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{\displaystyle \{{\alpha },\beta ,\mathbb {N} ,\alpha \%\},then=(\alpha \uparrow ...(\beta \uparrow 's)...\uparrow \mathbb {N} )\uparrow \alpha \%}
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{\displaystyle \{\alpha ,\beta ,[\mathbb {N} ],\alpha \$\}\equiv \{\alpha ,\alpha ,\mathbb {N} ,\beta \%\},\%,\$\simeq 0.(\mathbb {N} )\uparrow \alpha }
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{\displaystyle \{10,\delta ,[5],7\}=10\{\{\{\{\{7\}\}\}\}\}\delta ,\delta =\alpha \%/\$~(opt.)}
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{\displaystyle \mathbb{N}}
{10^100, 10^100, [10^10^10^100&], 10$} (Limit of GEAF) is the point where the lightstein's rule (in finite numbers) gets unstable, going further from this point will not result in a valid value
Googology Wiki
![{\displaystyle \{\alpha ,\beta ,[\mathbb {N} ],\alpha \$\}\equiv \{\alpha ,\alpha ,\mathbb {N} ,\beta \%\},\%,\$\simeq 0.(\mathbb {N} )\uparrow \alpha }](https://services.fandom.com/mathoid-facade/v1/media/math/render/svg/3201de9af084a8b3f0831ba0d1397a449b88cd93)
![{\displaystyle \{10,\delta ,[5],7\}=10\{\{\{\{\{7\}\}\}\}\}\delta ,\delta =\alpha \%/\$~(opt.)}](https://services.fandom.com/mathoid-facade/v1/media/math/render/svg/32754eed67d71613598eff8d4443801f2b0969aa)
