Talk:Square-free integer

Square-free → Square-free integer

Maybe this should really be Square-free integer? -- Walt Pohl 01:40, 2 March 2004 (UTC)

The separable polynomial page does use the term more generally.

Charles Matthews 08:17, 2 March 2004 (UTC)

There's now a square-free polynomial page, too. I've changed the separable polynomial page to link there instead of here.

Baccala@freesoft.org 06:28, 23 January 2006 (UTC)

We have a lot of equivalent characterizations already,

I know, but here's another:The number of divisors of a squarefree integer is a power of two.Rich 06:55, 1 November 2006 (UTC)

How about 8? Its 4=2^2 factors are 1, 2, 4 and 8, but it is not square-free. 128.101.10.146 23:22, 7 June 2007 (UTC)

Indeed. Having a number of divisors that is a power of two is a necessary, but not sufficient, condition for being squarefree. Doctormatt 23:39, 7 June 2007 (UTC)

Loop quantum gravity section

That section does not make much sense. There is something crucial missing from the formulas, but I suspect that it masks a conceptual misapprehension. Is this saying more than "any integer $a$ can be uniquely represented as $a=n^{2}\zeta ,$ where $\zeta$ is square-free"? What is the mathematical statement there, and what is result of some experimental spetroscopy? Unless someone comes up with a really compelling reason, I would propose to remove (or at least move) this section from the article. Arcfrk 07:32, 10 March 2007 (UTC)

I have moved the whacky section from the main text to here. Arcfrk 22:28, 23 March 2007 (UTC)

Application in Loop Quantum Gravity

In the theory of loop quantum gravity area is an observable operator. As a consequence, the area of a quantum surface is quantized. Abhay Ashtekar and his colleagues in 1996 found that three incident edges of spins j₁, j₂, and j₃ at a trivalent vertex generate the patch of area:

$a=\ell _{P}^{2}{\sqrt {2j_{1}(j_{1}+1)+2j_{2}(j_{2}+1)-j_{3}(j_{3}+1)}},$

where $\ell _{P}$ is the Planck length.

The spectroscopy of a canonically quantized black hole showed that the area eigenvalue formula fits into the following reduced formula

$\forall n\in N,a=\ell _{P}^{2}n{\sqrt {2\zeta }}$

(subject to the identification of repeated numbers) where $\zeta$ is a square-free number and $\{\zeta \}=$ the set of all square-free numbers.

This helps to expect that black hole Hawking radiation is concentraited on a few lines whose energy is proportional to the square root of square-free numbers.

References

• Spectroscopy of a Canonically Quantized Black Hole

— Preceding unsigned comment added by Arcfrk (talk • contribs) 22:28, 23 March 2007 (UTC)

There is a proof in the reference for this. As far as I learn, the proof is simple and neat anyway. Any number is decomposed into its prime numbers, each to an odd or even power. The even power comes up to make a square number, the odd factors make up a square-free number. (129.97.58.55 22:31, 26 March 2007 (UTC))

Square-free test

Is it known something about the complexity of testing if an integer is square-free? Maybe some relation with Primality test. 193.144.198.250 (talk) 11:28, 11 March 2014 (UTC)

1 as a squarefree integer

I cannot understand: whether today any mathematicians consider squarefree numbers without 1 or not. Is it possible (for contemporary scientists) to define "squarefree number" as "a number that is the product of integer number of different primes"? --Tamtam90 (talk) 22:06, 5 August 2017 (UTC)

Square free numbers may be defined as products of primes that are all different. This definition is equivalent with the one that is given in the first sentence of the article, as 1 is the empty product of primes. Thus, presently, 1 is always defined to be square free. D.Lazard (talk) 08:30, 6 August 2017 (UTC)

Thank you for your answer. I think I'd ask about this subject Mr. John Derbyshire and Mr. Dennis Hejhal. --Tamtam90 (talk) 23:57, 7 August 2017 (UTC)