Radiation Hazards

See also: Nuclear_power_reconsidered

See also: Fear of radiation

Fig. 1 Handy chart from xkcd.com compares radiation doses.

© Image: Robert Hargraves, PhD
Fig. 2 Effects of free radicals on DNA.

Radiation hazards are not as straightforward to understand as anyone would like. A primary obstacle to gaining public acceptance for improved nuclear energy technology is a generalized fear of radiation. People have difficulty distinguishing between a little and a lot, so that this has often been oversimplified to, "The only acceptable amount of radiation is zero!", a goal has never been met, since (for example) all living things are radioactive. A sensible criterion must be based on an understanding of where radiation comes from, what sorts of damage radiation does, and how much of which kind of radiation, delivered over what time scale, it takes to do it.

Figure 1 compares a range of radiation exposures, from the dose received from sleeping next to another human for a night (0.05 $\mu$Sv) to the usually fatal dose of 4 Sv, a hundred million times greater. Warning: such comparisons can be misleading unless one understands that some are "delivered all at once" and others are "accumulative" over times up to a year. There is great controversy over the latter, since DNA usually "heals" strand-breaks due to free radicals produced by ionizing radiation (see Fig. 2) within hours or days, suggesting that whole-body doses may not "accumulate" over longer periods.

Mortality

Paraphrased from memory: Front page of special HEALTH edition of the LA Free Press (around 1970):

"No matter how much money you have, how good your health care provider or how healthy your diet and life style, you, personally, are going to die."

(I don't really want to believe this any more than you do, but I have to confess that the evidence for it is persuasive.)

Either way, it makes an excellent starting point for any discussion of hazards. We cannot (for now) avoid dying, but we can exercise some influence over when we will die and from what causes. We also (for now) get to choose how much of our enjoyment of life and liberty we sacrifice to this effort.

What is "Radiation"?

There are many kinds of "rays" and waves that act like tiny particles, carrying a large amount of kinetic energy for their size and traveling at or near the speed of light, that are termed "radiation" in this context. Whether they constitute a "hazard" depends on their charge, mass and energy. They fall into the following general groups:

• Electromagnetic Waves:

- AM Radio, FM Radio, Shortwave Radio, TV, Cell Phones, WiFi, Microwave, Visible Light — all harmless at low intensity.

- Near Ultraviolet (UV) — beneficial at low doses (Vitamin D)

- Far UV, X-rays, Gamma-rays — damaging wherever absorbed. (Note that a sunburn is a second-degree radiation burn to the skin.)

• Fast Massive Particles:

- Electrons ($\beta$-rays)

- Protons & Neutrons

- $\alpha$-rays (⁴He nuclei)

- Heavy Ion Beams

• What does the Damage?

- Enough intensity of anything will "cook" you.

- Highly reactive free radicals produced by (among other things) Ionizing Radiation.

What is Ionizing Radiation?

Radiation is ionizing if its quantum energy is enough to ionize a neutral atom or molecule, typically 2 eV. For electromagnetic radiation, this means the wavelength must be shorter than half a micron (blue light). So ultraviolet, X-rays and gamma rays can all be ionizing. Cell phones and microwave ovens cannot. Note that quantum energy ($\varepsilon =\hbar \omega$) is not the same as the intensity of the radiation. A microwave produces a huge quantity of very low-energy photons. It will heat your food, but thermal energy is not ionizing until you get up to a few thousand degrees C (when the flame emits light). The sun is 5000 degrees, so if you went there, you would be totally ionized.

Charged particle radiation (alpha, beta) is ionizing, because the particles typically have energies much larger than 2 eV.

Neutrons cause ionization indirectly. Slow (thermal) neutrons can be absorbed by a stable nucleus, activating it to a radioisotope that later decays by emitting an ionizing charged particle or a gamma ray. Fast (high energy) neutrons cause "secondary ionization" by colliding elastically with charged nuclei (especially hydrogen) which recoil with enough energy to ionize other atoms. Fast neutrons usually do more damage than slow neutrons.

What sort of damage?

Ionizing Radiation $\to$ DNA Strand Breaks

• Single strand breaks usually heal in less than a few hours.

• Double strand breaks are sometimes permanent, causing…

- Cell Reproductive Death (most common): Cells usually survive for natural lifetimes — a few days for hair follicles, skin and mucous membrane cells; "forever" for neurons and some muscle cells.

- Genetic Mutation (most subtle): Damaged gamete cells → mutations (usually fatal to foetus; almost always detrimental to individual…)

- Cancer (most unpleasant): Runaway replicative zeal of a misguided cell…

Cancer Therapy

Most cancer radiation therapies involve radiation insults that inflict DNA damage similar to that caused by "bad" radiation.

Strategy: to kill every single cancer cell (along with up to 90% of nearby normal cells).

Dose may be more than 10,000 times maximum legal limit for "accidental" radiation exposure… but are normally not "whole body".

Why Worry, and When? (Informed Consent vs. Public Policy)

Cost/Benefit Analyses: Every public policy decision creates risks. Is this likely to do any good? How much good? Is it likely to do any harm? How much harm? What are the relative probabilities of good and harm? How many people are likely to suffer from the harm? How many people are likely to benefit from the good? And of course the two questions most important to politicians: "Which people?" and "When?"

Any sensible policy regarding radiation hazards, whether public or personal, must take into account that each of us is going to die, that our lifespan is frustratingly short no matter what we do, and that our chances of dying of cancer (radiation-induced or otherwise) are already rather high. (Men have just over a 20% risk of dying from cancer, while women's risk is just over 18%.)

How Bad is How Much of What?

Units:

• 1 rad ≡ 100 erg/g (energy deposited per unit mass)

• 1 Gray (Gy) ≡ 100 rad ≡ 1 J/kg. [SI units]

Relative Biological Effectiveness (RBE) "fudge factor":

• X-rays, γ-rays & β-rays (fast electrons): RBE = 1 (by definition)

• Slow neutrons: average RBE ≈ 3. (Variable!)

• Fast neutrons, protons & α-rays: RBE = 10.

• Fast heavy ions: RBE = 20.

REM (R, Roentgen Equivalent to Man):

• 1 R ≡ RBE × rad.

• (1 mR ≡ milliREM] ≡ 10−3 R.)

• Sievert (Sv) [Standard International unit]: 1 Sv ≡ 100 REM

EFFECTS

• Instant Death: ∼ 5000 R (50 Sieverts [Sv]) “whole-body” wipes out central nervous system (CNS) immediately when delivered all at once.

• Overnight Death: ∼ 900 R (9 Sv) whole-body usually accomplishes the same thing in about a day.

• Ugly Death: ∼ 500 R (5 Sv) → severe radiation sickness (nausea, hair loss, skin lesions, etc.) as short-lived cells fail to provide new generations to replace their normal mortality. Complications (infection) usually kill. Some recover completely but may develop leukemia 10-20 years later; offspring (if any) will likely have genetic mutations.

• Sub-Acute Exposures: ∼ 100 R (1 Sv) whole-body delivered in less than 1 week → no immediate symptoms, but possible leukemia in 10-30 years and possible genetic mutations in offspring.

• Marginal Exposures: average exposure in USA from natural & medical sources ∼ 620 mR (6.2 mSv) per year. (The current federal occupational limit of exposure per year for an adult (the limit for a worker using radiation) in the USA is "as low as reasonably achievable; however, not to exceed 5,000 mR [50 mSv]" above the 300+ mR of natural sources of radiation and any medical radiation.)

Different body parts have dramatically different resistance to radiation. Hands can withstand radiation doses that would kill if delivered to the whole body. The gonads and the lens of the eye are considered to be the most vulnerable.

Note that for long-lived cells like neurons and muscle cells, cumulative doses over times as long as a year have little meaning in light of the typical time scale of DNA strand-break healing. (See Ref. 2.) However, short-lived cells like skin cells replicate fast enough that even a partially damaged cell can sometimes propagate itself into a local "precancerous" population that is then vulnerable to subsequent damage leading to malignant cancer. For this reason the most common type of dangerous radiation-induced cancer is the skin cancer melanoma, which is strongly associated with sun exposure. In the USA, the rate of melanoma diagnoses is 78,000 per year or 21.8 per 100,000. The mortality rate is 11.5%.

There is some evidence (e.g. from Ramsar, Iran) for radiation hormesis (marginal exposures may actually promote better health).

Sources of Ionizing Radiation

According to the 2021 EPA survey, the average annual doses to USA population have the following sources and magnitudes:

See EPA pie chart.

Note that cosmic rays make a significant contribution to these accumulated doses. Fortunately our atmosphere makes an excellent shield; but since it is most dense near sea level, people living at high altitude (like Denver) receive a higher annual dose, and flying at 40,000 feet delivers about 0.7 mR per hour.

NOTE: Since rates of exposure vary constantly, the temptation to average over a year is understandable; however, for the majority of cell types, given that the only damage that matters (DNA strand breaks) usually heals on a time scale of less than days, the above numbers are almost meaningless in terms of health risk -- except for sun damage to the skin, which is accumulative.

More useful are the "all at once" exposures we are apt to encounter:

• Medical X-rays:

- Whole Body CT scan: 1,000 mR (10 mSv) per exposure

- Upper GI X-ray: 600 mR (6 mSv) per exposure

- Head CT scan: 200 mR (2 mSv) per exposure

- Mammogram: 42 mR (0.42 mSv) per exposure

- Chest X-ray: 10 mR (0.1 mSv) per exposure

Natural Terrestrial Radionuclides

Gamma (γ) radiation is fairly uniform in the USA, ranging from 30 mR/y in Texas to 115 mR/y in South Dakota.

The Really Bad Stuff: Ingested Radionuclides

Many radionuclides (radioactive isotopes) emit fast α particles (⁴He nuclei). The range of most α "rays" is only on the order of cm in air and mm in tissue. This is good if they are at arm's length; but it's bad if you swallow them or breathe them! A wide variety of radioactive elements have assorted chemical properties, each with a specific hazard.

• Radon: All rock contains some radium which slowly decays, releasing the chemically inert noble gas radon, itself a radioactive element which emits a low energy α (difficult to detect). Radon probably killed Madame Curie. Radon exposure is widespread and dangerous because it accumulates in the air of any building made of rock, brick or concrete (especially those with closed air circulation) and thence in the lungs of the people breathing that air, who become radioactive (easy to detect). Different regions have a huge range of radium content, so a stone house may be perfectly safe in one place and hazardous in another.

• Potassium & Carbon: Radioisotopes of K and C are continually created in the atmosphere by cosmic ray bombardment and build up to a constant level in all living tissues, only to decay away in a few thousand years after death. You are radioactive! Potassium-Argon and ¹⁴C dating provides handy means of estimating how long ago biological matter was alive.

• Man-Made Radionuclides: Formerly most famous: plutonium, ²³⁹Pu, of which fission bombs are made. A deadly chemical poison as well as a nasty radioisotope, a miniscule grain of ²³⁹Pu caught in your lungs or other tissues exposes (only) nearby tissue to a huge dose.

Newly famous: polonium, ²¹⁰Po, is made in reactors by adding neutrons to bismuth. It is an even deadlier poison.

The food chain concentrates "harmless" levels to dangerous ones; fission waste products include many radionuclides with chemical properties not seen in naturally occurring isotopes. Otherwise it might be marginally sensible to dispose of radioactive waste by diluting it in the oceans. Although radioisotopes from the Fukushima meltdown were easily detected on the Pacific coast of North America, the levels were utterly harmless.

It's important to understand the difference between "detectable" and "dangerous".

In the 1960s we could detect parts per million (ppm) of Selenium (Se), a heavy metal which is poisonous at that concentration. The US Congress then passed a law making it illegal for any foodstuffs to contain a detectable amount of Se. A few years later we were able to detect parts per billion (ppb). That’s when we discovered that Se is an essential mineral. This illustrates the foolishness of any policy of "zero tolerance". The current policy regarding radiation exposure from nuclear reactors is ALARA ("As Low As Reasonably Achievable"), which is routinely interpreted as "zero tolerance" even though there is no evidence for significant deleterious effects of marginal exposures, and even some evidence for beneficial effects ("radiation hormesis").

Protection Against Radiation

The best shielding is provided by Gauss' Law: intensity ∝ 1/r². Localized sources are labelled with their activity at a given distance, for instance "10 mR/h at 1 m", which becomes 0.1 mR/h at 10 m. Just walk away! By the same token, never touch a radioactive source! (1/r² → ∞ as r → 0).

Lead aprons are effective only for X-rays, γ-rays and low energy β-rays. Thick concrete shielding is needed for neutrons and high-energy charged particles.

For ingested radionuclides, chelation can sometimes help. In the case of tritium (³H), one should drink lots of beer!