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title: "ChEn 433 Nuclear"
date: Class 16-17
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# Nuclear
What are the major issues associated with nuclear power?

::: incremental
* No GHG emissions (CO$_2$)
* Environmental concerns
* Safety concerns
* Proliferation
* Waste storage
* Fuel resources
* Regulation
* Public perception
:::

# Nuclear timeline
<div class="scrollpic">
<img src="https://whatisnuclear.com/img/nuclear_timeline.png" title="https://whatisnuclear.com/img/nuclear_timeline.png" alt="image">
</div>

# U.S. nuclear power by year
<img src="nuclear_by_year.png" title="https://www.eia.gov/energyexplained/nuclear/us-nuclear-industry.php" width=80% alt="image">

## U.S. nuclear plant locations
<img src="https://www.eia.gov/energyexplained/nuclear/images/US_nuclear_power_plants_map.png" title="https://www.eia.gov/energyexplained/nuclear/images/US_nuclear_power_plants_map.png" width=90% alt="image">

## U.S. nuclear plant stats
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* [20% of U.S. electricity from nuclear](https://www.eia.gov/tools/faqs/faq.php?id=427&t=3)
* First plant in U.S. in 1958
* 2021 stats
    * 94 reactors, ~1 GW each (avg)
    * 56 plants
    * 28 states
    * Average age is 39 years
* Oldest plant is Nine Mile Point (NY), Dec. 1969, 52 years
* Newest is [Vogtle Unit 4, 2023](https://www.georgiapower.com/company/news-hub/press-releases/vogtle-unit-4-enters-commercial-operation.html), Georgia
:::
::: {.col2-v}
<img src="https://www.asme.org/wwwasmeorg/media/asmemedia/about%20asme/whoweare/history/landmarks/47-shippingport-nuclear-power-station_01.jpg" title="https://www.asme.org/wwwasmeorg/media/asmemedia/about%20asme/whoweare/history/landmarks/47-shippingport-nuclear-power-station_01.jpg" width=600 alt="image">
<p style="font-size: 0.7em">
*Shippingport Power Station, Pennsylvania*
</p>
:::
:::

## U.S. nuclear plants timeline
<img src="https://www.eia.gov/todayinenergy/images/2023.08.01/main.svg" title="https://www.eia.gov/todayinenergy/images/2023.08.01/main.svg" width=1200 alt="image">

::: notes
bar chart of US nuclear power capacity additions, by year of initial operation (1970-2023), GW, includes Vogtle 3 unit
:::


## World nuclear plants
<img src="nuclear_countries.png" title="https://www.eia.gov/energyexplained/nuclear/data-and-statistics.php" width=1000 alt="image">

* ~156 plants in service (> 1000 MW)
* Google "list of nuclear reactors" --> people also ask...

## World nuclear plants
<img src="world_nuclear_plants.svg" title="data, not plot, from https://en.wikipedia.org/wiki/List_of_nuclear_power_stations" width=3600 alt="image">

# Exercise: World Electricity as Nuclear
::: {.cols2}
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* Look up the world total electricity production. <a href="https://www.energyinst.org/statistical-review" target="_blank">Energy Institute</a>
* Convert this to <a href="https://en.wikipedia.org/wiki/A_Cubic_Mile_of_Oil" target="_blank">CMO</a>
* If run continuosly over the year, find the power in GW
* What is the largest nuclear power plant, and it's power?
* What is the <a href="https://en.wikipedia.org/wiki/List_of_nuclear_power_stations" target="_blank">average size</a> nuclear power plant > 1000 MW?
* How many of the largest and average size plants are needed?
* If one plant is built per week, how many years are needed?
:::
::: {.col2-v}
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/5/56/Kashiwazaki-Kariwa_04780017_%288388173865%29.jpg/600px-Kashiwazaki-Kariwa_04780017_%288388173865%29.jpg" title="https://en.wikipedia.org/wiki/File:Kashiwazaki-Kariwa_04780017_(8388173865).jpg" width=700 alt="image">
:::
:::

## Exercise: World Electricity as Nuclear

::: incremental
* BP: 26823 TWh $\cdot$ 3600 s/h = 9.65628E19 J (per year)
* 1.6E20 J/CMO $\rightarrow$ 0.6 CMO
* 9.65628E19 J/yr $\cdot$ yr/(3600 $\cdot$ 24 $\cdot$ 365 s) $\cdot$ GW/1E9 W = 3062 GW 
* Largest plant is the [Kashiwazaki-Kariwa (K-K) Plant](https://en.wikipedia.org/wiki/Kashiwazaki-Kariwa_Nuclear_Power_Plant) in Japan
    * 7965 MW
* Avg size plant = 2382 MW (for plants over 1000 MW)
    * 155 plants over 1000 MW
* \# K-K plants = 3062/7.965/0.92 = 418 
    * with a [92% capacity factor](https://www.energy.gov/ne/articles/what-generation-capacity#:~:text=Nuclear%20has%20the%20highest%20capacity,and%20solar%20(25%25)%20plants.)
    * 1 plant per week for 8 years
* \# avg plants = 3062/2.382/0.92 = 1397
    * 1 plant per week for 27 years
:::

# Isotope binding energy
Isotope Binding Energy
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/5/53/Binding_energy_curve_-_common_isotopes.svg/1342px-Binding_energy_curve_-_common_isotopes.svg.png" title="https://upload.wikimedia.org/wikipedia/commons/thumb/5/53/Binding_energy_curve_-_common_isotopes.svg/1342px-Binding_energy_curve_-_common_isotopes.svg.png" width=1200 alt="image">

## Stardust
[Genesis 3:19](https://www.churchofjesuschrist.org/study/scriptures/ot/gen/3?lang=eng) ...for dust thou art, and unto dust shalt thou return

["It is totally 100% true: nearly all the elements in the human body were made in a star and many have come through several supernovas."](https://www.nhm.ac.uk/discover/are-we-really-made-of-stardust.html)

<img src="https://www.nhm.ac.uk/content/dam/nhmwww/discover/we-are-stars/stardust-infographic-two-column.jpg.thumb.768.768.jpg" title="https://www.nhm.ac.uk/content/dam/nhmwww/discover/we-are-stars/stardust-infographic-two-column.jpg.thumb.768.768.jpg" width=800 alt="image">

## Emission/Decay
* $\alpha$ (helium nucleus), e.g., 
    * $^{238}_{92}\text{U} \rightarrow ^{234}_{90}\!\!\text{Th} + ^4_2\!\text{He}$
* $\beta^-$ (emitted electron)
    * $n \rightarrow p + e^- + v_e$
* $\beta^+$ (positron, ~ a positively charged electron)
    * $p \rightarrow n + e^+ + v_e$
* $\gamma$ (high energy photon)
    * often occurs from an excited daughter nucleus after $\alpha$ or $\beta$ decay

::: notes
$\beta^+$ and $\beta^-$ emission occur in nuclei not bare $p$ or $n$
:::

## Table of Nuclides
<iframe src="https://www-nds.iaea.org/relnsd/vcharthtml/VChartHTML.html" width=1200 height=800></iframe>

## Half life
::: {.cols2}
::: {.col2-l}

**Equation for radiactive decay?**

::: incremental
* Radioactive decay is governed by $\frac{dN}{dt} = -N/\tau$,  $N(0) = N_0$.
* Here, $\tau$ is the characteristic decay time.
* The analytic solution is 
<div style="color:blue">
$$N = N_0e^{-t/\tau}$$
</div>
* Relate this to the half-life: $\frac{N}{N_0} = \frac{1}{2} = e^{-t_{1/2}/\tau}\rightarrow \tau = -t_{1/2}/\ln(1/2)$
    $$\tau = t_{1/2}/\ln(2)$$
    $$t_{1/2} = \tau\ln(2)$$
<p style="color:red">
$$N = N_0\left(\frac{1}{2}\right)^{t/t_{1/2}}$$
</p>
:::
:::
::: {.col2-v}
::: fragment
<img src="halflife.svg" width=800 alt="image">
:::
:::
:::

## Radiation penetration
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/6/61/Alfa_beta_gamma_radiation_penetration.svg/2880px-Alfa_beta_gamma_radiation_penetration.svg.png" title="https://upload.wikimedia.org/wikipedia/commons/thumb/6/61/Alfa_beta_gamma_radiation_penetration.svg/2880px-Alfa_beta_gamma_radiation_penetration.svg.png" width=800 alt="image">

* $\alpha$ stopped by paper, dead outer layer of skin (dangerous if injested)
    * Polonium-210 [poisoning of Alexander Litvinenko](https://en.wikipedia.org/wiki/Poisoning_of_Alexander_Litvinenko#Illness_and_poisoning)
* $\beta$ stopped by aluminum foil, can penetrate ~1/2 inch into skin
* $\gamma$ stopped by lead, thick concrete

## Radiation penetration
<iframe width="1244" height="700" src="https://www.youtube.com/embed/wsspFQn0mWM?cc_load_policy=1" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>

## Ionization demonstration
<iframe width="1244" height="700" src="https://www.youtube.com/embed/ZBHIp967TD8?cc_load_policy=1" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>

# U-235 Fission
::: {.cols2}
::: {.col2-vp}
* $^{235}U + n \rightarrow [^{236}U] \rightarrow ^{144}Ba + ^{89}Kr + 3n$
    * typical
* 1n $\rightarrow$ 2.5n *daughter* neutrons
* *prompt* neutrons are fast: 
    * ~2 MeV = 19.5 million m/s (7% of light).

<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/6/68/ThermalFissionYield.svg/2560px-ThermalFissionYield.svg.png" title="https://upload.wikimedia.org/wikipedia/commons/thumb/6/68/ThermalFissionYield.svg/2560px-ThermalFissionYield.svg.png" width=600 alt="image">
:::
::: {.col2-v}
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/1/15/Nuclear_fission.svg/1024px-Nuclear_fission.svg.png" title="https://upload.wikimedia.org/wikipedia/commons/thumb/1/15/Nuclear_fission.svg/1024px-Nuclear_fission.svg.png" height=800 alt="image">
:::
:::

## Chain reaction
::: {.cols2}
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::: incremental
* Neutron fate:
    * Fission
    * Absorbed (e.g., by U-238)
    * Escape 
        * (bare n is unstable $\rightarrow$ p+$e^-$)
        * half life ~ 10 minutes.
* [Chain reaction](https://en.wikipedia.org/wiki/Nuclear_chain_reaction)
    * 1 fission creates $\ge$ 1 fission
* Energy from mass:
$$\Delta m = m_\text{reactants} - m_\text{products}$$
$$\Delta m = \frac{E}{c^2}$$
    * mass difference as kinetic energy of fission products $\rightarrow$ slows $\rightarrow$ heat.
* Neutrons + protons are conserved, electrons are not (formed).
* Energy released as more stable nuclei are formed (sounds familiar)
:::
:::
::: {.col2-v}
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/9/9a/Fission_chain_reaction.svg/1024px-Fission_chain_reaction.svg.png" title="https://upload.wikimedia.org/wikipedia/commons/thumb/9/9a/Fission_chain_reaction.svg/1024px-Fission_chain_reaction.svg.png" width=500 alt="image">
:::
:::

## Exercise: mass $\rightarrow$ energy
How much mass converted fully to energy equivalent to 1 CMO?

::: incremental
* 1 CMO = 1.6E20 J 
* $E = mc^2$ $\rightarrow$ $m = E/c^2$
* c = 299792458 m/s
* m = 1780 kg
* ~ 2 m$^3$ of oil (@ 890 kg/m$^3$)
* Volume is 9 billion times less than 1 CMO
:::
::: fragment
*Of course, nuclear reactions never approach full mass conversion.*  
1 CMO requires about 2000 tons of U-235 fission
:::
::: notes
U235 + n --> Ba-144 + Kr-189 + 3n
mU = 235.043928 amu
mn = 1.008664916 amu
mBa = 143.922955 amu
mKr = 88.907835 amu
dM = mReact - mProd = 0.195808 amu
dM/mU = 0.000833 = rest mass change per mass of U-235
So, if 1 cmo = 1780 kg, then 1780/0.000833 is the mass of U235 fission for 1 CMO = 2.1368E6 kg = 2355 tons
CMO book p 130 quotes "about 2000 tons of U235 can release as much energy as burning 4.2 billion tons of oil (which is 1 CMO)."
:::

## Cross section
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* [Cross section](https://www.nuclear-power.com/nuclear-power/reactor-physics/nuclear-engineering-fundamentals/neutron-nuclear-reactions/microscopic-cross-section/) is an area of interaction of a target particle
* May be bigger or smaller than the geometrical area
    * In this sense it's *like* a probability of interation
* Units: 1 **barn** = 10$^{-28}$ m$^3$
    * as in "you couldn't hit the broad side of a barn"
* Depends on the nucleus and the neutron energy
    * Fast (prompt) neutrons are released during fusion ([0.1 - 10 MeV](https://www.nuclear-power.com/nuclear-power/fission/prompt-neutrons/prompt-neutrons-and-delayed-neutrons/)).
    * These have low fission cross sections though, so they are slowed down to "thermal" by neutron interactions with a *moderator*.
    * Thermal neutrons (0.025 eV at 17 $^o$C, ~2.2 km/s=4900 mph)
:::
::: {.col2-v}
<img src="https://nuclear-power.com/wp-content/uploads/2016/01/nuclear-cross-section-min.png" title="https://nuclear-power.com/wp-content/uploads/2016/01/nuclear-cross-section-min.png" height=800 alt="image">
:::
:::

## Cross section
<img src="http://nuclear-power.com/wp-content/uploads/2014/11/cross-sections_nuclides.png" title="http://nuclear-power.com/wp-content/uploads/2014/11/cross-sections_nuclides.png" height=700 alt="image">

[nuclear-power.com](https://www.nuclear-power.com/nuclear-power/reactor-physics/nuclear-engineering-fundamentals/neutron-nuclear-reactions/microscopic-cross-section/)

## Neutron moderator
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<div style="font-size:0.8em;">
* Fast (prompt) neutrons are released during fusion ([0.1 - 10 MeV](https://www.nuclear-power.com/nuclear-power/fission/prompt-neutrons/prompt-neutrons-and-delayed-neutrons/)).
* These have low fission cross sections though, so they are slowed down to "thermal" by neutron interactions with a [*moderator*.](https://www.nuclear-power.com/neutron-moderator/)
* Thermal neutrons (0.025 eV at 17 $^o$C, ~2.2 km/s=4900 mph)

::: fragment
**Question: how to slow the neutrons down?**
:::
::: fragment
Collide with masses similar to the mass of a neutron. Recall [elastic collisions](https://en.wikipedia.org/wiki/Elastic_collision). So, what to use?
:::
::: fragment
Hydrogen (water)
:::
::: fragment
Also consider absorption cross section.  
Graphite, heavy water...
:::
</div>
:::
::: {.col2-v}
<img src="cross_section_energy.png" title="https://whatisnuclear.com/barn-jams.html" height=700 alt="image">
:::
:::

# Uranium
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* U-235
    * 0.72% abundance
    * Only natural fissile isotope
    * half life of 703.8 million years
    * $\rho=19.1$ g/cm$^3$ (lead is 11.3)
:::
::: {.col2}
* U-238
    * 99.27% abundance
    * [non-fissile](https://en.wikipedia.org/wiki/Fissile_material#Fissile_vs_fissionable)
    * half life of 4.468 billion years
    * can form Pu-239
:::
:::
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/d/d8/HEUraniumC.jpg/1920px-HEUraniumC.jpg" title="https://upload.wikimedia.org/wikipedia/commons/thumb/d/d8/HEUraniumC.jpg/1920px-HEUraniumC.jpg" height=400 alt="image">
&emsp; &emsp;
<img src="https://upload.wikimedia.org/wikipedia/commons/c/c1/Uranium_ore_square.jpg" title="https://upload.wikimedia.org/wikipedia/commons/c/c1/Uranium_ore_square.jpg" height=400 alt="image">

## Uranium deposits
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* 40 times more common than silver, 500 times more common than gold.
* Found everywhere.
* Highest grade deposits in [Canada](https://en.wikipedia.org/wiki/Athabasca_Basin#Uranium_mines)
:::
::: {.col2-v}
<img src="https://d9-wret.s3.us-west-2.amazonaws.com/assets/palladium/production/s3fs-public/media/images/U_Regions%20Annotated.jpg" title="https://www.usgs.gov" width=800 alt="image">
:::
:::
## US Uranium sources
<img src="uranium_sources.svg" title="data from https://www.eia.gov/energyexplained/nuclear/where-our-uranium-comes-from.php" width=700 alt="image">
<img src="uranium_sources_2.png" title="https://www.eia.gov/energyexplained/nuclear/where-our-uranium-comes-from.php" width=700 alt="image">

## Uranium processing
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<div style="font-size:0.8em;">
* Uranium oxide, dissolved with acid, then precipitated as U$_3$O$_8$ (yellowcake)
* Mined where concentration 0.5-5%
* Mining type
    * underground
    * open pit
    * gold and phosphorus tailings.
    * [In-situ leach (ISL) mining](https://world-nuclear.org/information-library/nuclear-fuel-cycle/mining-of-uranium/in-situ-leach-mining-of-uranium.aspx) (57%)
        * sulfuric acid or sodium bicarbonate
* Enrichment
    * Reaction to UF$_6$ (gas, liquid, solid).
        * reacts with water to form HF, corrosive!
    * [Ultracentrifuge](https://energyeducation.ca/encyclopedia/Gas_centrifuge_for_uranium_enrichment) to separate $^{238}UF_6$ from $^{235}UF_6$ based on density differences.
        * MW = 349, 352 (0.8% different).
        * ~100,000 RPM
</div>
:::
::: {.col2-v}
<img src="https://energyeducation.ca/wiki/images/thumb/8/8c/Gcc.jpg/600px-Gcc.jpg" title="https://energyeducation.ca/wiki/images/thumb/8/8c/Gcc.jpg/600px-Gcc.jpg" height=300 alt="image">
<img src="centrifuge.svg" title="https://en.wikipedia.org/wiki/Gas_centrifuge#/media/File:Countercurrent_Gas_Centrifuge.svg" height=300 alt="image">

<img src="https://www.deepisolation.com/wp-content/uploads/2020/11/image10-1024x793.png" title="https://www.deepisolation.com/wp-content/uploads/2020/11/image10-1024x793.png" height=300 alt="image">
:::
:::

## Uranium reserves
<div style="font-size:0.85em;">
* [8 million tonnes (2019) uranium metal](https://www.iaea.org/newscenter/pressreleases/worlds-uranium-resources-enough-for-the-foreseeable-future-say-nea-and-iaea-in-new-report)
    * "Reasonably assured and inferred" resource
    * Recoverable at market prices 40-260 $US/kgU
    * *From the "red book"*
* [80 years](https://phys.org/news/2011-05-nuclear-power-world-energy.html#:~:text=Uranium%20abundance%3A%20At%20the%20current,for%20less%20than%205%20years.) at current rate of consumption with conventional reactors
* Current reactors (in the U.S.) are "once through." 
* Reprocessing
    * [Gain 25-30%](https://world-nuclear.org/information-library/nuclear-fuel-cycle/fuel-recycling/processing-of-used-nuclear-fuel.aspx) more energy from the original uranium.
    * reduce volume of waste
    * reduce level of radioactivity
* Breeder reactors
    * produce more fuel than they consume
    * U-238 (forming Pu-239), "fast" reactor
    * Th-232 (forming U-233) "thermal" reactor
        * Thorium is 3.5 times as common as uranium.
    * could raise fuel availability 40-50 times

> "It has been estimated that doubling the price of uranium ore, which as mentioned above would increase the cost of the electricity by less than 1 ¢/kWh, would increase the known conventional resources base 10-fold. This increase could easiliy support a much larger (CMO/yr-level) role of nuclear power for several centuries" *--Crane et al., A cubic mile of oil, 2010*.
</div>

# Nuclear reactors
<img src="reactors_types.png" title="https://world-nuclear.org/information-library/nuclear-fuel-cycle/nuclear-power-reactors/nuclear-power-reactors.aspx" width=1400 alt="image">
<p style="font-size:0.8em">
*[world-nuclear.org](https://world-nuclear.org/information-library/nuclear-fuel-cycle/nuclear-power-reactors/nuclear-power-reactors.aspx)*
</p>

## Nuclear reactors: PWR
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* [Pressurized water reactor](https://world-nuclear.org/information-library/nuclear-fuel-cycle/nuclear-power-reactors/nuclear-power-reactors.aspx)
* Pressurized water in contact with fuel
* Water transfers heat and moderates the neutrons
* Nonboiling (high P)
* Heat transfer to separate steam loop
* T: 290 $\rightarrow$ 325 $^oC$
* P: 15 MPa (2250 psi)
:::
::: {.col2-v}
<img src="https://world-nuclear.org/getmedia/fad063be-d367-4e28-b882-d28a170638d7/pressurized-water-reactor-pwr.png.aspx" title="https://world-nuclear.org/information-library/nuclear-fuel-cycle/nuclear-power-reactors/nuclear-power-reactors.aspx" height=700 alt="image">
:::
:::

## Nuclear reactors: PWR
<img src="pwr.png" title="Lamarsh, Introduction to Nuclear Engineering, 3rd ed., p. 138" height=700 alt="image">
&emsp; &emsp;
<img src="pwr_plan.png" title="Steam, 41 ed., p. 46-7" height=500 alt="image">

## Nuclear reactors: PWR
<img src="steam_generator.png" title="Lamarsh, Introduction to Nuclear Engineering, 3rd ed., p. 139" height=700 alt="image">
<img src="pwr_photo.png" title="Lamarsh, Introduction to Nuclear Engineering, 3rd ed., p. 139" height=700 alt="image">

## Nuclear reactors: BWR
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* Boiling water reactor
* Steam is formed directly in the reactor (*direct cycle*)
    * No separate heat transfer loop or steam generators needed.
* Latent vs sensible heat $\rightarrow$ less water flow.
* Water becomes radioactive $\rightarrow$ turbine, pumps, pipes, etc. shielded.
* P: 7 MPA (900 psi)
* T: 290 $^oC$
* Larger unit for same energy vs. PWR; (BWR lower energy per volume)
:::
::: {.col2-v}
<img src="https://www.nrc.gov/images/bwrsm.jpg" title="https://www.nrc.gov/images/bwrsm.jpg" height=700 alt="image">
:::
:::

## Nuclear reactors: PHWR/CANDU
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<div style="font-size:0.8em;">
* Pressurized Heavy Water Reactor/Canadian Deuterium-Uranium
* Use natural, unenriched Uranium
    * Light water absorbs some neutrons requiring enriched U
* Deuterium (heavy water) doesn't absorb thermal neutrons.
    * But less efficient at moderating neutrons $\rightarrow$ longer travel, larger vessel.
    * Also, unenriched fuel has a lower fissile density $\rightarrow$ larger vessel.
* Large pressure vessel is expensive and complex, so the overall reactor is cool, unpressurized,  filled with D$_2$O moderator, but penetrated by horizontal [pressure tubes](https://www.researchgate.net/figure/Current-CANDU-reactor-fuel-channel_fig1_267580730) containing the fuel and coolant with a surrounding CO$_2$ shroud.
    * can be refueled during operation.
* P: 8 MPA (1285 psi)
* T: [~305 $^oC$](http://large.stanford.edu/courses/2013/ph241/kallman1/docs/nuclear_reactors.pdf)
* Indirect steam cycle
</div>
:::
::: {.col2-v}
<img src="candu.png" title="Steam, 41 ed., p. 46-6" height=800 alt="image">
:::
:::
::: notes
* safety: 
    * careful alignment is needed. If tubes overheat, they bend, throwing off the alignment.
    * add lightwater --> slows reaction as water absorbs neutrons
:::

## Nuclear reactors: PHWR/CANDU
<iframe width="1422" height="800" src="https://www.youtube.com/embed/wzhIAjqDE3o?cc_load_policy=1" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>

## Nuclear reactors: AGR
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::: {.col2-l}
* Advanced Gas Reactor
* CO$_2$ cooled
    * non-reactive with fuel or moderator, non-absorbing
    * not pressurized
* [Graphite moderated](https://energyeducation.ca/encyclopedia/Neutron_moderator)
* enriched U-235 (2.5-3.5%)
* T: 650 $o^C$.
    * Higher efficiencies: 41%
* Indirect steam but heat transfer internal to the reactor vessel.
:::
::: {.col2-v}
<img src="https://explorenuclear.com/wp-content/uploads/2023/12/AGR.png" title="https://explorenuclear.com/wp-content/uploads/2023/12/AGR.png" height=700 alt="image">
:::
:::

## Nuclear plant tour
<iframe width="1422" height="800" src="https://www.youtube.com/embed/_AdA5d_8Hm0" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>

# Economics
* Dominated by capital costs
* Fuel costs are around 15% of the cost of the power
    * Compared to 30% and 70% for coal and NG (~2006)
* Time to complete
    * Gas-fired: 2 years
    * Coal-fired: 2-4 years
    * Nuclear: 3-5 or more years
* Each nuclear plant is one-of-a-kind
    * Lack of standardization, contributes to long approval process
* Prices of steel and concrete
    * Headline: "Steel prices are up 219% since early 2020. What to expect next"
        * [fortune.com](https://fortune.com/2021/08/16/steel-prices-2021-covid-commodities-lumber-costs/) August 16, 2021

## Economics
<img src="https://upload.wikimedia.org/wikipedia/commons/thumb/a/af/20201019_Levelized_Cost_of_Energy_%28LCOE%2C_Lazard%29_-_renewable_energy.svg/2560px-20201019_Levelized_Cost_of_Energy_%28LCOE%2C_Lazard%29_-_renewable_energy.svg.png" title="https://en.wikipedia.org/wiki/Levelized_cost_of_energy" width=1200 alt="image">

<a href="https://en.wikipedia.org/wiki/Cost_of_electricity_by_source" style="color:black;">
<div style="font-size:0.8em;">
>"The levelized cost of energy (LCOE) is a measure of a power source that allows comparison of different methods of electricity generation on a consistent basis. The LCOE can also be regarded as the minimum constant price at which electricity must be sold in order to break even over the lifetime of the project."
</div>
</a>

::: notes
* [Gas (peaker)](https://en.wikipedia.org/wiki/Peaking_power_plant) are plants that only run on high demand so have a high cost per kWh
* This plot will explain some of the increasing wind, solar, and natural gas plants
:::



# Radiation exposure: units
<div style="font-size:0.9em; max-width:90%; padding-left:50px;">
* Energy: electron-Volt (eV); 1 eV = 1.60218E-19 J
* Decay rate 
    * curie Ci; 1 Ci = 3.7E10 decays per second
    * becquerel Bq; 1 Bq = 1 decay per second
* Ionization producted: roentgen R
    * 1 electrostatic unit (3.33E-10 coul) of charge of one sign from the interaction of $\gamma$ radiation in 0.001293 g of air (or 1 cm$^3$ of air at 1 atm and O $^oC$)
    * 1 R = $2.58\times 10^{-4}$ coul/kg.
* Absorbed dose
    * rad (radiation absorbed dose)
        * 1 rad = 0.01 J/kg = 100 ergs/g
    * **gray Gy (SI unit)**
        * 1 Gy = 1 J/kg = 100 rads
* Equivalent dose
    * Absorbed dose is not as useful as how much harm it causes.
    * Harm depends on: amount of radiation imparted, type of radiation, part of the body exposed 
    * [video](https://www.youtube.com/watch?v=vRYwUPBZ-J4), [video](https://www.youtube.com/watch?v=MpQzhZ0RRDM)
    * multiply grays by a modification factor.
    * rem (roentgen equivalent man)
    * **sievert Sv (SI unit)**
        * 1 Sv = 100 rem
</div>

## Radiation quality factors
<img src="quality_factors.png" title="Lamarsh, Introduction to Nuclear Engineering, 3rd ed., 473. 139" height=800 alt="image">

$$Sv = Gy \cdot W_R$

::: notes
Q is quality factor (related to $W_R$)
:::



## Radiation dose
<iframe src="https://xkcd.com/radiation/" width=1200 height=800></iframe>

# Nuclear Regulatory Commission
<iframe width="1422" height="800" src="https://www.youtube.com/embed/kZYQtSJEIIg" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture" allowfullscreen></iframe>


