Science
Travelling at the speed of lightTravelling at the Speed of light This part courtesy of Dr Karl Kruszelinick
Bubbles in guiness Why do the bubbles in Guinness® go down?
The Principle Of ComplementarityThe Principle Of Complementarity
The Copenhagen InterpretationThe Copenhagen Interpretation
Wave Particle DualityWave Particle Duality
The Relativity of SimultaneityThe Relativity of Simultaneity
E.P.R. ParadoxE.P.R. Paradox
Heisenberg's Uncertainty PrincipleHeisenberg's Uncertainty Principle
The Inverse Square LawThe Inverse Square Law
What's an Isotope?What's an Isotope?
The Principle of Least ActionThe Principle of Least Action
Schrodingers CatSchrödingers Cat
Table Of Elematary ParticlesTable Of Elematary Particles
Traveling at the Speed of LightTraveling at the Speed of Light
A Bit Of Science FictionA Bit Of Science Fiction

The Speed Of Light

If you've ever watched the show Star Trek, you surely must have wished that you could travel in their wonderful starship, the Enterprise. It can accelerate almost instantly from zero to Impulse Speed, which is about one third of the speed of light. At flat chat, the Enterprise can travel at 2,000 times the speed of light. You could certainly get a close look at a lot of the nearby stars if you could travel at such enormous speeds. Can we ever get to the stars in a human lifetime? Well, the Old Physics says "No", but there's a New Physics on the way that says "Maybe".

Light travels awfully fast - around 300,000 kilometres in one second. Einstein threw a spanner in the works with his Special Theory Of Relativity. He said that nothing can travel faster than the speed of light. As you gradually speed up an object it gets heavier.You then have to apply more energy to make this extra mass go faster. By the time you get up to the speed of light, the object that you're trying to push now has an infinite mass, which is ridiculous!

Now with our present-day science, it seems awfully hard to get to even the nearest stars in a reasonable time. There are three stars in the Alpha Centauri complex, about 4.3 light years away. (A light year is the distance that light travels in one year, and it's a really long way. For example, the planet Neptune is only about 4 light hours from the Sun, but it took the Voyager spacecraft 12 years to get there.)

Suppose you wanted to send the American Space Shuttle to the nearest stars. Suppose that you had a pretty good artificial hibernation process for humans, and you were happy for the journey to take 1,000 years. Well, the fuel needed to get it there in that relatively long period of 1,000 years would be much greater than all of the mass of the Universe - in fact, over 10,000 million million million million million million million million million million times greater than all the mass in the entire known Universe!

So if we're going to get to the stars, we're going to need some radically New Physics to get us there. Some, but definitely not all, physicists think that a New Physics is just around the corner.

It's a bit like the situation that existed a century ago. Back then, there were a few problems in the Land Of Science, but they were too hard to solve and so the physicists just ignored them - they swept them under the carpet. One of these problems was the Age of the Sun. The geologists said that the Earth had to be at least 25 million years old, and probably a lot more. The astronomers knew how big the Sun was. But the best fuel that the physicists could come up with was coal. If the Sun was made entirely from coal, the Sun was big enough to burn for only a million years. How could the Sun keep on burning for the extra 24 million years?

Scientists came up with bizarre theories like the Sun getting extra heat energy from millions of comets that were supposedly continually ramming into it at high speed - but basically, they swept the problem under the cosmic carpet. Early in the 20th century, nuclear energy was discovered, and the problem was solved. But the problem had to be solved with a New Physics, not the Old Physics.

Today, at the end of the 20th century, we're in a similar situation. There are quite a few problems that we sweep under the carpet and ignore, simply because we can't solve them. One of these little problems is the Missing Mass Of The Universe - yes, according to the astronomers, 95% of the Universe is missing. Today, many scientists think that because of this and many other problems, we're heading for another revolution in physics. NASA thinks so too. Over the last few years NASA has quietly organised some extraordinary science. One of them has the seemingly-harmless title of "Breakthrough Propulsion Physics Program". What it's really about is coming up with some short-term or near-term, ways of making the breakthroughs that are needed to be able to travel to the stars and back in a normal human life span.

Last time I was talking about how difficult it is to get to the stars using our current technology. For example, look at the amount of fuel you would need to get something like the Space Shuttle to the nearest stars, the Centauri complex, which is about 4 light years away.

If you're prepared to put up with a fairly slow trip lasting about 1,000 years, and used ordinary rocket fuel, the amount of juice needed is squillions of times bigger than the mass of the entire known Universe! If you use a nuclear fission rocket, you would need about a billion super-tankers of propellant (each weighing about a quarter of a million tonnes). If you use a nuclear fusion rocket, you'd need only about 1,000 super-tankers, but with an antimatter rocket, you'd need only about 10 railway tankers. But in half a century, we have made only one tenth of a billionth of a gram of antimatter - which is only enough to get your fully-loaded family wagon about 15 metres down the driveway before it splutters to a high-tech halt!

But there are a few new methods of space travel, based on the science that does exist today.

Back in the 50s, scientists came up with Project Orion, which is basically strapping nuclear bombs to your butt!


They would explode five nuclear weapons every second, which would push on a giant plate at the back of the spaceship, which would be protected from the spaceship by giant springs.

In 1973, the British Interplanetary Society came up with Project Daedalus.


It was similar to Orion, but instead of five nuclear explosions every second, they wanted to have 250 micro-fusion nuclear explosions every second. They reckoned that they would be able to shove a pay load of a hundred tonnes up to about 12% of the speed of light. This would get you to the Centauri complex in about half a century.

Bussard came up with another way, when he invented the Interstellar Ramjet in 1960.


It didn't carry its own fuel - instead, it would scoop up fuel from the space that it travelled through. It had a funnel out the front, about 2,000 kilometres across. This funnel was not made of solid stuff, but of electromagnetic fields that were generated by an enormous magnetic solenoid. Particles would be trapped by the funnel, fed to the fusion reactor, burnt and thrown out of the back of the Bussard Ramjet.

Robert Forward invented Interstellar Laser Sails.


He reckons "use light, rather than rockets". After all, light can exert a very tiny push on an object. If you have a very powerful light shining on a very large object, the "push" gets reasonably big.

His first plan proposed using a sail 1,000 kilometres across, and shining a 10 million gigawatt laser on it. He reckoned he could send a vehicle weighing 1,000 tonnes to the Centauri complex in just 10 years. The catch was that neat little 10 million gigawatt laser. 10 million gigawatts is 10,000 times more than all of the power used on the Earth today!

So Robert Forward came up with a smaller version of the Interstellar Laser Sail. The new sail is a grid of fine wires weighing only 16 grams, but covering a kilometre. This time, the laser is only 10 gigawatts, which is only one hundredth of all the power generated on the Earth today. The penalty is that the trip would take twice as long (20 years), and the payload would not be 1,000 tonnes, but only 4 grams!

So you can see that we are not going to get to the stars and back in a human lifetime with our present technology. We need to make a big jump. After all, we didn't invent photocopiers by trying to make better carbon paper. We didn't invent steamships by improving sails and rigging.

Instead, we have made various breakthroughs in our technology. We went from the sailing ship, to the steamship, to the propellor plane, then the jet plane, and today we have the rocket. We need to make the breakthrough from the rocket to the next stage.


In a relatively short time, we humans have made it from the Stone Age to the Space Age. Even so, our space travel technology is still pretty primitive. Our robot spacecraft have already left the Solar System, but we humans can barely get to the Moon. With our current technology, getting to the stars and back in a human lifetime is impossible. However, a NASA team has identified three breakthroughs that will get us to the stars. The breakthroughs are (first) to get rid of the need for propellant, (second) to travel much faster, and (third) to harness new sources of energy.

In 1996, Marc Mellis of the NASA's Lewis Research Center created the Breakthrough Propulsion Physics Program. This program has a small floating group of scientists from government, university and industry. Since 1996, they've banged their heads together, and worked out what needs to be done. The first breakthrough the scientists are thinking about is getting rid of, or at least dramatically reducing, the need for propellant. After all, when you drive your car down the road, your wheels grip the road, and your engine turns the wheels. But in space, there's nothing to grip onto. That's why rockets (which go forward by tossing stuff out the back) are the only practical way we have of travelling through space - at least, at the moment. But to get the Space Shuttle to the nearby Centauri stars, in a 1,000-year-journey and using conventional fuels, you need to throw away huge amounts of mass - squillions of times greater than the mass of the entire Universe!

So some scientists are trying to reduce the amount of propellant needed, by fusion, or even anti-matter. This would get our space ship moving rapidly, but still well below the speed of light. But, even so, using anti-matter to accelerate a space ship from zero to half the speed of light, and back to zero, would take 700 times the mass of the space ship. There has to be a better way.

So other scientists are trying to get rid of the propellant entirely. They're thinking about how to manipulate gravity or inertia, or how to interact directly between matter and the spacetime fabric of the universe. Here, they may be able to travel faster than the speed of light!

If we imagine that the fabric of spacetime is a sheet of paper, and our spaceship is a pencil, then Einstein tells us that our pencil (a spaceship) can't move faster than the speed of light - but Einstein doesn't mind one bit that our sheet of paper (the spacetime fabric) can move faster than the speed of light. After all, back in the good old days, just after the Big Bang happened, it's claimed that the fabric of spacetime expanded faster than the speed of light.

So Miguel Alcubierre, a physicist at the University of Wales in Cardiff, worked out (theoretically) how to "warp" spacetime, and travel faster than the speed of light. All you had to do was shrink the fabric of spacetime in front of your spaceship, and at the same time expand it behind your space ship.

Unfortunately Mitchell Pfenning and Larry Ford from Tufts University in Medford in Massachusetts actually worked out the numbers, and found that you could warp only a very tiny section of spacetime (much smaller than an atom), and that the energy needed to do this is around 10 billion times all the energy in the entire Universe - hardly worth it!


Another way to get moving faster than the speed of light is to use a "wormhole". Imagine that you have a two-dimensional sheet of paper with a little black dot at the top right hand corner, and another little black dot in the bottom left hand corner. If you wanted to get from one dot to the other, normally you would have to crawl all the way from one corner of the paper to the other. But suppose that you bend the sheet of paper and bring the two dots in contact with each other. If you knew how to manipulate the Third Dimension, and jump out of the paper and back into it again, you could travel from one dot to the other without having to cross the space in between. Maybe a wormhole could be used to do the same thing, but in our four-dimensional spacetime universe.


Notice that with both the "warping of space" method, and the "wormhole" method, we're no longer throwing propellant out of the back of our spaceship.

To have fair-dinkum space travel (zipping to the stars and back in a human lifetime) we need better technology than we have today. Not only do we need to get rid of most, or all, of the propellant, but we also need to be able to travel much faster, and we need to harness new sources of energy. Let's look at travelling faster. If we travel at 100 kilometres per hour, we can get to the nearby Centauri stars in 50 million years. If we travel at the speed that the Apollo Astronauts used to go to the Moon, it's down to only 900,000 years. And if we travel at the speed of the Voyager II spacecraft, our journey time is 80,000 years. The conclusion is obvious - we have to get up to either some decent fraction of the speed of light, or faster than the speed of light.


The third breakthrough needed for real space travel is some sort of fundamentally new way of generating energy. Nuclear fission, nuclear fusion or even anti-matter simply won't give us enough energy.

But there are other energy sources on the horizon. There's a strange thing called Zero Point Energy. Suppose you make a small hollow metal box, with an internal volume of one cubic centimetre - roughly the volume of the tip of your little finger. Suppose that you remove every particle of matter from inside your little box. All you have left is a vacuum. But this vacuum is not nothing - no, it's made up of a strange sea of particles and anti-particles that wink into existence, and almost instantly, wink out again. Their coming and going creates their strange energy called the Zero Point Energy. This energy is huge - up to 1054 joules in each cubic metre. To put that into Plain English, there's enough Zero Point Energy in the vacuum in our tiny metal box to boil all of the oceans on our planet!

Zero Point Energy Diagram

That is the kind of energy level that we need to travel to the stars. And we now know that it's real, not just theory. In 1997, scientists were able to measure, for the first time, the Zero Point Energy pushing two metal plates together.

There is still so much science that we do not know. As far as the physicists are concerned, the natural universe can be explained in terms of the Four Forces. These forces are the Electromagnetic Force (radio, TV, telephones, your Hi-Fi unit, and the like), the Gravity Force (which keeps the planets spinning in their orbits around the Sun, and keeps stuck to the ground), the Weak Nuclear Force (which is responsible for some forms of radioactivity) and the Strong Nuclear Force (which holds the positively charged particles in the core of the atom together).

Forces Diagram

Of these Four Forces, at the end of the 20th century, we humans can manipulate only one - the Electromagnetic Force. We can measure the waves and the particles that make up the Electromagnetic Force, and we can generate and block the Electromagnetic Force. Today we can use it to talk on a mobile phone to somebody on the other side of the planet, almost instantly.

But 400 years ago we could hardly use the Electromagnetic Force at all. The most sophisticated thing that we could do with the Electromagnetic Force was to cut an orange in half, stick a copper nail into one side of the cut orange and an iron nail into the other side of the cut orange, and touch the two different metals to the wet leg of a frog. The leg of the frog would then jump as the electricity went through it - hardly high-tech at all.

Our knowledge and our ability to use and manipulate the remaining Three Forces of the Universe is not even at that primitive stage, where we were with the Electromagnetic Force 400 years ago. We have a long way to go in our knowledge and our understanding - and somewhere along that pathway, we will uncover the secrets which will get us to the stars.

Now some breakthroughs happen really rapidly. There are only three decades from 1911 (when we first began to understand radioactive decay) to 1942 (when the first working nuclear reactor was built under a gymnasium at Chicago University). It was only in 1997 that the Zero Point Energy was actually measured for the first time. Who knows where we'll be in the next three decades?

Why should we go down this pathway towards getting to the stars? Well, one answer is that it's incredibly cheap, as compared to the annual military budget for the world. Another answer is that we are investing in the future for our children, and for the human race. We are one of the few animals that can see the stars, and the stars are our destiny.

Bubbles In Guinness


Most may have noticed that the bubbles in Guinness® do indeed go down. One reason, an incorrect assumption is that they are affected by the electrical currents caused by yeast in beer (you can run a small radio receiver on a couple of glasses of any beer)The correct reason, and a rather simple reason is that the chemical that makes the bubbles is nitrogen, unlike carbon dioxide in other drinks with bubbles that have graduated. This is similar to when you see nitrogen gasses flowing out of a canister, it appears to be in a liquid form and runs down the side of the cannister then disappates.

The Principle of Complementarity


This principle was developed by Neils Bohr. It can be defined as the coexistence of two different and seemingly incompatible descriptions of physical phenomena, but both are needed to have a complete description of a system. An example is wave-particle duality, a phenomenon by which particles in the atomic domain show properties of both particles and waves. This principle is similar to Heisenberg's Uncertainty Principle, and was one area they disagreed on until deciding both principles end up with the same result and therefor were both correct.

The Copenhagen Interpretation


The Copenhagen Interpretation implies the division of the physical world into two parts. An observed system, which can be any atom, subatomic particle or atomic process. The other being the observing system which may consist of experimental apparatus and physicists.
In this case, the object being observed follows quantum physics and the observing system follows classical physics. As a result, the momentum and displacement of an object can never determined with total accuracy as the mere observation of the object changes its behaviour. The best way of describing the position and momentum is in terms of probabilities.

Wave Particle Duality


Prince Louis de Broglie suggested that all matter, even that usually thought of as particles, should display wave like properties. Using Einstein's formula concerning energy and mass (E=mc2) and Plank's formula concerning energy and frequency, de Broglie showed that with any particle there ought to be an associated wave. He also showed that the wavelengths of such particles is inversely related to the particle's momentum and inturn that momentum depends on the particle mass and velocity (P=mv).

The Relativity of Simultaneity


Newton's universe assumed that absolute time was being ticked off by an unseen universal clock, that if it was 12 noon on earth, it was 12 noon everywhere in the universe. This means that events can occur simultaneously, which as Einstein later showed us, causes a paradox.
Einstein pointed out that light tales time to travel and he cited the case of a two lightning bolts striking a train track at the same time. To an observer in the middle but away from the two bolts would see them strike at the same time, however an observer traveling toward bolt A and away from bolt B would see bolt A strike first and vice versa if the direction of travel was opposite. Einstein went on to say there is no privileged observer, in other words all are correct. Hence, two events are simultaneous in one frame of reference but not in two others.

E.P.R. Paradox


Einseint payed close attention to one particular part of the stranger assertions of quantum theory. The path a particle will take from point A to point B in unknowable. As well as this, all paths are posible and each has a probability associated with it.
To reveal what he thought was an inconsistency he worked with Boris Podolsky and Nathan Rosen (the P. and R.). the developed a thought experiment. The basic idea was, to use experimental information about one particle to deduce the properties (such as momentum (p) and position (s)) of a second. they imagined two particles that interact with each other then fly apart, not interacting with anything else until they are observed. Each particle has its own momentum and a position in space. The experimenter (who is only an idea, not a physical entity) is allowed to measure precisely the total momentum of the two particles and the distance between them.
At a later time, the experimenter measures the momentum of one, he should ultimately know the other as the total momentum remains a constant.
However, according to Heisenberg's uncertainty principle, the state of particle B depends on the measurement taken on particle A, which leads to the question How does it know?
Eventually Bohr and co. pointed out a discrepancy, that two distinct measurements would have to be taken, in no one measurement could one measure both the position and the momentum with precision.

Heisenberg's Uncertainty Principle


The realisation at the heart of the Uncertainty Principle arose from theoretical attempts to measure the exact orbit of an electron. in order to detect the electron, it is necessary to illuminate it in some way, that is a beam of short-wave electromagnetic radiation must be focused on the electron. However this radiation behaves like so many particles, and when even one particle impacts with an electron, it alters the path. Therefor the very act of illuminating the electron for observation changes the motion of the electron and the position can therefor not be measured with certainty.
Heisenberg showed that uncertainty isn't just confined to the microworld, but occurs in nature and is unavoidable. Heisenberg showed through mathematics that the product of the uncertainties (the ultimate effect) of say momentum and and position is often far from minute and is always greater than a small physical quantity.
The inverse Square Law
Came as a result of Newton's attempts to find a gravitational constant. The well known story of the falling apple played a major part, actually the apple played a larger part than the story but you know what I mean. Newton postulated that the force that pulled the apple to the ground also pulled the moon to the earth. He calculated that as it fell vertically it was also pulled horizontally enough to keep it in orbit.
He then attempted to quantify the difference in force exerted on the apple to that exerted on the moon. He accomplished this through use of of Kepler's third law of planetary motion. He eventually arrived at the Inverse square law. It states the gravitational forces on an object diminishes by the square of the distance. the apple is 60 times closer to the earths center of gravity, therefor it should experience a force 3600 times stronger than that felt by the moon ( 602 = 3600). Conversly, the moon should curve down through space (follow its orbit) 1/3600 as far as the apple fell in the same amount of time.

An Isotope?


An isotope refers to a group of particles who all share the same position in the periodic table but differ in the number of neutrons they contain.

The Principle of Least Action


this is the principle that got Richard Faynman interested in physics. It states, there is a number - the kinetic energy (KE) minus the potential energy (PE) -the action of which, when averaged out over the path, is least for the true path. This principle applies to light when it is refracted as it travels through a glass prism or other medium denser than air, it always follows the path of least time

Schrödinger's Cat


Schrödinger proposes that a cat, a weak radioactive source and a detector of radio particles is placed in a steel box and sealed. Also in the box is an amount of poison and a hammer connected to a triggering mechanism. If the hammer is released, it will break the container of poison, releasing the gas and killing the cat.
The detector in the box is switched on only once and for only one minute. The radioactive material has a 50% chance of emitting particle during that minute and therefore a 50% chance of not emitting a particle. If a particle is detected the hammer is released and in turn the poison which kills the cat. It is important to note that no one can see into the box.
According to the strict Copenhagen interpretation of quantum physics, after the minute has passed, and before the box is opened we can't speak of the cat as dead or alive because we cannot observe at that moment whether it is dead or alive.
To those who believe that quantum physics apply to the macroworld (the world in which we live, consists of more than one atom or particle) the cat is in an indeterminate state, suspended animation until the cat can be observed and its medical condition assessed.

Table of Elementary Particles


Standard Model
of Particle Physics
FERMIONS
matter constituents
Ordinary Matter
Leptons Quark
Electron
0.511
Electron Neutrino
?
Up
5
Down
8
Exotic matter
Muon
105.7
Muon Neutrino
?
Charm
1,270
Strange
175
Tau
1,784
Tau Neutrino
?
Top
174,000
Bottom
4,250
The estimated mass of each particle is shown in the energy equivalent expressed in millions of electron volts. The highly diverse masses are yet to be explained
Bosons
force carriers
Photons Gluons Intermediate
Vector Bosons
Gravitrons
Antimatter

Matter made of particles with identical mass and spin to particles of ordinary matter, but with opposite charge - for every particle type there is a corresponding antiparticle type.

Travelling at the Speed of Light


This is one of Einstein's Gedankenexperiment or though experiment. Imagine that the speed of light wasn't 300,000 km/h but a modest speed of 40 km/h, and Strictly enforced, meaning there are no penalties (such as infinite mass) for breaking the laws of nature as there are no crimes. This is because nature is self-regulating and merely arranges things so that its prohibitions are imposible to transgress.
As your speed increases, you begin to see around the corners of passing objects. While you are facing rigidly forward, things that are behind you begin to appear in you forward feild of vision. Close to the speed of light, you see the world through an odd point of veiw, ultimately everything is squeezed into a small circular window which stays just ahead of you. From the point of a stationary observer, light reflected of you is reddened as you depart and blued as you arrive. If you travel towards the observer at nearly the speed of light, you will become enveloped in an eerie chromatic radiance: your usually invisible infrared emmission will be shifted to the shorter wavelengths. You become compressed in the direction of motion, your mass increases and time, for you slows down, an effect known as time dilation (it stops when travelling at the speed of light and reverses when travelling faster).

A Bit Of Science Fiction


An idea of mine, I don't think it occurs, but its mind-boggling to think about.
I'll just clear up the concept of parallel universes:
An idea that our sense of being is also duplicated but with alterations of the way we see things, eg. trees may be blue and the sky green.
Imagine that there are a finite amount of parallel universes, each with no conscious awareness of the other. In each different universe, a different set of events have occurred and therefor changed history. Imagine that our destiny is already set out for us but we still have a choice in any decision we may make. Our destiny is set out for us in the sense that there is a parallel universe for every possible decision that every human, animal or plant has had to make. When we make a decision, all we are doing is choosing which parallel universe to travel through.
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