>
<p>Now, the geek part. We have to teach Arduino how to calculate the temperature and give us the answer.</p>
<table border="0">
<tbody>
<tr>
<td>
<blockquote><p>#include &lt;math.h&gt;<br />
#define READING_PIN 0</p>
<p>double R1 = 10000.0; //resistance put in parallel<br />
double V_IN = 5.0;</p>
<p>double A = 1.129148e-3;<br />
double B = 2.34125e-4;<br />
double C = 8.76741e-8;<br />
double K = 9.5; // mW/dec C &#8211; dissipation factor</p>
<p>double SteinhartHart(double R)<br />
{<br />
// calculate temperature<br />
double logR  = log(R);<br />
double logR3 = logR * logR * logR;</p>
<p>return 1.0 / (A + B * logR &#8211; C * logR3 );</p>
<p>}</p>
<p>void setup() {<br />
Serial.begin(9600);<br />
}</p>
<p>void loop() {<br />
double adc_raw = analogRead(READING_PIN);<br />
//Serial.println(adc_raw);<br />
double V =  adc_raw / 1024 * V_IN;<br />
Serial.print(&#8220;V =&#8221;);<br />
Serial.print(V);</p>
<p>//calculate resistance<br />
double R_th = (R1 * V ) / (V_IN &#8211; V);<br />
Serial.print(&#8220;V   R_th = &#8220;);<br />
Serial.print(R_th);</p>
<p>double kelvin = SteinhartHart(R_th) &#8211; V*V/(K * R_th);<br />
double celsius = kelvin &#8211; 273.15;<br />
Serial.print(&#8220;Ohm  &#8212;   T = &#8220;);<br />
Serial.print(celsius);<br />
Serial.print(&#8220;C\n&#8221;);<br />
delay(1000);<br />
}</p></blockquote>
</td>
</tr>
</tbody>
</table>
<p>Compile it and send it to Arduino. Open up the Serial Terminal, and enjoy the output stream.</p>
<h2>Now it&#8217;s up to you</h2>
<p>Probably, the temperature you&#8217;re measuring is quite unconvincing. You have to set up the coefficient according to you thermistor. This will be covered in a following post&#8230;</p>
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		<title>Solar-Powered Arduino Board</title>
		<link>http://disipio.wordpress.com/2009/07/17/solar-powered-arduino-board/</link>
		<comments>http://disipio.wordpress.com/2009/07/17/solar-powered-arduino-board/#comments</comments>
		<pubDate>Fri, 17 Jul 2009 09:55:17 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Electronics]]></category>
		<category><![CDATA[Experimentals Pints]]></category>
		<category><![CDATA[Hardware]]></category>
		<category><![CDATA[Arduino]]></category>
		<category><![CDATA[Green Energy]]></category>
		<category><![CDATA[Renewable Energy]]></category>
		<category><![CDATA[Solar Panel]]></category>

		<guid isPermaLink="false">http://disipio.wordpress.com/?p=17</guid>
		<description><![CDATA[Components

 Arduino Duemilanove Board
 12V Solar Panel
 1N4007 Diode
 25V 100uF Capacitor
 9V Rechargeable Battery and connector
 A breadboard and some wires (suggested red and black)
 A multimeter to measure tensions

1) Green Power
Arduino datasheet suggests us to power it with 6-20V, being aware that the upper limit could be dangerous. It seems that 9V fits [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=17&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h2>Components</h2>
<ul>
<li> Arduino Duemilanove Board</li>
<li> 12V Solar Panel</li>
<li> 1N4007 Diode</li>
<li> 25V 100uF Capacitor</li>
<li> 9V Rechargeable Battery and connector</li>
<li> A breadboard and some wires (suggested red and black)</li>
<li> A multimeter to measure tensions</li>
</ul>
<h2>1) Green Power</h2>
<p>Arduino datasheet suggests us to power it with 6-20V, being aware that the upper limit could be dangerous. It seems that 9V fits well, and it&#8217;s of course very easy to find a 9V battery in a shop. But if we really want to start our own little Green Revolution, we would like to get this electricity from some renewable source, e.g. the Sun, so we need a solar panel. It is a device made up of solar (or photovoltaic) cells, which convert light directly into electricity by the photovoltaic effect.</p>
<p>Now, one problem is that you can be sure that a solar panel will not provide a 9V tension constantly: As everybody know, the Sun walks through the sky during the day, and the energy that reach our panel (even given an ideal 100% conversion efficiency) changes according to the depth of air that the sun rays cross. As a matter of fact, at noon this depth is lower than at dawn or dusk. Moreover, during the night the solar panel is completely useless. So? If you&#8217;re smart enough (or if you google it), the solution is to use the solar panel to charge a 9V rechargeable battery, which in turn powers the Arduino board.</p>
<p>There are many solar panels on the market, so which one fits best with our Arduino board? My rule of thumb is to minimize the cost while maximizing the voltage. You can buy a 12V solar panel for ~20€, probably less. Just remember that we want to charge a 9V battery, so it&#8217;s better if our solar panel provides more than 9V.</p>
<h2>2) Re-charging the battery</h2>
<p>This part is the core of our little experiment. We want to wire up the board so that once the circuit is working fine, we just have to put the Arduino board in parallel to power it up.</p>
<h3>2.1) Basic setup (wrong one)</h3>
<p>In a circuit, electrical current (I) flows from the positive (+) outlet of the battery to the negative (-) one, just like a river flows from the mountain to the sea. Anyway, remember that in this case the charge carriers, the electrons, flows the other way around. Now, if you connect a battery to a load (e.g. a resistance), you basically deplete the battery extracting the accumulated charges. If you want to re-charge the battery, you have to push electrons inside the battery. Thus, the idea is to connect the same-sign sides of the solar panel and the battery, given that the solar panel is more positive (12V) than the battery (9V). This idea is good, but what happens during the night? The battery will send the electrons to the solar panel because now the battery (9V) is &#8220;more positive&#8221; than the panel (ideally 0V). We don&#8217;t really want that&#8230;</p>
<h3>2.2) Basic setup (the right one)</h3>
<p>We have to find a way to prevent this &#8220;night-effect&#8221;: The solution resides in the use of a diode. The most common function of a diode is in fact to allow an electric current in one direction (called the <em>forward biased</em> condition) and to block the current in the opposite direction (the <em>reverse biased</em> condition). Take a look at the 1N4007 diode: at one end (the cathode) there is a gray ring: The current can&#8217;t flow from this side (but you can check with a multimeter that there is a very small voltage anyway of about 0.6V). Now you are free to connect all the devices this way:</p>
<p>solar panel (+) &#8212;&gt; (-) diode (+) &#8211;&gt; (+) battery (-) &#8211;&gt; (-) solar panel</p>
<p>you can convince yourself that during the night the current will not flow from the battery to the solar panel.</p>
<div id="attachment_25" class="wp-caption alignright" style="width: 124px"><img class="size-medium wp-image-25" title="arduino_solar" src="http://disipio.files.wordpress.com/2009/07/arduino_solar1.gif?w=114&#038;h=300" alt="Circuit Schematics" width="114" height="300" /><p class="wp-caption-text">Circuit Schematics</p></div>
<h2>3) Connecting the Arduino board</h2>
<p>Now that we are able to charge the battery with the solar panel, we can link the Arduino board to the whole circuit. The idea is simple: connect the (+)VIN terminal of Arduino to the (+) terminal of the battery/diode, and the (-) GND terminal to the common ground of the battery/solar panel. This way, Arduino will drain current from the &#8220;more positive&#8221; generator between the battery and the solar panel. As I said before, the problem is that the current generated by the panel is not constant. A trick to &#8220;smooth out&#8221; the voltage is to insert a capacitor between the (+) and (-) terminals of Arduino.</p>
<h2>4) A few comments before I leave</h2>
<p>You&#8217;ve probably seen around those fantastic devices that turns solar panels towards the Sun during the day in order to maximize the energy absorption. You could do that as well, but be aware of the fact that 12V are too much for the Arduino analog inputs! Maybe we will talk about that in next post.</p>
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		<title>ATLAS: Last detector connected</title>
		<link>http://disipio.wordpress.com/2008/07/22/atlas-last-detector-connected/</link>
		<comments>http://disipio.wordpress.com/2008/07/22/atlas-last-detector-connected/#comments</comments>
		<pubDate>Tue, 22 Jul 2008 15:00:30 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
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		<category><![CDATA[Physics]]></category>

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		<description><![CDATA[The LUCID detector, which will measure the luminosity of the collisions occurring in the centre of ATLAS, was among the last pieces of the detector to get approval. In fact, the small collaboration, based in Bologna, Italy; Alberta, Canada; Lund, Sweden; and at CERN, didn’t even begin building until February of last year.
LUCID is composed [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=15&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><span style="font-weight:bold;">The LUCID detector, which will measure the luminosity of the collisions occurring in the centre of ATLAS, was among the last pieces of the detector to get approval. In fact, the small collaboration, based in Bologna, Italy; Alberta, Canada; Lund, Sweden; and at CERN, didn’t even begin building until February of last year.</span></p>
<p>LUCID is composed of two detectors that surround the beampipe, one on each side of ATLAS, at 17 metres from the collision point. Its commissioning started June 9th and 16th, when the last two pieces of the beampipe entered the cavern with detectors attached.</p>
<p>Vincent Hedberg, LUCID technical coordinator, and Marco Bruschi, project leader, are quick to downplay the challenges of their commissioning tasks when their detector has 40 channels compared to the millions of channels in other subdetectors. “They’d laugh us out of the house!” says Vincent. However, accessing their detector, 15 metres above the floor, in between the outer endcap muon chambers and endcap toroid magnet, was a feat in itself. “Vincent exaggerates a bit about how easy it is,” says Marco, “since the problem was to fit all the work into a very narrow allotted time, like in a Formula 1 pit stop.”</p>
<p>A portion of the beam shielding block is already in place on the beamline, half a cylinder with a flat top, resembling a bridge between the big muon wheel and the endcap toroid magnet. They built a platform on top of this as a work area. Without access by ladder or stairs, they had to commute to and from LUCID on cherry-picker cranes.</p>
<p>Connecting LUCID to all its services took more time than expected because other activities, such as the beampipe installation, were competing for work space and access to the cherry-pickers. Even so, they successfully connected the copper pipes to carry gas for detecting particles and water for cooling. They also hooked up the cables that will transmit the detector signals as well as the high and low voltage electricity that makes it run.</p>
<p>The bulk of the cabling was completed in the first two weeks, finishing around June 23rd, but a few difficult areas took a bit more time. According to Vincent, in an interview on July 2nd: “We finished with the last problem cable yesterday at nine o’clock.”</p>
<p>Testing began as soon as the first services were connected. As of July 15th, the cooling and gas systems, and high voltage were all working. “The only thing remaining is a broken LED electronics card on one side,” says Marco, “but that we will fix in the next few days. We are now preparing the read-out so that we can be fully prepared to catch the very first collisions from the LHC machine and provide luminosity measurement from day one!”</p>
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		<title>Accumulating evidence for nonstandard leptonic decays of Ds mesons</title>
		<link>http://disipio.wordpress.com/2008/07/15/accumulating-evidence-for-nonstandard-leptonic-decays-of-ds-mesons/</link>
		<comments>http://disipio.wordpress.com/2008/07/15/accumulating-evidence-for-nonstandard-leptonic-decays-of-ds-mesons/#comments</comments>
		<pubDate>Tue, 15 Jul 2008 07:53:19 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Experimentals Pints]]></category>
		<category><![CDATA[fermilab]]></category>
		<category><![CDATA[Add new tag]]></category>
		<category><![CDATA[bsm]]></category>
		<category><![CDATA[flavour physics]]></category>
		<category><![CDATA[higgs]]></category>
		<category><![CDATA[qcd]]></category>
		<category><![CDATA[supersymmetry]]></category>

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		<description><![CDATA[from arXiv:0803.0512v2 [hep-ph]
The measured rate for D_s -&#62; l nu decays, where l is a muon or tau, is larger than the standard model prediction, which relies on lattice QCD, at the 3.8 sigma level. We discuss how robust the theoretical prediction is, and we show that the discrepancy with experiment may be explained by [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=13&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>from <a href="http://arxiv.org/abs/0803.0512v2">arXiv:0803.0512v2</a> [hep-ph]</p>
<blockquote><p>The measured rate for D_s -&gt; l nu decays, where l is a muon or tau, is larger than the standard model prediction, which relies on lattice QCD, at the 3.8 sigma level. We discuss how robust the theoretical prediction is, and we show that the discrepancy with experiment may be explained by a charged Higgs boson or a leptoquark.</p></blockquote>
<p>Dobrescu and Kronfeld show that the tree-level exchange of a spin-0 particle with mass of order 1TeV may account for the discrepancy.</p>
<blockquote><p>[...]  A spin-0 particle of charge +1, H +, appears in models with two or more Higgs doublets. [...] The limits are satisﬁed for M &lt; 500GeV.</p></blockquote>
<blockquote><p>Given that this model has not been previously studied, its 1-loop contributions to ﬂavor-changing processes (such as b → sγ ) → need to be computed before deciding whether some ﬁne tuning is required to evade experimental bounds.</p></blockquote>
<blockquote><p>The charge −1/3 and +2/3 exchanges correspond to leptoquarks [...] These interactions are present, for example, in R-parity violating supersymmetric models.</p></blockquote>
<blockquote><p>A ˜d scalar leptoquark of charge −1/3 may solve the Ds. At the LHC, the ˜d can be strongly produced in pairs, and the ﬁnal states would be ℓ+ℓ j j , where ℓ is a τ or a µ, and j is a c-jet. The current limits on the ˜d mass from similar searches at the Tevatron are around 200 GeV.</p></blockquote>
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		<title>Theory of Everything: A geometric approach to the standard model</title>
		<link>http://disipio.wordpress.com/2007/11/17/theory-of-everything-a-geometric-approach-to-the-standard-model/</link>
		<comments>http://disipio.wordpress.com/2007/11/17/theory-of-everything-a-geometric-approach-to-the-standard-model/#comments</comments>
		<pubDate>Sat, 17 Nov 2007 19:07:20 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Theoretical Pints]]></category>
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		<category><![CDATA[Clifford Algebra]]></category>
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		<category><![CDATA[Garrett Lisi]]></category>
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		<description><![CDATA[ Here is Garrett&#8217;s conclusions paragraph giving a descriptive overview of what he has accomplished:
&#8220;This paper has progressed in small steps to construct a complete picture of gravity and the standard model from the bottom up using basic elements with as few mathematical abstractions as possible. It began and ended with the description of a [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=12&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p> Here is Garrett&#8217;s conclusions paragraph giving a descriptive overview of what he has accomplished:</p>
<p>&#8220;This paper has progressed in small steps to construct a complete picture of gravity and the standard model from the bottom up using basic elements with as few mathematical abstractions as possible. It began and ended with the description of a Clifford algebra as a graded Lie algebra, which became the fiber over a four dimensional base manifold. The connection and curvature of this bundle, along with an appropriately restricted BF action, provided a complete description of General Relativity in terms of Lie algebra valued differential forms, without use of a metric. This “trick” is equivalent to the MacDowell-Mansouri method of getting GR from an so(5) valued connection. Hamiltonian dynamics were discussed, providing a possible connecting point with the canonical approach to quantum gravity. Further tools and mathematical elements were described just before they were needed. The matrix representation of Clifford algebras was developed, as well as how spinor fields fit in with these representations. The relevant BRST method produced spinor fields with gauge operators acting on the left and right. These pieces all came together, forming a complete picture of gravity and the standard model as a single BRST extended connection. If this final picture seems very simple, it has succeeded. As a coherent picture, this work does have weaknesses. Everything takes place purely on the level of “classical” fields – but with an eye towards their use in a QFT via the methods of quantum gravity, which must be applied in a truly complete model. The BRST approach to deriving fermions from gauge symmetries, although a straightforward application of standard techniques, may be hard to swallow. If this method is unpalatable, it is perfectly acceptable to begin instead with the picture of a fundamental fermionic field as a Clifford element with gauge fields acting from the left and right in an appropriate action. The model conjectured at the very end, based on the related u(4) GUT, is yet untested and should be treated with great skepticism until further investigated. In a somewhat ironic twist, after arguing in the beginning for the more natural description of the MM bivector so(5) model in terms of mixed grade Cl1,3 vectors and bivectors, this conjectured model is composed purely of bivector gauge fields. Although the model stands on its own as a straightforward Cl8 fiber bundle construction over four dimensional base, there are many other compatible geometric descriptions. One alternative is to interpret ⇁ ̃A as the connection for a Cartan geometry with Lie group G – with a Lie subgroup, H, formed by the generators of elements other than ⇁e, and the spacetime “base” formed by G/H. Another particularly appealing interpretation is the Kaluza-Klein construction, with four compact dimensions implied by the Higgs vector, φ = −φ ψΓ ψ, and a corresponding translation of the components of ⇁ ̃A into parts of a vielbein including this higher dimensional space. The model may also be extended to encompass more traditional unification schemes, such as using a ten dimensional Clifford algebra in a so(10) GUT. All of these geometric ideas should be developed further in the context of the model described here, as they may provide valuable insights. In conclusion, and in defense of its existence, this work has concentrated on producing a clear and coherent unified picture rather than introducing novel ideas in particular areas. The answer to the question of what here is really “new” is: “as little as possible.” Rather, several standard and non-standard pieces have been brought together to form a unified whole describing the conventional standard model and gravity as simply as possible.&#8221;</p>
<p>see pre-print on <a href="http://arxiv.org/abs/0711.0770" title="http://arxiv.org/abs/0711.0770">http://arxiv.org/abs/0711.0770</a></p>
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		<title>ATLAS helps shed light on the retina</title>
		<link>http://disipio.wordpress.com/2007/11/14/atlas-helps-shed-light-on-the-retina/</link>
		<comments>http://disipio.wordpress.com/2007/11/14/atlas-helps-shed-light-on-the-retina/#comments</comments>
		<pubDate>Wed, 14 Nov 2007 17:58:33 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Experimentals Pints]]></category>
		<category><![CDATA[atlas]]></category>
		<category><![CDATA[cern news]]></category>
		<category><![CDATA[eye]]></category>
		<category><![CDATA[retina]]></category>
		<category><![CDATA[technology transfer]]></category>

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		<description><![CDATA[ Technology developed for high-energy physics has led to the discovery of a retinal cell that eluded biologists for 40 years.                                    [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=11&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><strong><a title="Article4" name="Article4" class="articletitle"></a></strong> <!--HTML--><em><strong>Technology developed for high-energy physics has led to the discovery of a retinal cell that eluded biologists for 40 years. </strong></em><a href="http://bulletin.cern.ch/eng/articles.php?bullno=46/2007&amp;base=art#Article4">                                         </a><br />
<strong></strong><br />
<a href="http://cdsweb.cern.ch/record/1065978"></a><br />
<strong><em>The 512 electrode array, inspired by silicon microstrip detector technology in ATLAS, records the electrical activity of retinal neurones.</em></strong><br />
ATLAS expertise have crossed over to biology enabling the discovery of a retinal cell type that may help humans see motion. The research, carried out by ATLAS collaborators at the University of California, Santa Cruz, and by neurobiologists at the Salk Institute in La Jolla, California, appeared in the 10 October issue of the Journal of Neuroscience and may help open biologists’ eyes to the uses of techniques developed in high-energy physics.</p>
<p>At least 22 different types of primate retinal output cell are known from anatomical studies, but the functions of only a handful of these have been determined. The cells discovered have been called upsilon retinal ganglion cells and the team speculates that they are used to see moving objects and patterns. High-density electrode arrays and associated electronics, inspired by the silicon microstrip detector technology used in ATLAS to track the charged particles coming from collisions, were used to measure their distinct responses to visual images. The upsilons’ large light-sensitive areas and very sharp, rapid, and non-linear responses to changing patterns of light suggested that they were movement detectors.</p>
<p>The retina is the coating at the back of the eye that transforms arriving photons of light into electrical signals that it sends to the brain. The upsilon cells, part of the last layer of cells that send signals along the optic nerve, have been eluding biologists for 40 years. &#8220;These upsilon cells make up maybe a few percent of the output cells of the primate retina, and the chances of finding them are small as they’re so rare,&#8221; explains Alan Litke, senior author of the paper.</p>
<p>The experiment involved focusing a movie onto the retina and comparing this visual input with the electrical output from the retinal cells. Finding the rare cells required a huge number of electrodes within a small space, and so involved a miniaturisation process that was familiar to the CERN collaborators.</p>
<p>A critical part in the miniaturisation was amplifying, filtering, and reading out these electrode signals at high density. A set of multichannel integrated circuits, designed by ATLAS collaborator Wladyslaw Dabrowski and his team from the AGH University of Science and Technology in Krakow, Poland, allows 512 tightly packed electrodes to probe the retina, as opposed to the 61 previously, or just one of early experiments. The increase in electrodes meant a greater number of neurons could be probed at once, allowing researchers to monitor hundreds of cells at once, rather than just one or a few. &#8220;Finding one of these upsilons would be rare, and if you find a cell with unusual properties, you think maybe there’s something wrong, maybe it’s sick,&#8221; explains Alan. &#8220;What you really want to see is a mosaic of cells with similar properties and then you start to believe.&#8221;</p>
<p>ATLAS expertise was also employed in designing the software, which had to be designed from scratch as the amount of data collected was a huge step up for traditional neurobiology, though small compared to LHC standards. Dumitru Petrusca, one of the main software developers of the ATLANTIS event display program for ATLAS, undertook this task and was the first author of the upsilon paper.</p>
<p>Thanks to this software and technology, the neurobiologists, in collaboration with the physicists, are able to look at the bigger picture to gain a more complete idea of the vision process. &#8220;Traditionally, neurobiologists looked at just one neuron at a time. But to understand how a neural system, such as the retina or the brain, really works, we need to see the patterns of electrical activity generated by many neurons. Just like in ATLAS it would be near impossible to get at the underlying physics by looking at just one particle per event. You want to see the whole event because then you can say, for instance, there are two jets of particles with this total mass, and that’s the decay of the Higgs.&#8221;</p>
<p>For Alan, the processing and encoding of information is just one part of the puzzle of how the retina works. Another is how it gets wired up: &#8220;It’s a three-dimensional wiring problem. The upsilon cell connects to all these other cells and layers and we want to find out how the cells know where to go, how they connect to one another and make the right connection. It would be like the thousands of cables in ATLAS growing out of the pit and finding their way to the right control room, rack of electronics, crate and finally module, all on their own.&#8221;</p>
<p>Related projects include retinal prosthesis: using electrode array technology to electrically stimulate retinal output cells, using input from a video camera, to bypass the degraded photoreceptors in patients with macular degeneration. Small arrays that give some basic vision are already being trialled in six blind patients by Mark Humayun and his team at the University of Southern California.</p>
<p>This result may open up further opportunities for transferring expertise and techniques from high-energy physics to biology. &#8220;It’s not just the upsilon, it’s the combination of the technique and the discovery,&#8221; says Alan. &#8220;Biologists are rarely aware of the technologies developed for high energy physics, so one way to bring this to the attention of the neurobiological community is to have an interesting neurobiological result. Now we’ll see where it takes us.&#8221;</p>
<p><strong>Ideas that spring from the meeting of minds</strong></p>
<p>Progress is not often a scientific activity alone, but is helped on its way by chance meetings and cafeteria conversations. Whilst working at SLAC and watching his children learn to walk, talk and develop, Alan Litke wondered how silicon microstrip detector technology could be applied to understanding the fascinating depths of the brain, but without a scientist’s &#8220;six degrees of Kevin Bacon&#8221; the research wouldn’t have happened. &#8220;I had some pretty crazy ideas, but in the end one of the post-docs in my group had a neighbour who was a neurobiologist at Stanford and who was working in the lab of someone who was one of the world experts on the retina. So I started to help in any way I could.&#8221; And he hasn’t looked back. In the past some of the best science has comes from collaborations with those outside a tradition and this one has already made great steps in unravelling the mysteries of the retina.</p>
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		<title>Doubly Special Relativity</title>
		<link>http://disipio.wordpress.com/2007/11/05/double-special-relativity/</link>
		<comments>http://disipio.wordpress.com/2007/11/05/double-special-relativity/#comments</comments>
		<pubDate>Mon, 05 Nov 2007 11:50:56 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Theoretical Pints]]></category>
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Doubly-special relativity — also called deformed special relativity or, by some, extra-special relativity — is a modified theory of special relativity in which there is not only an observer-independent maximum velocity (the speed of light), but an observer-independent minimum length (the Plank length).
This was first proposed in a paper by Giovanni Amelino-Camelia, though it is [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=10&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading"></h1>
<p style="position:absolute;z-index:100;right:100px;top:0;" class="metadata">&nbsp;</p>
<p><!-- start content --><strong>Doubly-special relativity</strong> — also called <strong>deformed special relativity</strong> or, by some, <strong>extra-special relativity</strong> — is a modified theory of <a href="http://en.wikipedia.org/wiki/Special_relativity" title="Special relativity">special relativity</a> in which there is not only an observer-independent maximum velocity (the <a href="http://en.wikipedia.org/wiki/Speed_of_light" title="Speed of light">speed of light</a>), but an observer-independent minimum length (the <a href="http://en.wikipedia.org/wiki/Plank_length" title="Plank length">Plank length</a>).</p>
<p>This was first proposed in a paper by <a href="http://en.wikipedia.org/wiki/Giovanni_Amelino-Camelia" title="Giovanni Amelino-Camelia">Giovanni Amelino-Camelia</a>, though it is at least implicit in a paper by <a href="http://en.wikipedia.org/w/index.php?title=Paul_Merriam&amp;action=edit" class="new" title="Paul Merriam">Paul Merriam</a>. An alternate approach to doubly-special relativity theory, inspired by that of Amelino-Camelia, was proposed later by <a href="http://en.wikipedia.org/wiki/Jo%C3%A3o_Magueijo" title="João Magueijo">João Magueijo</a> and <a href="http://en.wikipedia.org/wiki/Lee_Smolin" title="Lee Smolin">Lee Smolin</a>. There exist proposals that these theories may be related to <a href="http://en.wikipedia.org/wiki/Loop_quantum_gravity" title="Loop quantum gravity">loop quantum gravity</a>.</p>
<p>One of the motivations for this work is the observation of high-energy <a href="http://en.wikipedia.org/wiki/Cosmic_ray" title="Cosmic ray">cosmic rays</a> that appear to violate the <a href="http://en.wikipedia.org/wiki/Greisen-Zatsepin-Kuzmin_limit" title="Greisen-Zatsepin-Kuzmin limit">Greisen-Zatsepin-Kuzmin limit</a>: the so-called <a href="http://en.wikipedia.org/wiki/Ultra-high-energy_cosmic_ray" title="Ultra-high-energy cosmic ray">Oh-My-God particles</a>.</p>
<p>The theory is highly speculative as of first publishing in <a href="http://en.wikipedia.org/wiki/2002" title="2002">2002</a>. The theory is built using a well-established approach in theoretical physics named <a href="http://en.wikipedia.org/wiki/Invariant_%28physics%29" title="Invariant (physics)">invariance under transformation</a>, which is colloquially (even in science) called <a href="http://en.wikipedia.org/wiki/Relativistic" title="Relativistic">relativistic</a>. Nevertheless the theory is not considered a promising approach by a majority of members of the <a href="http://en.wikipedia.org/wiki/High-energy_physics" title="High-energy physics">high-energy physics</a> community.</p>
<p>DSR is based upon a generalization of symmetry to <a href="http://en.wikipedia.org/wiki/Quantum_group" title="Quantum group">quantum groups</a>. The <a href="http://en.wikipedia.org/wiki/Poincar%C3%A9_symmetry" title="Poincaré symmetry">Poincaré symmetry</a> of ordinary <a href="http://en.wikipedia.org/wiki/Special_relativity" title="Special relativity">special relativity</a> is deformed into some <a href="http://en.wikipedia.org/wiki/Noncommutative" title="Noncommutative">noncommutative</a> <a href="http://en.wikipedia.org/wiki/Symmetry" title="Symmetry">symmetry</a> and <a href="http://en.wikipedia.org/wiki/Minkowski_space" title="Minkowski space">Minkowski space</a> is deformed into some <a href="http://en.wikipedia.org/wiki/Noncommutative_space" title="Noncommutative space">noncommutative space</a>. This theory is not a violation of Poincaré symmetry as much as a deformation of it and this symmetry is exact. This deformation is scale dependent in the sense that the deformation is huge at the Planck scale but negligible at much larger length scales. Many models which are significantly Lorentz violating at the Planck scale are also significantly Lorentz violating in the infrared limit because of nasty radiative corrections. Without any exact Lorentz symmetry to protect them, such Lorentz violating terms will be generated with abandon by quantum corrections. However, DSR models do not succumb to this difficulty since the deformed symmetry is exact and will protect the theory from unwanted radiative corrections — assuming the absence of <a href="http://en.wikipedia.org/wiki/Quantum_anomalies" title="Quantum anomalies">quantum anomalies</a>.</p>
<p>Jafari and Shariati have constructed <a href="http://en.wikipedia.org/wiki/Canonical_transformation" title="Canonical transformation">canonical transformations</a> that relate both the doubly-special relativity theories of Amelino-Camelia and of Magueijo and Smolin to ordinary special relativity. They claim that doubly-special relativity is therefore only a complicated set of coordinates for an old and simple theory. However, all theories are related to free theories by canonical transformations. Therefore supporters of doubly-special relativity may claim that while it is equivalent to ordinary relativity, the momentum and energy coordinates of doubly-special relativity are those that appear in the usual form of the <a href="http://en.wikipedia.org/wiki/Standard_model" title="Standard model">standard model</a> interactions. This implies that ordinary special relativity and doubly-special relativity make distinct physical predictions in high energy processes, and in particular the derivation of the <a href="http://en.wikipedia.org/wiki/Greisen-Zatsepin-Kuzmin_limit" title="Greisen-Zatsepin-Kuzmin limit">Greisen-Zatsepin-Kuzmin limit</a> is not valid if one asserts that <a href="http://en.wikipedia.org/wiki/Quantum_electrodynamics" title="Quantum electrodynamics">quantum electrodynamics</a> takes its usual Maxwell form only in the coordinate systems of doubly-special relativity.</p>
<p><a title="Literature" name="Literature" id="Literature"></a></p>
<h2><span class="editsection"></span><span class="mw-headline">Literature</span></h2>
<ul>
<li>Fabio Cardone<a href="http://cardonefabio.awardspace.com/" class="external autonumber" title="http://cardonefabio.awardspace.com" rel="nofollow">[1]</a>, Roberto Mignani , <em>Energy and Geometry: An Introduction to Deformed Special Relativity</em>, World Scientific 2004, <a href="http://en.wikipedia.org/w/index.php?title=Special:Booksources&amp;isbn=9812387285" class="internal">ISBN 981-238-728-5</a></li>
</ul>
<p><a title="External_references" name="External_references" id="External_references"></a></p>
<h2><span class="editsection"></span><span class="mw-headline">External references</span></h2>
<ul>
<li>Giovanni Amelino-Camelia, &#8220;Doubly-Special Relativity: First Results and Key Open Problems.&#8221; <em>Int. J. Mod. Phys.</em> D11 (2002) 1643. Online copy at <a href="http://arxiv.org/abs/gr-qc/0210063" class="external free" title="http://arxiv.org/abs/gr-qc/0210063" rel="nofollow">http://arxiv.org/abs/gr-qc/0210063</a></li>
<li>Giovanni Amelino-Camelia, <em>Doubly-Special Relativity.&#8217;</em> <a href="http://lanl.arxiv.org/abs/gr-qc/0207049" class="external free" title="http://lanl.arxiv.org/abs/gr-qc/0207049" rel="nofollow">http://lanl.arxiv.org/abs/gr-qc/0207049</a>, a non-technical review</li>
<li>Nosratollah Jafari, Ahmad Shariati, <em>Doubly Special Relativity: A New Relativity or Not?</em> <a href="http://arxiv.org/abs/gr-qc/0602075" class="external free" title="http://arxiv.org/abs/gr-qc/0602075" rel="nofollow">http://arxiv.org/abs/gr-qc/0602075</a></li>
</ul>
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		<title>[CERN] A word from the DG: LHC commissionning  enters the home straight</title>
		<link>http://disipio.wordpress.com/2007/10/25/cern-a-word-from-the-dg-lhc-commissionning-%e2%80%a8enters-the-home-straight/</link>
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		<pubDate>Thu, 25 Oct 2007 14:35:27 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
				<category><![CDATA[Experimentals Pints]]></category>
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		<category><![CDATA[cern news]]></category>

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		<description><![CDATA[A word from the DG: LHC commissionning  enters the home straight

&#160;
In an age of blogs there are seemingly no secrets, so by the time Lyn Evans gave his talk on the status of LHC commissioning on 13 September, everyone seemed to know about plug-in modules, beam position monitors and transmitters embedded in ping-pong balls. All [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=9&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><strong><a name="Article2" class="articletitle"></a>A word from the DG: LHC commissionning  enters the home straight</strong></p>
<blockquote class="sessionbody"><p><!--HTML--></p>
<p align="justify">&nbsp;</p>
<p>In an age of blogs there are seemingly no secrets, so by the time Lyn Evans gave his talk on the status of LHC commissioning on 13 September, everyone seemed to know about plug-in modules, beam position monitors and transmitters embedded in ping-pong balls. All the on-line speculation made for interesting reading, and is a clear sign of the growing interest there is in CERN as we approach LHC start-up. We are now entering the final phase of commissioning, and things are going well given the unprecedented complexity of the task in hand.</p>
<p>Following the cool-down, powering and warm-up of Sector 7-8 earlier this year, we have learned a great deal about what it means to commission the LHC. There have inevitably been hitches, including the plug-in modules, or PIMs. When the LHC is cooled down, each sector shrinks by about 10 metres in length, and this has to be absorbed by bellows between components and a system of sliding copper fingers (PIM) that ensure electrical connectivity around the ring. When warming up Sector 7-8, a small number of fingers buckled as the machine expanded and are being repaired. The problem is understood, and concerns only a small percentage of the PIMs. To identify precisely where the problem occurs, an ingenious system involving blowing an object like a ping-pong ball with a 40 MHz transmitter (the frequency of the beam bunches seen by the position monitors) along the beam pipe has been devised.</p>
<p>Lessons learned from Sector 7-8 are being put into practice in other sectors. A second sector has been rapidly cooled to 80 degrees above absolute zero, a third is undergoing pressure tests, and testing of the remaining five sectors will now start at the rate of one every two weeks. In the sectors currently under test, vacuum leaks have been isolated and are also being repaired.</p>
<p>Meanwhile, the repair of the LHC’s inner triplet magnets is complete. A team from CERN, Fermilab, KEK and the Lawrence Berkeley National Laboratory has successfully completed the repairs. So far, three of the eight triplets have been installed and successfully pressure-tested in the tunnel. The remaining triplets are in the process of installation and pressure testing.</p>
<p>All of this is business as usual when bringing a new particle accelerator on-line. There are inevitably hurdles to be overcome, but so far there have been no show stoppers. We can all look forward to the LHC producing its first physics in 2008.</p>
<p><em>Robert Aymar</em></p></blockquote>
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		<title>Supersymmetry for the masses</title>
		<link>http://disipio.wordpress.com/2007/10/09/supersymmetry-for-the-masses/</link>
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		<pubDate>Tue, 09 Oct 2007 10:09:07 +0000</pubDate>
		<dc:creator>Riccardo Di Sipio</dc:creator>
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		<description><![CDATA[Introduction
Since the times of the Ancient Greece, Natural Philosophers (they had several names, from time to time) have often asked themselves what the &#8220;world&#8221; is really made of. The first answer was &#8220;atoms&#8221; (&#8220;impossible to divide further&#8221;), and, as today, we still can&#8217;t prove if it&#8217;s true or not. Nowadays, this word has the different [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=disipio.wordpress.com&blog=927783&post=8&subd=disipio&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><strong>Introduction</strong><br />
Since the times of the Ancient Greece, Natural Philosophers (they had several names, from time to time) have often asked themselves what the &#8220;world&#8221; is really made of. The first answer was &#8220;atoms&#8221; (&#8220;impossible to divide further&#8221;), and, as today, we still can&#8217;t prove if it&#8217;s true or not. Nowadays, this word has the different meaning of &#8220;minimal entities of chemistry&#8221;, but chemical atoms are not impossibile to divide since now we know they are made of more fundamental constituents called quarks and electrons.</p>
<p>The best description we (I mean the western Natural Philosophers) have found so far is called &#8220;Standard Model&#8221;, and it&#8217;s based on a more deeper cookbook called &#8220;quantum field theory&#8221;. While nobody has yed proved the latter to be wrong, we know the former to be an incomplete description of the world we live in. For some aspects it&#8217;s even flawed, since it predicts that some elusive objects called neutrinos are weightless, but experiments show they are not. This is not bad news: after all, it suggests that there&#8217;s still a lot of work to do. In physics, greek atoms are called elementary particles.</p>
<p><strong>Relativistic Quantum Field Theory</strong><br />
At the beginning of the XXth century, physicists (mainly Planck, Einstein, Heisemberg, Schroedinger) discovered that our world, when considered at very short length, behaves differently from, let me say, at our &#8220;scale of distances&#8221;. They discovered the &#8220;quantum mechanics&#8221;. A famous physicist once noticed that we are all well accustomed to quantization: for example, when we order a beer at the pub, we buy it in pints, even if the beer flows continuously from the cask.<br />
Basically, in the atomic world, energy is sold in glasses of different size. But always in glasses.</p>
<p>What does it mean the word &#8220;field&#8221; in the name of this theory? A field is an entity defined everywhere in the space. For example, when we watch forecasts on tv, we actually observe the &#8220;temperature field&#8221; or the &#8220;wind field&#8221;. We define the temperature to be a &#8220;scalar&#8221; (it can be measured with some kind of scaler), while the wind is a &#8220;vector&#8221; (wind has a magnitude and a direction, like &#8220;from south to west&#8221;: this makes a vector). There can be more uncommon type of fields, and they turn out to be very important for our discussion.<br />
Anyway, the whole thing is that  when you mix up &#8220;quantum&#8221; and &#8220;field&#8221; you discover that the particles are fields of waves. When two bodies exchange energy they do this through waves of the field that we recognize as particles.</p>
<p>Let&#8217;s talk about the word &#8220;relativistic&#8221;. Again, at the dawn of the previous century, Albert Einstein proved that the laws describing electrical and magnetic phenomena imply that space and time must be considered in a particular combination as a single entity (the so-called spacetime). This is inavoidable if we believe that everyone, independently of their place and speed (and possibily religious beliefs).<br />
What followed from this discover has been an incredible breakthrough in Natural Philosophy: the speed of light in vacuum is the fastest speed that everything can reach, and it is the same for everyone, independently of their place and speed. Experiments boldly confirmed this theory. It&#8217;s so difficult to understand how it can be, that I suggest you to accept it as a fact, until it will be proven false. But don&#8217;t get crazy, nobody can understand it: We can only describe this weird thing with math.</p>
<p>Now, relativity let us toss and turn object in 4 dimensions: time and space. When we rotate something in space we call this operation&#8230;well, rotation. When we rotate something in 2 spatial dimensions and time we obtain a &#8220;Lorentz boost&#8221;. It has no obvious meaning in everyday life, but scientists discovered that it can explain a property of particles called &#8220;spin&#8221;: when placed in a magnetic field, electrically charged particles behave like they&#8217;re rotating, but they are not.<br />
Particles can be classified according to the numerical value of their spin, which is always the same for each one. In fact, if you put together relativity and quantum mechanics, you discover that the spin is quantized (&#8220;sold in glasses&#8221;). If you measure the spin in a unit called &#8220;Planck constant&#8221;, it turns out that all the particles can have a spin that is either an integer multiple of this unit (let&#8217;s say 1, 2, 3&#8230;), or a semi-integer multiple (1/2, 3/2&#8230;). The first kind is called &#8220;boson&#8221; after the indian physicist Satyendra Bose, while the second is called &#8220;fermion&#8221; after Enrico Fermi. From calculations, it turns out that spin-0 particles are scalars, spin-N/2 are &#8220;spinors&#8221;, spin-1 are &#8220;vector bosons&#8221;  and spin-2 are &#8220;tensors&#8221;. Don&#8217;t be afraid of spinors and tensors: you don&#8217;t need to know exactly what they are.</p>
<p><strong>The Standard Model</strong><br />
Ok, now we have all the ingredients. What can we do with them?  Let&#8217;s assign a kind of field for each particle discovered so far.<br />
Experiments show that bosons are responsible of forces (like electromagnetism and nuclear reactions), while fermions are the &#8220;building blocks&#8221; of the world called quarks and leptons, let&#8217;s say, they form atoms, molecules, human beings etc. It is still experimentally unproven, but very likely, that gravitation is due to a spin-2 boson called &#8220;graviton&#8221;, but remember: gravitation is not a part of the Standard Model!</p>
<p>Now, a main issue is: &#8220;how come that particles have mass?&#8221;. Despite the fact that we can fancy several ways to get this results, the more simple and elegant is through the so-called &#8220;Higgs mechanism&#8221;, after the physicist who proposed it. Basically, Standard Model states that there is a field (a scalar one) that interacts only with some particles, but not all. Heavy particles interact very strongly with the Higgs field, while photons do not at all (light is &#8220;weightless&#8221;). It act, more or less, like putting a sheet of paper on a wet table top: paper absorbs water and it gets heavy. If you try doing the same with a plastic card it doesn&#8217;t work.</p>
<p>The problem is that nobody has ever <em>officially</em> seen a Higgs particle (some rumors from Fermilab). So far. Moreover, this theory doesn&#8217;t predicts the value of the masses, and other parameters.</p>
<p>So we&#8217;ve got:</p>
<ul>
<li>  Spin-0: scalar particles (Higgs)</li>
<li>  Spin-N/2: &#8220;spinor&#8221; fields (quarks, electrons, neutrinos..)</li>
<li>  Spin-1: vector boson fields (electroweak interaction)</li>
</ul>
<p>Is this all?</p>
<p><strong>Beyond the Standard Model: Merits and flaws</strong></p>
<p>Despite some rumors, the SM is a magnificent theory. Of course, it&#8217;s not perfect. For example, a lot of parameters are put in &#8220;by hand&#8221; (like the value of the masses, which is, IMHO, the biggest flaw), but it let us explain why the sun is so hot and so long-lived, and a lot of other important stuffs. Moreover, gravity is not included. Nobody tells us that we will eventually find a &#8220;Theory of everything&#8221;, but it is so attracting that it&#8217;s worth trying.</p>
<p>In the past 30 years (or more) a lot of effort has been made in this direction. Einstein has tried, too, but without much success. Actually, Grand Unification is the Tree of Life of particle physics, and it seems to have a large number of limbs. But only one trunk. Supersymmetry is one branch that is very promising.</p>
<p>You can see SUSY from different points of view, anyway, it states that fermions and bosons are two faces of the same coin, if you knew how to see it properly. Of course, in our world, they are not the same thing: fermions are the bricks of the Cosmos, and bosons act like glue. So what has SUSY to do with out world?</p>
<p>In Field Theory there&#8217;s an important operation called &#8220;commutation&#8221;. Commutation is made of &#8220;operators&#8221;, which are mathematical objects describing some kind of transformation.</p>
<p>The point is that if you apply SUSY twice and then come back to the initial state, you get a shift in one direction.</p>
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