Save
Upgrade to remove ads
Busy. Please wait.
Log in with Clever
or

show password
Forgot Password?

Don't have an account?  Sign up 
Sign up using Clever
or

Username is available taken
show password


Make sure to remember your password. If you forget it there is no way for StudyStack to send you a reset link. You would need to create a new account.
Your email address is only used to allow you to reset your password. See our Privacy Policy and Terms of Service.


Already a StudyStack user? Log In

Reset Password
Enter the associated with your account, and we'll email you a link to reset your password.
focusNode
Didn't know it?
click below
 
Knew it?
click below
Don't Know
Remaining cards (0)
Know
0:00
Embed Code - If you would like this activity on your web page, copy the script below and paste it into your web page.

  Normal Size     Small Size show me how

ENU4612

TermDefinition
Fast electrons Beta particles (β⁺ or β⁻), energetic electrons from any process
Heavy charged particles All energetic ions with mass ≥ 1 amu
Charged Particulate Radiation Fast electrons or Heavy charged particles (e.g. Alpha particles, protons, fission products, nuclear reaction products)
Electromagnetic radiation X-rays from electron shell rearrangement, gamma rays from nuclear transitions
Neutrons Generated in nuclear processes
Uncharged Radiation Electromagnetic radiation, Neutrons, and Further divided into slow neutron and fast neutron subcategories
hardness Radiations differ in their "___________" or ability to penetrate thicknesses of material.
Soft Radiations (e.g.) Alpha particles and Low-energy X-rays,
Soft Radiations (Source Thickness) micrometers
Soft Radiations (Problem) Self-absorption affects number and energy spectrum
Medium Penetration (e.g.) Beta particles which are more penetrating than alphas
Medium Penetration (Source Thickness) Few tenths of millimeter
Medium Penetration (Tolerance) Can usually be tolerated
Hard Radiations (e.g.) Gamma rays and Neutrons
Hard Radiations (Source Thickness) Millimeters to centimeters
Hard Radiations (Advantage) Minimal self-absorption effects
Self-Absorption Effect Only atoms near the surface contribute photons that escape from thicker sources. This affects both the intensity and energy spectrum of emerging radiation.
Fundamental Law of Radioactive Decay dN/dt|decay = -λN; Where: N = number of radioactive nuclei, λ = decay constant
milli (m) 0.001 or 10^-3
micro (μ) 0.000001 or 10^-6
nano (n) 0.000000001 or 10^-9
kilo (k) 1000 or 10^3
mega (M) 1000000 or 10^6
giga (G) 1000000000 or 10^9
Curie (Ci) Exactly 3.7 × 10¹⁰ disintegrations/second, Based on activity of 1 gram of pure ²²⁶Ra, More suitable for laboratory sources, historical unit
Becquerel (Bq) One disintegration per second, Adopted in 1975, Conversion: 1 Bq = 2.703 × 10⁻¹¹ Ci
Activity _________ measures source disintegration rate, which is NOT synonymous with radiation emission rate
Specific Activity _____________________ = Activity/Mass = λN/(NM/Av) = λAv/M; M = molecular weight of sample, Av = Avogadro's number (6.02 × 10²³ nuclei/mole), λ = radioisotope decay constant (= ln 2/half-life)
Pure samples Unmixed with other nuclear species
Diluted samples Mixed with stable nuclei of same element
Chemical compounds Additional stable nuclei from other elements
large Higher specific activity are obtained using radionuclides with _____ λ
Short half-life = = high specific activity
Electron Volt (eV) Traditional unit, Kinetic energy gained by electron accelerated through 1 volt potential difference, Convenient for particulate radiation
Joule (J) 1 eV = 1.602 × 10⁻¹⁹ J; SI unit though eV is not likely to be phased out due to physical basis and universal use in literature
Planck's constant h = 6.626 × 10⁻³⁴ J·s or 4.135 × 10⁻¹⁵ eV·s
Energy-Frequency E = hν
Wavelength-Energy λ = 1.240 × 10⁻⁶/E; where λ is in meters and E is in eV
Beta Decay Continuous energy spectrum from nuclear decay
Internal Conversion Monoenergetic electrons from nuclear transitions
Auger Electrons Low-energy electrons from atomic processes roughly the analogue of internal conversion electrons when the excitation energy originates in the atom rather than in the nucleus
Fast Electron Sources The most common source of fast electrons in radiation measurements
Beta Decay equation A ZX → AZ+1Y + β⁻ + ν-
Recoil nucleus Very small recoil energy, below ionization threshold
Beta Decay Products Final nucleus Y, beta particle, antineutrino
Neutrino Extremely small interaction probability - undetectable
Beta Decay Detectable radiation Only the fast electron (beta particle)
Beta Decay Source Availability Most radionuclides from neutron bombardment are beta-active, Large assortment readily available from reactor production, Wide range of half-lives: days to thousands of years, Many decay to excited states → gamma rays also emitted
Q-Value and Energy Sharing in Beta Decay Each specific beta decay transition is characterized by a fixed decay energy or Q-value. Since recoil nucleus energy is virtually zero, this energy is shared between the beta particle and the "invisible" neutrino
Beta Decay Energy Distribution Range: Zero to "beta endpoint energy", Endpoint energy: Numerically equal to Q-value, Shape: Continuous spectrum (see Fig. 1.1), Multiple components: If several excited states populated
"Pure" Beta-Minus Sources nuclides that decay directly to ground state (no gamma contamination); e.g. 3H, 14C, 32P
Internal Conversion Process -Begins with excited nuclear state -Alternative to gamma-ray emission -Nuclear excitation energy transferred directly to orbital electron -Most often occurs for somewhat inhibited gamma emission
Internal Conversion Formula Ee- = Eex - Eb Ee- = conversion electron energy Eex = nuclear excitation energy Eb = electron binding energy in original shell
Electron Shell Groups K-shell conversion: Highest electron relative yield L-shell conversion: Lower electron relative yield M-shell conversion: Lowest electron relative yield
Auger Electron Energy Formula EAuger = Eatomic excitation - Ebinding energy
Auger Electrons Process - Initial state: Vacancy in normally complete electron shell - Cause: Preceding process (e.g., electron capture) - Competing process: Characteristic X-ray emission - Alternative: Energy transferred directly to outer electron
Created by: user-2062823
 

 



Voices

Use these flashcards to help memorize information. Look at the large card and try to recall what is on the other side. Then click the card to flip it. If you knew the answer, click the green Know box. Otherwise, click the red Don't know box.

When you've placed seven or more cards in the Don't know box, click "retry" to try those cards again.

If you've accidentally put the card in the wrong box, just click on the card to take it out of the box.

You can also use your keyboard to move the cards as follows:

If you are logged in to your account, this website will remember which cards you know and don't know so that they are in the same box the next time you log in.

When you need a break, try one of the other activities listed below the flashcards like Matching, Snowman, or Hungry Bug. Although it may feel like you're playing a game, your brain is still making more connections with the information to help you out.

To see how well you know the information, try the Quiz or Test activity.

Pass complete!
"Know" box contains:
Time elapsed:
Retries:
restart all cards