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Nuclear Physics

Most commonly known for its applications in nuclear energy and nuclear weapons, Nuclear Physics also has applications in medicine and archaeology. This category is for questions about the branch of physics that deals with the study of the forces, reactions, and internal structures of atomic nuclei, Nuclear Physics.

3,164 Questions

What is the half life of Abraxane?

The half life of Abraxane, a chemotherapy medication, is around 22 hours. This means it takes about 4-5 days for the drug to be eliminated from the body after the last dose.

What are beta rays?

Beta radiation is the name of the particle released in a type of nuclear decay called (naturally) beta decay. The radiation, the particle, is either a high energy electron or a high energy anti-electron or positron. These little guys come out of the decay event like a bullet from a gun, but don't have a lot of penetrating power. They can be stopped by a sheet of aluminum foil.

Hit the links below for further information, particularly the one on what beta decay is. As an aside, there is an anti-neutrino or neutrino (respectively) released in the decay events also, but these little dudes don't interact strongly with other particles and just pass right through.

Who was Rutherford?

He was a chemist and physicist who became known as the father of nuclear physics.

He discovered the concept of radioactive half life.

He demonstrated the nuclear nature of atoms.

He transmuted one element to another in Cambridge where nitrogen convert to oxygen trough nuclear reaction.

He theorized about neutrons.

Why is energy released when the nuclear reactions take place?

In general, energy is released when nuclear reactions take place because atomic nuclei are moving into lower energy states. To move to a lower energy state, energy must be released, as you might have guessed. And many nuclear fission and fusion reactions accomplish this. Note that there are some nuclear reactions that do not release energy, but actually require it. One example is the fusion of lighter elements into the heavy elements beyond iron. When stars, which are giant nuclear fusion engines, are young, the energy that is released in the fusion processes promotes continued fusion. But at some point, they run out of fuel. Nuclear fusion that creates trans-iron elements requires that energy be put into the reaction, and that's where supernova event has value. All elements heavier than iron are created in a supernova.

You set up a pulley to help you lift something you anchor the rope at one end and arrange a moveable pulley to achieve a mechanical advantage of 2 by the time you have lifted the object 5m off the gro?

you set up a pulley to help you lift something you anchor the rope at one end and arrange a moveable pulley to achieve a mechanical advantage of 2 by the time you have lifted the object 5m off the ground how much rope have you pulled through the pulley

answer is (10m)

How does a quark produce hadron jets when hadrons are made up of quarks?

When high-energy collisions occur in particle accelerators, the energy is converted into new particles through processes like quark-quark interactions. These interactions can result in the creation of high-energy quarks that then hadronize, forming collimated sprays of hadrons known as jets. This is due to the strong force that binds quarks together, allowing them to form color-neutral hadrons rather than existing as free quarks.

What is the diameter of nucleus?

The diameter of a nucleus can vary depending on the type of cell it belongs to. On average, the diameter of a cell nucleus is about 5-10 micrometers. However, in some larger cells or under certain conditions, the nucleus can be larger.

What is the simple formula in calculating the half life of protactinium-234?

The formula for calculating the half-life of a radioactive substance is t1/2 = (ln(2) / λ), where t1/2 is the half-life, ln is the natural logarithm, and λ is the decay constant. For protactinium-234, the decay constant (λ) is 2.53 x 10^-6 per year. Plug in this value into the formula to calculate the half-life of protactinium-234.

Why does radioactive decay occur?

Radioactive pollution is something unwanted going into the environment. It can be very dangerous because radiation can cause cancer.

Whats the smallest particle of an atom?

Smallest particles in an atom are named as subatomic particles. They have been categorized into four. They are photons, leptons, mesons and baryons.

Baryons are further classified into nucleon and hyperon.

Photon is the smallest one whose rest mass is zero. Though it does not have mass, it has momentum. The energy content of a photon is mainly decided by the frequency of the radiation. So E = h v. v (nu) is the frequency

Leptons are some how heavier but lighter than mesons. Electrons, positrons, neutrino, muons all come under this category

Mesons have different types such as pi meson, eta meson, k meson etc

Baryons have nucleons (protons and neutrons) and hyperons. (much heavier than nucleon)

Apart from these there are strange particles and these are being studied and science now and then comes across new discoveries of subatomic particles. So far more than 100 particles have been discovered.

A device in which droplets of alcohol condenses around a radioactive substance causing it to leave a trail is called?

The device you are referring to is called a cloud chamber. It is used to observe the paths of charged particles, such as those emitted from radioactive decay, as they ionize the alcohol vapor in the chamber, producing visible tracks.

Why do heavy atoms tend to undergo fission of fusion?

It has something to do with the binding energy per nucleon in the nucleus, but mostly has to do with the range of the residual strong force versus the electromagnetic force. Let's check it out. The dynamics of the nucleus are modestly straightforward and can, for the most part, be reduced to two interactions. Setting aside the intricacies of quantum chromodynamics (QCD), we first consider the protons pushing against each other via the coulomb force, an expression of the electromagnetic force. The electromagnetic force, one of the four fundamental forces in the universe (with the weak interaction or weak force, the strong interaction or strong force, and the gravitational force), operates over distance in a 1/d2 manner. At half the distance, four times the force is felt. At twice the distance, one fourth the force is felt. The thing that holds the nucleus together is the residual strong force, or residual strong nuclear force, the nuclear force or sometimes the (nuclear) binding energy or nuclear glue. (All these terms are sometimes seen.) This force has a quirky nature, and operates in the manner of 1/d4 across distances. You don't have to be a rocket scientist to see that it is really short range compared to the coulomb forces pushing the protons apart. And across large nuclei, it has an increasingly difficult time holding the nucleus together until, at some point, it simply can't do it. Links can be found below to check facts and learn more.

Positron-emission tomography forms images of body tissues this is known as what?

Positron-emission tomography (PET) forms images of body tissues using radioactive tracers that emit positrons. This imaging technique is used to detect functional processes in the body, such as metabolism or blood flow, and is commonly used in medical diagnosis and research.

How do particle accelerators work?

They accelerate particles using magnets. Once going at speed close to the speed of light, particles smash into each other. Accelerators are used to examine the properties of subatomic particles. There is an accelerator in Chicago called Fermilab, and another, larger on in Europe. See the large hadron collider for more info on current accelerators.

What is the most highly active atom in the nuclear atom system?

If you are looking for the most chemically reactive atom or element, it is fluorine. As regards which atom is the most active in its nucleus, there are a lot of very unstable radioactive atomic nuclei. Some are so unstable that they can only exist for a small fraction of a second, or, more properly, have an extremely short half-life.

Where are positrons found?

Positrons are anti-electrons. They're antimatter. They don't generally "hang around" in our "regular matter" universe very long. They can be created in a type of radioactive decay called beta plus decay. That means that any radioisotope that decays by beta plus means will create some.

We also find positrons here and there where high energy gamma rays are present. That's because gamma rays of sufficient energy will create electron-positron pairs (in an even called -- no surprise -- pair production) if those gamma rays pass close to atomic nuclei.

During stellar nucleosynthesis, the process powering most stars, positrons are created in astronomical numbers. These positrons are "contained" within the star and add energy to the fusion process within the star.

Because positrons find an electron to "combine" with in mutual annihilation, we don't "find" positrons around much. In an antimatter universe, they'd be circling the nuclei of antimatter atoms just like the electrons form up around the nuclei of the "regular" atoms in our universe.

How is a positron produced?

A positron is created in a pair production event or in beta+ nuclear decay (which is called positron emission). It (the positron) appears "out of nowhere" with an associated electron under certain conditions in pair production. And in the nuclear decay schemes of some radionuclides, it is generated spontaneously within the (unstable) nucleus and exits that nucleus in the decay event. Curious? Let's look further.

In positron emission (beta+ decay), a proton in an atomic nucleus experiences a change mediated by the weak interaction (the weak force), and one of its up quarks is transformed into a down quark. The change results in the "conversion" of a proton into a neutron. This causes atomic number to go down by one because there is one fewer proton in the atomic nucleus than just before the event. Here's an example:

In the beta plus decay of carbon-11, a new element, boron-11, is created. A positron, a neutrino, and a gamma ray will be ejected from the nucleus. Here's the equation for it:

6C => 5B + e+ + ve + 0.96 MeV

An atom of carbon becomes an atom of boron. The e+ is the positron and the ve is the neutrino. The gamma ray has an energy of 0.96 MeV (million electron-volts). There aren't many nuclei that do this. It is only seen in carbon-11, potassium-40, nitrogen-13, oxygen-15, fluorine-18, and iodine-121. That's it. Beta+ decay isn't all that tough to understand. What about pair production?

Pair production is the "making" of a positron and an electron out of a high energy gamma ray. Both pair production and beta plus nuclear decay occur naturally, so the positron can be said to occur in nature. Remember that the positron is an antiparticle - it's antimatter - and it will, after appearing, slow down via scattering and will eventually combine with an electron in mutual annihilation. The positron has a short mean lifetime and a short mean path of travel. They usually don't last long after they're created. But lets look at the creation of the particle pair.

The energy of the photon that creates the electron pair must have must meet a minimum threshold. And the threshold energy necessary for this even to be possible is 1.022 MeV. That's a lot of energy, and all that energy will be converted into mass - the rest mass of the electron and the rest mass of the positron. Higher energy gamma rays might still initiate pair production, but the extra energy would be accounted for in the kinetic energies of the pair of particles produced.

A gamma ray of sufficient energy passes near an atomic nucleus and the pair is produced. Note that pair production is not the spontaneous "option" that high energy gamma rays have. The photons must pass close by an atomic nucleus for there to be a probability that pair production will occur. This is because momentum must be conserved, and the "assisting" nucleus will handle this chore.

We should also note that researchers using high powered lasers on gold target material are able to produce considerable quantities of positrons for research, and this work is continuing. Links are provided to associated Wikipedia articles and related questions.

What is the Ruby laser wavelength?

A ruby laser is a red laser with a wavelength between 694 nm and 628 nm. 1 nanometer = 1×10−9 meter.

What are the uses of beta-glucanase?

Uses of Beta Glucanase
  • Beta Glucanase digests fiber. It helps remedy digestive problems such as malabsorption.
  • Beta Glucanase is a very important enzyme because the human body cannot produce it on its own.
  • Beta Glucanase helps in the breakdown of plant walls (cellulose), and increases the overall efficiency of binding excess cholesterol and toxins in the intestines for removal.
  • Beta Glucanase may be beneficial for food and environmental allergies, drug withdrawal, cell detoxification, colon cleaning and pain syndromes, Candida (yeast infections), gas, bloating, acute food allergies, facial pain or paralysis.
  • Beta Glucanase is used for commercial food processing in coffee.
  • It performs hydrolysis of cellulose during drying of beans.
  • Beta Glucanase is used in the fermentation of biomass into biofuels, although this process is relatively experimental at present.
  • Beta Glucanase is used as a treatment for Phytobezoars, a form of cellulose bezoar found in the human stomach.
  • Beta Glucanase is used in animal healthcare as a feed supplement for better FCR and Milk yield Inhancer in Poultry and Cattle industry.
  • Beta Glucanase is used in textile industry as a fading agent.

    http://www.enzymeindia.com/enzymes/beta-glucanase.asp

If Pu239 emits alpha particles of energy 5.4Mev calculate the decay probability?

It is possible to relate a decay constant of some α emitting nucleus to an energy of α particle in the framework of the Gamow theory (see Related links) that is based on the quantum mechanics description of the tunneling through the potential barriers.

Previous view (by Quirkyquantummechanic)The fact that 239Pu decays by alpha particle emission (with the α particle coming away at 5.245 Mev) has nothing to do with this isotope of plutonium's decay probability. The decay probability of 239Pu (or anything else) can be expressed as a distribution function. That's math speak. What that means is that any nuclear decay event has "odds" that it may happen. Let's look at that a bit.

All unstable radionuclides will eventually decay. But when? Well, they all have some, um, "quirks" about them. Some take a long time to eventually fall apart, but some don't take that long. All we can do is "average out" the decay of a given material. Got that idea? It's important. And one of the ways we talk about the decay probability is in terms of something called the half life of a material. In the case of 239Pu, for example, the half life is 2.41 x 104 years. That's 24,100 years. What that means is that if we have a kilogram of the stuff, in 24,100 years, only half of the plutonium we started with will be left. Make sense? Mmhmm. But check this out. If we have two atoms of the stuff, does that mean that in 24,100 years only one will be here? No, it does not. They could both decay in the next week or the next month. Or the next century. Half life is a "probability thing" with unstable materials. And it is calculated across a "curve" of probability (that distribution function we mentioned) based on measurements of a quantity of the material being considered. It's that simple.

As an aside, but on a related note, if you guessed that the artificial elements (we call them synthetic, because they must be synthesized or made) that we know of by only a few atoms don't have very accurate measurements of their half lives, you'd be absolutely right. It's really difficult to (with accuracy) "guestimate" the half life of something, of some element, that is known from only a dozen atoms of the material....

A magnetic field is created by a charged particle that is?

in motion. The moving charged particle generates a magnetic field around it, with the strength of the field depending on the particle's charge and velocity. This magnetic field exerts a force on other moving charged particles in its vicinity, influencing their motion.

Mass of alpha particle?

The mass of an alpha particle is 4 atomic mass units, 2 protons and 2 neutrons, or about 6.644656 x 10-27 kg.

Why are alpha and beta rays deflected in opposite directions in a magnetic field?

An alpha particle, which is a 24He nucleus, has a mass of 4 and a charge of +2. A beta particle has a charge of +1 or -1, depending on whether it is a positron (beta +) or an electron (beta -). It's mass is minuscule compared to the alpha particle, and it will undergo a comparatively huge deflection in the same field as an alpha particle would. Though the alpha particle has twice the charge as a beta particle, it has several thousand times the mass of that beta particle. As it is so much more massive than the beta particle, its inertia will be much more difficult to overcome even though it has twice the charge.

Does an electron-positron collision violate the law of conservation of matter?

No, electron-positron collision does not violate the law of the conservation of matter. Momentum and charge are also conserved. Electrons and positrons can collide in what are called scattering events, and they can do this without necessarily undergoing mutual annihilation. Because both these little critters can exist as a wave (particle-wave duality), their behavior can be fairly easily assessed using a "basic tool kit" to analyze electromagnetic wave interaction. But electrons and positrons can annihilate each other rather than scatter. Annihilation doesn't violate the law of conservation of matter, either. And there's a reason for that. The "old" idea of the conservation of matter was that matter could neither be created nor destroyed. But we now know that matter can be converted into energy. That's what happens in annihilation. The article in Wikipedia on the annihilation event touches on electron-positron collision. And there is an article on electromagnetic scattering as well. They aren't that difficult to understand, and the curious person will find links to those posts below.