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| 70 | +
|
| 71 | +\title{Nucleonics} |
| 72 | + \author{Matt Lilley} |
| 73 | + \date{\today} % Default to today if no date is provided |
| 74 | +
|
| 75 | +\begin{document} |
| 76 | +\maketitle |
| 77 | +
|
| 78 | +\section{What is nucleonics?}\label{what-is-nucleonics} |
| 79 | +
|
| 80 | +\begin{quote} |
| 81 | +\textbf{Nucleonics is a scientific and engineering discipline that |
| 82 | +studies and applies the principles of physics to design, create, and |
| 83 | +operate devices that manipulate nucleons.} |
| 84 | +\end{quote} |
| 85 | +
|
| 86 | +We take inspiration from the emergence of electronics that marked a |
| 87 | +fundamental shift in humanity's relationship to information. Underlying |
| 88 | +that shift was a revolution in the way we understood and interacted with |
| 89 | +electrons: rather than continuing to blow large aggregates of electrons |
| 90 | +through vacuum tubes, the transistor represented deliberate, precise |
| 91 | +control of electronic states. |
| 92 | +
|
| 93 | +What if, similar to our control of electronic states, we gained precise |
| 94 | +control of nuclear states? Before we can answer that question, it's |
| 95 | +essential to first ask the ``Is it possible?'' question. |
| 96 | +
|
| 97 | +Some of the essential physics of nucleonics (e.g.~nuclear superradiance) |
| 98 | +was already proposed in |
| 99 | +\href{https://doi.org/10.1103/physrevlett.14.589}{1965 by Terhune and |
| 100 | +Baldwin}, but it's only in recent years that it's been possible to |
| 101 | +verify those ideas - see |
| 102 | +\href{https://www.nature.com/articles/s41567-017-0001-z}{Chumakov et.al |
| 103 | +2017}. We're now seeing increased interest and experimental progress in |
| 104 | +the controlling of nuclear states |
| 105 | +e.g.~\href{https://www.science.org/doi/10.1126/sciadv.abc3991}{Bocklage |
| 106 | +et.al 2021} , |
| 107 | +\href{https://www.nature.com/articles/s41586-021-03276-x}{Heeg et.al |
| 108 | +2021}, and |
| 109 | +\href{https://www.nature.com/articles/s41567-024-02773-w}{Chai et.al |
| 110 | +2025}. |
| 111 | +
|
| 112 | +The answer seems to be yes - nucleonics is possible. Now to the question |
| 113 | +of ``What if?''. |
| 114 | +
|
| 115 | +\section{A vision for nucleonics}\label{a-vision-for-nucleonics} |
| 116 | +
|
| 117 | +What if, similar to our control of electronic states, we gained precise |
| 118 | +control of nuclear states? We might imagine a world where nuclear |
| 119 | +radiation is a thing of the past or a world where we can increase |
| 120 | +nuclear fusion rates in solid states to technologically relevant levels. |
| 121 | +
|
| 122 | +There are other possible visions for nucleonics, e.g.~one might take an |
| 123 | +information technology angle relating to nuclear spintronics. However, |
| 124 | +our vision takes an energy angle. We can recast the vision into a |
| 125 | +``mission statement'' |
| 126 | +
|
| 127 | +\begin{quote} |
| 128 | +\textbf{We want to enable rational engineering of small-scale devices |
| 129 | +fueled by clean nuclear energy} |
| 130 | +\end{quote} |
| 131 | +
|
| 132 | +Now that we have a ``destination'', how are we going to get there? Are |
| 133 | +there any potential roadblocks along the way? We need a roadmap. |
| 134 | +
|
| 135 | +\section{Nucleonics Roadmap}\label{nucleonics-roadmap} |
| 136 | +
|
| 137 | +To meet the vision, we need nucleonics to be more than possible, we need |
| 138 | +it to be practical and so the essential question that a nucleonics |
| 139 | +roadmap is answering is: |
| 140 | +
|
| 141 | +\begin{quote} |
| 142 | +\textbf{Is nucleonics practical?} |
| 143 | +\end{quote} |
| 144 | +
|
| 145 | +It may be that manipulating nuclear states for the purposes of energy |
| 146 | +technology is sufficiently difficult to make it more of an academic |
| 147 | +curiosity than an enabler of new technology. |
| 148 | +
|
| 149 | +From the energy perspective that our mission statement focusses on, |
| 150 | +practicality means that we need to be able to: |
| 151 | +
|
| 152 | +\begin{itemize} |
| 153 | +\tightlist |
| 154 | +\item |
| 155 | + Accelerate nuclear transitions by many orders of magnitude |
| 156 | +\item |
| 157 | + Transfer nuclear energy from one type of nucleus to another |
| 158 | +\item |
| 159 | + Control nuclear transitions with low frequency stimulation |
| 160 | +\item |
| 161 | + Extract nuclear energy in benign forms |
| 162 | +\end{itemize} |
| 163 | +
|
| 164 | +From a theoretical perspective, nucleonics does seem practical. In 2024, |
| 165 | +\href{https://arxiv.org/pdf/2501.08338}{Hagelstein et.al} showed for the |
| 166 | +first time that known quantum physics principles could be applied to |
| 167 | +satisfy the above criteria and moreover explain long standing |
| 168 | +experimental nuclear anomalies found in LENR experiments. |
| 169 | +
|
| 170 | +Hagelstein's theoretical framework relies on combining several pieces of |
| 171 | +well established quantum physics in a novel way. The central question is |
| 172 | +whether Mother Nature respects this novel combination. The framework |
| 173 | +needs to be stress tested in several carefully designed experiments in |
| 174 | +order to pass the ultimate litmus test. |
| 175 | +
|
| 176 | +\subsection{Accelerating nuclear transitions by many orders of |
| 177 | +magnitude}\label{accelerating-nuclear-transitions-by-many-orders-of-magnitude} |
| 178 | +
|
| 179 | +One of the key bit of physics responsible for accelerating nuclear |
| 180 | +transitions is Dicke Superradiance. First proposed by |
| 181 | +\href{https://doi.org/10.1103/PhysRev.93.99}{Dicke in the 1950s} for |
| 182 | +atoms and then extended by |
| 183 | +\href{https://doi.org/10.1103/physrevlett.14.589}{Terhune and Baldwin in |
| 184 | +the 1960s} for nuclei, Dicke's model showed that \(N\) particles can |
| 185 | +radiate/decay collectively up to \(N^2\) faster that an individual |
| 186 | +particle. In a solid lattice, the number density is |
| 187 | +\(\sim 10^{28} \ \rm m^{-3}\) and so Dicke enhancements can in principle |
| 188 | +be extremely large. |
| 189 | +
|
| 190 | +The challenge for nuclear superradaince is how close the nuclei need to |
| 191 | +be for collective emission to occur. Dicke's model is based on all \(N\) |
| 192 | +nuclei being coupled together through an interaction with a common |
| 193 | +oscillating field. In order to get the full \(N^2\) enhancement, all the |
| 194 | +nuclei need to be located within a single wavelength of one other. The |
| 195 | +wavelength is determined by the frequency (and hence energy) of the |
| 196 | +field oscillations. Typically the frequency is chosen to be matched to |
| 197 | +the nuclear transitions which mostly have energies of |
| 198 | +\(E > 10 \ \rm keV\) and wavelengths of \(\lambda < 0.1 \ \rm nm\). In a |
| 199 | +typical solid lattice you can fit at most one particle in cube whose |
| 200 | +sides are given by such a small wavelength. |
| 201 | +\href{https://www.nature.com/articles/s41567-017-0001-z}{Chumakov et.al |
| 202 | +2017} achieved small levels of nuclear superradiance (\(\sim 10 \times\) |
| 203 | +rate enhancements) in \(\rm ^{57}Fe\) experiments because of this. |
| 204 | +
|
| 205 | +Much larger Dicke enhancement rates are required for practical |
| 206 | +applications. Bridging the rate enhancement gap can in principle be |
| 207 | +achieved by choosing a low frequency (and hence long wavelength) that's |
| 208 | +mismatched with respect to the nuclear transitions. In such a set-up, a |
| 209 | +nucleus radiates a number of smaller energy oscillator quanta instead of |
| 210 | +a single large one. The challenge with this approach is that the more |
| 211 | +quanta that are involved, the slower the process becomes - this can |
| 212 | +dominate over Dicke enhancements depending on the specific details. |
| 213 | +
|
| 214 | +There is a novelty in demonstrating Dicke enhancements with oscillator |
| 215 | +and nuclei that are mismatched. It would therefore be preferable to |
| 216 | +separate that novelty from the specific demonstration of extremely large |
| 217 | +nuclear Dicke enhancements. One way to do this is to repeat the Chumakov |
| 218 | +experiment but instead of using \(\rm ^{57}Fe\) we use |
| 219 | +\href{https://en.wikipedia.org/wiki/Isotopes_of_thorium\#Thorium-229m}{\(\rm ^{229m}Th\)}. |
| 220 | +
|
| 221 | +\(\rm ^{229}Th\) has a nuclear isomer \(\rm ^{229m}Th\) whose existence |
| 222 | +was hypothesised for many years but |
| 223 | +\href{https://link.springer.com/article/10.1140/epjs/s11734-024-01098-2}{was |
| 224 | +only nailed down in 2024}. \(\rm ^{229m}Th\) is unique in that it has an |
| 225 | +extremely low energy nuclear transition energy of \(8.36 \ \rm eV\) |
| 226 | +which corresponds to a wavelength of \(148 \ \rm nm\). A cube of this |
| 227 | +size would contain about \(3\times 10^7\) nuclei at typical solid |
| 228 | +density - more than enough to observe some very large Dicke |
| 229 | +enhancements. |
| 230 | +
|
| 231 | +The specifics of \(\rm ^{229m}Th\) require us to arrange the system to: |
| 232 | +
|
| 233 | +\begin{itemize} |
| 234 | +\tightlist |
| 235 | +\item |
| 236 | + Maximise radiative decay over internal conversion |
| 237 | +
|
| 238 | + \begin{itemize} |
| 239 | + \tightlist |
| 240 | + \item |
| 241 | + Excite half of the \(\rm ^{229m}Th\) nuclei instead of all of them |
| 242 | + will give us \(N^2\) enhancement of radiation and only \(N/2\) |
| 243 | + enhancement of internal conversion |
| 244 | + \end{itemize} |
| 245 | +\item |
| 246 | + Minimise the reflection of the UV laser light from the surface |
| 247 | +
|
| 248 | + \begin{itemize} |
| 249 | + \tightlist |
| 250 | + \item |
| 251 | + Embed the \(\rm ^{229m}Th\) into an UV transparent material |
| 252 | + \end{itemize} |
| 253 | +\end{itemize} |
| 254 | +
|
| 255 | +\printbibliography |
| 256 | +
|
| 257 | +
|
| 258 | +\end{document} |
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