<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JHEPGC</journal-id><journal-title-group><journal-title>Journal of High Energy Physics, Gravitation and Cosmology</journal-title></journal-title-group><issn pub-type="epub">2380-4327</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jhepgc.2021.73062</article-id><article-id pub-id-type="publisher-id">JHEPGC-110381</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Looking at Quantization of a Wave Function, from Weber (1961), to Signals from Wavefunctions at the Mouth of a Wormhole
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Andrew</surname><given-names>Beckwith</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Physics Department, College of Physics, Chongqing University, Chongqing, China</addr-line></aff><pub-date pub-type="epub"><day>03</day><month>06</month><year>2021</year></pub-date><volume>07</volume><issue>03</issue><fpage>1037</fpage><lpage>1048</lpage><history><date date-type="received"><day>4,</day>	<month>June</month>	<year>2021</year></date><date date-type="rev-recd"><day>4,</day>	<month>July</month>	<year>2021</year>	</date><date date-type="accepted"><day>7,</day>	<month>July</month>	<year>2021</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  We utilize how Weber in 1961 initiated the process of quantization of early universe fields to the problem of what may be emitted at the mouth of a wormhole. While the wormhole models are well developed, there is as of yet no consensus as to how, say GW or other signals from a wormhole mouth could be quantized or made to be in adherence to a procedure Weber cribbed from Feynman, in 1961. In addition, we utilize an approximation for the Hubble parameter parameterized from Temperature using Sarkar’s H ~ Temperature relations, as given in the text. Finally, after doing this, we go to the Energy as E also ~ Temperature, and from there use E (energy) as ~ signal frequency. This gives us an idea of how to estimate frequency generated at the mouth of a wormhole.
 
</p></abstract><kwd-group><kwd>Minimum Scale Factor</kwd><kwd> Cosmological Constant</kwd><kwd> Space-Time Bubble</kwd><kwd>  Bouncing Cosmologies</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>We bring up this study first a result given by Weber, in 1961 [<xref ref-type="bibr" rid="scirp.110381-ref1">1</xref>] as to getting an initial wavefunction given in [<xref ref-type="bibr" rid="scirp.110381-ref2">2</xref>], which may be able to model behavior of what happens in the mouth of a wormhole if we make the assumption given in [<xref ref-type="bibr" rid="scirp.110381-ref3">3</xref>] that H (Hubbles parameter) is proportional to Temperature, and then go to Energy ~ Temperature. The last part will be enough to isolate, up to first principles a net frequency value.</p><p>The behavior of frequency, versus certain conditions at the mouth of a wormhole may give us clues to be investigated later as to polarization states relevant to the wormhole [<xref ref-type="bibr" rid="scirp.110381-ref4">4</xref>] as well as examining what may be relevant to measurement of signals from a wormhole [<xref ref-type="bibr" rid="scirp.110381-ref5">5</xref>].</p><p>In doing all of this, the idea is that we are evolving from the Einstein-Rosen bridge to a more complete picture of GR which may entail a new representation of the Visser “Chronology protection” paper as in [<xref ref-type="bibr" rid="scirp.110381-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref7">7</xref>].</p></sec><sec id="s2"><title>2. Looking at the Weber Book as to Reformulate Quantization Imposed in GR</title><p>Using [<xref ref-type="bibr" rid="scirp.110381-ref1">1</xref>] a statement as to quantization for a would be GR term comes straight from:</p><p>Ψ Later = ∫ ∑ H e ( i I H / ℏ ) ( t , t 0 ) Ψ Earlier ( t 0 ) d t 0 (1)</p><p>The approximation we are making is to pick one index, so as to have:</p><p>Ψ Later = ∫ ∑ H e ( i I H / ℏ ) ( t , t 0 ) Ψ Earlier ( t 0 ) d t 0 → H → 1 ∫ e ( i I H FIXED / ℏ ) ( t , t 0 ) Ψ Earlier ( t 0 ) d t 0 (2)</p><p>This corresponds to say being primarily concerned as to GW generation, which is what we will be examining in our ideas, via using:</p><p>e ( i I H FIXED / ℏ ) ( t , t 0 ) = exp [ i ℏ ⋅ c 4 16 π G ⋅ ∫ Μ d t ⋅ d 3 r − g ⋅ ( ℜ − 2 Λ ) ] (3)</p><p>We will use the following, namely, if Λ is a constant, do the following for the Ricci scalar [<xref ref-type="bibr" rid="scirp.110381-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref9">9</xref>],</p><p>ℜ = 2 r 2 (4)</p><p>If so then we can write the following, namely: Equation (3) becomes, if we have an invariant Cosmological constant, so we write Λ → alltime Λ 0 everywhere, then,</p><p>e ( i I H FIXED / ℏ ) ( t , t 0 ) = exp [ i ℏ ⋅ c 4 ⋅ π ⋅ t 0 16 G ⋅ ( r − r 3 Λ 0 ) ] (5)</p><p>Then, we have that Equation (1) is rewritten to be:</p><p>Ψ Later = ∫ ∑ H e ( i I H / ℏ ) ( t , t 0 ) Ψ Earlier ( t 0 ) d t 0 → at wormhole ∫ exp [ i ℏ ⋅ c 4 ⋅ π ⋅ t 0 16 G ⋅ ( r − r 3 Λ 0 ) ] Ψ Earlier ( t 0 ) d t 0 (6)</p></sec><sec id="s3"><title>3. Examining the Behavior of the Earlier Wavefunction in Equation (6)</title><p>[<xref ref-type="bibr" rid="scirp.110381-ref2">2</xref>] states a Hartle-Hawking wavefunction which we will adapt for the earlier wavefunction as stated in Equation (6) so as to read as follows:</p><p>Ψ Earlier ( t 0 ) ≈ Ψ H H ∝ exp ( − π 2 G H 2 ⋅ ( 1 − sinh ( H t ) ) 3 / 2 ) (7)</p><p>Here, making use of Sarkar [<xref ref-type="bibr" rid="scirp.110381-ref3">3</xref>], we set, if say g ∗ is the degree of freedom allowed [<xref ref-type="bibr" rid="scirp.110381-ref9">9</xref>],</p><p>H = 1.66 g ∗ T temp 2 / M Planck (8)</p><p>We assume initially a relatively uniformly given temperature, that H is constant.</p><p>So then we will be attempting to write out an expansion as to what Equation (6) gives us while we use Equation (7) and Equation (8), with H approximately constant.</p></sec><sec id="s4"><title>4. Methods Used in Calculating Equation (6), with Interpretation of the Results</title><p>We will be considering how to express Equation (6) and in doing this we will be looking at having a constant value for Equation (8). If so then,</p><p>Ψ Later = ∫ exp [ i ℏ ⋅ c 4 ⋅ π ⋅ t 0 16 G ⋅ ( r − r 3 Λ 0 ) ] exp ( − π 2 G H 2 ⋅ ( 1 − sinh ( H t ) ) 3 / 2 ) d t 0 (9)</p><p>Then using numerical integration, [<xref ref-type="bibr" rid="scirp.110381-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref12">12</xref>] on page 751 of this [<xref ref-type="bibr" rid="scirp.110381-ref12">12</xref>] citation:</p><p>Ψ Later → t M → ε + ∫ 0 t M e i ⋅ ( α ˜ 1 ) ⋅ t − ( α ˜ 2 ) ⋅ ( 1 − sinh ( H t ) ) 3 / 2 d t ≈ t M 2 ⋅ ( e i ⋅ ( α ˜ 1 ) ⋅ t M − ( α ˜ 2 ) ⋅ ( 1 − sinh ( H ⋅ t M ) ) 3 / 2 − 1 ) α ˜ 1 = [ c 4 ⋅ π 16 G ℏ ⋅ ( r − r 3 Λ 0 ) ] ,     α ˜ 2 = π 2 G H 2 (10)</p><p>Notice the terms for the H factor, and from here we will be making our prediction.</p><p>If the energy, E, has the following breakdown,</p><p>H = 1.66 g ∗ T temp 2 / M Planck ⇒ E ≈ k B T Temp ≈ ℏ ⋅ ω signal ⇒ ω signal ≈ k B ⋅ M Planck H ℏ ⋅ 1.66 g ∗ (11)</p><p>The upshot is that we have, in this, a way to obtain a signal frequency by looking at the real part of Equation (11) above, if we have a small t, initially (small time step).</p></sec><sec id="s5"><title>5. How to Compare with a Kieffer Solution and Thereby Isolate the Cosmological Constant Contribution</title><p>Equation (11) would imply an initial frequency dependence. What we are doing next is to strategize as to understand the contribution of the cosmological constant in this sort of problem. I.e., the way to do it would be to analyze a Kieffer “dust solution” as a signal from the Wormhole. I.e., look at [<xref ref-type="bibr" rid="scirp.110381-ref13">13</xref>], where we assume that t, would be in this case the same as in Equation (10) above. I.e. in this case we will write having</p><p>Δ ω signal Δ t ≈ 1 (12)</p><p>If so then we can assume, that the time would be small enough so that:</p><p>Δ t ≈ ℏ 1.66 g ∗ k B ⋅ M Planck H (13)</p><p>If Equation (13) is of a value somewhat close to t, in terms of general initial time, we can write</p><p>ψ n ˜ , λ ( t , r ) ≡ 1 2 π ⋅ n ˜ ! ⋅ ( 2 λ ) n ˜ + 1 / 2 ( 2 n ˜ ) ! ⋅ [ 1 ( λ + i ⋅ t + i ⋅ r ) n ˜ + 1 − 1 ( λ + i ⋅ t − i ⋅ r ) n ˜ + 1 ] (14)</p><p>Here the time t would be proportional to Planck time, and r would be proportional to Planck length, whereas we set</p><p>λ ≈ 8 π G V volume ℏ 2 t 2 → G = ℏ = l Planck = k B = 1 8 π t 2 ≡ 8 π t (15)</p><p>Then a preliminary emergent space-time wavefunction would take the form of:</p><p>ψ n ˜ , λ ( Δ t , r ) ≡ 1 2 π ⋅ n ˜ ! ⋅ ( 2 ⋅ 8 π ⋅ ( Δ t ) − 1 ) n ˜ + 1 / 2 ( 2 n ˜ ) ! ⋅ [ 1 ( 8 π ⋅ ( Δ t ) − 1 + i ⋅ Δ t + i ⋅ r ) n ˜ + 1 − 1 ( 8 π ⋅ ( Δ t ) − 1 + i ⋅ Δ t − i ⋅ r ) n ˜ + 1 ] (16)</p><p>Just at the surface of the bubble of space-time, with t Planck ∝ Δ t , and r ∝ l Planck .</p><p>This is from a section, page 239 of the 3<sup>rd</sup> edition of Kieffer’s book, as to a quantum theory of collapsing dust shells. And so then we have the following procedure as to isolate out the contribution of the Cosmological constant. Namely, take the real part of Equation (16) and compare it with the Real part of Equation (10).</p><p>Another way to visualize this situation, and this is a different way to interpret Equation (15). To do so we examine looking at page 239 of Kieffer, namely [<xref ref-type="bibr" rid="scirp.110381-ref13">13</xref>] where one has an expectation value to energy we can write as</p><p>〈 E 〉 κ = n , λ = ( κ = n ) + 1 / 2 λ → λ ≈ 1 / ℏ ω ℏ ω ⋅ ( ( κ = n ) + 1 / 2 ) (17)</p><p>What we can do, is to ascertain the last step would be to make Equation (16) in a sense partly related to the simple harmonic oscillator. But we should take into consideration the normalization using that if ℏ = l P = G = t P = k B = 1 is done via Plank unit normalization [<xref ref-type="bibr" rid="scirp.110381-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref15">15</xref>]. If so, then we have that frequency is proportional to 1/t, where t is time. I.e. hence if there is a value of n = 0 and making use of the frequency, we then would be able to write Equation (16) as</p><p>Ψ 1 , κ = n = 0 ≈ ω π ⋅ [ 1 ω + i ⋅ ( t + r ) − 1 ω + i ⋅ ( t − r ) ] (18)</p><p>Or,</p><p>Ψ 2 , κ = n = 0 ≈ 1 π 8 π t ⋅ [ 1 8 π t + i ⋅ ( t + r ) − 1 8 π t + i ⋅ ( t − r ) ] (19)</p><p>With, say</p><p>ω ≈ 8 π t (20)</p><p>And this in a setting where we have the dimensional reset of Planck Units [<xref ref-type="bibr" rid="scirp.110381-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref15">15</xref>],</p><p>ℏ = l P = G = t P = k B = 1 (21)</p></sec><sec id="s6"><title>6. Formal Bounding of the Cosmological Constant, in Terms of Two Wavefunctions Plus Analysis of Initial Wormhole Frequency Values</title><p>To do this we, first of all, consider the real part of Equation (18) when n is set equal to zero, and the state should be the same as the real part of Equation (10). Then do the same with the real part of Equation (19) and compare it with Equation (10) in order to isolate out a bound to the cosmological constant.</p><p>Doing so, leads to the following situation, and keep in mind that we are using Equation (21) for regularization as well as setting</p><p>r ≡ B ⌢ ⋅ r P → r P → 1 B ⌢ (22)</p><p>If so, then we have the following bounding as far as the value of the cosmological “constant”, namely,</p><p>Ψ Later → t M → ε + ∫ 0 t M e i ⋅ ( α ˜ 1 ) ⋅ t − ( α ˜ 2 ) ⋅ ( 1 − sinh ( H t ) ) 3 / 2 d t ≈ t M 2 ⋅ ( e i ⋅ ( α ˜ 1 ) ⋅ t M − ( α ˜ 2 ) ⋅ ( 1 − sinh ( H ⋅ t M ) ) 3 / 2 − 1 ) Ψ 1 , κ = n = 0 ≈ ω π ⋅ [ 1 ω + i ⋅ ( t + r ) − 1 ω + i ⋅ ( t − r ) ] α ˜ 1 = [ c 4 ⋅ π 16 G ℏ ⋅ ( r − r 3 Λ 0 ) ] ,     α ˜ 2 = π 2 G H 2 (23)</p><p>We will be looking at comparing the real values of Equation (23) in order to obtain a bound on the cosmological constant, and in doing so we have employing the following Equation (11), Equation (20), Equation (21), Equation (22) and Equation (23) in order to get a bound on the Cosmological constant as given by:</p><p>Λ 0 ≈ B ˜ − 2 − 16 π ⋅ B ˜ − 2 ⋅ ( α ˜ 2 ⋅ ( 1 − sinh ( H ⋅ B ˜ ) ) 3 / 2 )                 − 16 π ⋅ B ˜ − 2 ⋅ cos − 1 [ 2 ⋅ 8 3 / 4 ⋅ π 1 / 4 8 π + ( 1 + B ˜ ) 2 − 2 ⋅ 8 3 / 4 ⋅ π 1 / 4 8 π + ( 1 − B ˜ ) 2 ] (24)</p><p>In doing this, taking into account the Planck units and their normalization, we also need to keep in consideration the frequency, which we will denote here as:</p><p>ω signal ≈ k B ⋅ M Planck H ℏ 1.66 g ∗ → ℏ = l P = G = t P = k B = 1 H 1.66 g ∗ ≈ T temperature 2 (25)</p><p>Whereas what we will be doing, after we obtain a frequency of a signal near the mouth of a wormhole is to use the following scaling of frequency, near Earth Orbit from this wormhole. First if the wormhole is right at the start of the Universe [<xref ref-type="bibr" rid="scirp.110381-ref8">8</xref>], we use:</p><p>( 1 + z initial era ) ≡ a today a initial era ≈ ( ω Earth orbit ω initial era ) − 1 ⇒ ( 1 + z initial era ) ω Earth orbit ≈ 10 25 ω Earth orbit ≈ ω initial era (26)</p><p>If we are say far closer to the Earth, or the Solar system, then we would likely see [<xref ref-type="bibr" rid="scirp.110381-ref8">8</xref>]</p><p>10 ⋅ ω Earth orbit signal ≈ ω wormhole mouth signal (27)</p><p>Our derivation so far is to obtain the initial signal frequency for Equation (26) and Equation (27). Our next task is to obtain some considerations as to the Polarization, of say GW to observe and look for, in conclusion of this document.</p></sec><sec id="s7"><title>7. The Big Picture, Polarization of Signals from a Wormhole Mouth May Affect GW Astronomy Investigations</title><p>We will be referencing [<xref ref-type="bibr" rid="scirp.110381-ref16">16</xref>] and [<xref ref-type="bibr" rid="scirp.110381-ref17">17</xref>], i.e. for [<xref ref-type="bibr" rid="scirp.110381-ref16">16</xref>] we have a rate of production from the wormhole mouth we can quantify as</p><p>Γ ≈ exp ( ω signal / T temperature ) (28)</p><p>Whereas we have from [<xref ref-type="bibr" rid="scirp.110381-ref17">17</xref>] a probability for “scalar” particle production from the wormhole given by</p><p>Γ ≈ exp ( − E / T temperature ) (29)</p><p>Whereas if we assume that there is a “negative temperature in Equation (28) and say rewrite Equation (29) as obeying having:</p><p>( ω signal / T temperature ) ≈ ( − E / T temperature ) (30)</p><p>This is specifying a rate of particle production from the wormhole. And so then, whereas what we are discussing in Equation (28) and Equation (29) is having a rate of, from a wormhole mouth, presumably from graviton production. If as an example, we are examining the mouth of a wormhole as being equivalent of a linkage between two black holes, or a black hole—white hole pair, we are presuming a release from the mouth of the wormhole commensurate with looking at [<xref ref-type="bibr" rid="scirp.110381-ref18">18</xref>] with an eye to “white holes” for a black hole model as of probability for “scalar” particle production given as, if M is the mass of the black (white) hole, m is the mass of an emitted “particle”, ω is frequency of emitted particles,</p><p>Γ ∝ exp ( − 8 π M ⋅ ω ⋅ [ 1 + β 4 ⋅ ( m 2 + 4 ω 2 ) ] ) (31)</p><p>Whereas we define the parameter β via a modified energy expression, as in [<xref ref-type="bibr" rid="scirp.110381-ref18">18</xref>] given by E ˜ as a modified energy expression in [<xref ref-type="bibr" rid="scirp.110381-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref19">19</xref>],</p><p>E ˜ = E ⋅ ( 1 − β ⋅ ( p 2 + m 2 ) ) (32)</p><p>Our Equations (28) and (29), which are for wormholes, should encompass the same information of Equation (31) which would be consistent with a white hole [<xref ref-type="bibr" rid="scirp.110381-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref21">21</xref>] at the mouth of a wormhole, as would be expected from Equation (31), whereas reviewing a linkage between black holes and white holes as may be for forming a wormhole may give more credence to the information loss criteria as given in [<xref ref-type="bibr" rid="scirp.110381-ref22">22</xref>].</p><p>Our next step is to ask if this permits speaking of say GW polarization in the mouth of a wormhole.</p><p>To do this, first of all, note that in [<xref ref-type="bibr" rid="scirp.110381-ref23">23</xref>] that the simplest version of a wormhole is one of two universes connected by a “throat” of the form of a “ball” given by π b 2 , whereas the term b, is in a diagram, consigned to be the radius, or shape of the initial “ball” joining two “universes”.</p><p>In the case of extending b to become the “shape” of the mouth of a wormhole, we would likely be using [<xref ref-type="bibr" rid="scirp.110381-ref24">24</xref>] for what is called by Visser the “shape” function of the wormhole [<xref ref-type="bibr" rid="scirp.110381-ref25">25</xref>], whereas what we are referring to in Equation (33) comes straight from [<xref ref-type="bibr" rid="scirp.110381-ref23">23</xref>]:</p><p>b ( r ) = [ r 0 γ − 1 γ + γ ⋅ ( 8 π G ) ω ˜ ˜ 1 / γ γ − 1 γ ⋅ ( r 3 − r 0 3 ) ] γ γ − 1 → r → r 0 r 0 (33)</p><p>Whereas we need to keep in mind the equation of state for pressure and density of [<xref ref-type="bibr" rid="scirp.110381-ref24">24</xref>]</p><p>p = ω ˜ ˜ ( r ) ⋅ ρ (34)</p><p>The long and short of it is as follows. Following [<xref ref-type="bibr" rid="scirp.110381-ref24">24</xref>] we have that:</p><p>ρ α ˜ = M ( 4 π α ˜ ) 3 / 2 ⋅ exp ( − r 2 / 4 α ˜ ) (35)</p><p>Whereas the b coefficient in the case of Noncommutative geometry is chosen [<xref ref-type="bibr" rid="scirp.110381-ref26">26</xref>]:</p><p>b ( r ) = 2 r s π ⋅ γ ⌢ ( 3 2 , r 2 4 α ˜ ) ≡ 2 r s π ⋅ ( r 2 4 α ˜ ) 3 / 2 ⋅ Γ ˜ ( 3 / 2 ) ⋅ e − 3 / 2 ⋅ ∑ k = 0 ∞ ( ( r 2 4 α ˜ ) k Γ ˜ ( ( 3 / 2 ) + k + 1 ) ) (36)</p><p>This is called the incomplete lower gamma function, with Γ ˜ being a gamma function [<xref ref-type="bibr" rid="scirp.110381-ref27">27</xref>].</p><p>From here, using that Equation (36) is to be included in the following metric, as given by the coefficient [ α ˜ ] = [ r 2 ] in terms of dimensional analysis is chosen so that the dimensions of [ α ˜ ] = [ r 2 ] are chosen to contain M as mass in a wormhole. i.e. the denominator of Equation (35) ( 4 π α ˜ ) 3 / 2 is chosen so that M is within the volume of space so subscribed. And this is for line element [<xref ref-type="bibr" rid="scirp.110381-ref26">26</xref>]. With Equation (35) fully described in [<xref ref-type="bibr" rid="scirp.110381-ref26">26</xref>] and [<xref ref-type="bibr" rid="scirp.110381-ref28">28</xref>],</p><p>d S 2 = − exp ( − 2 Φ ( r ) ) d t 2 + d r 2 1 − b ( r ) / r + r 2 ⋅ ( d θ 2 + ( sin 2 θ ) d φ 2 ) (37)</p><p>If we refer to black holes, with extra dimension, n, of Planck sized mass, we have a lifetime of the value of about:</p><p>τ ~ 1 M * ( M BH M * ) n + 3 n + 1 → M BH ≈ M Planck 10 − 26 seconds M * ≈ isthelowenergyscale , whichcouldbeaslowasafewTeV , (38)</p><p>The idea would be that there would be n additional dimensions, as given in Equation (38) which would then lay the door open to investigating [<xref ref-type="bibr" rid="scirp.110381-ref29">29</xref>] and [<xref ref-type="bibr" rid="scirp.110381-ref30">30</xref>] in terms of applications, with [<xref ref-type="bibr" rid="scirp.110381-ref30">30</xref>] of additional polarization states to be investigated, as to signals from the mouth of the wormhole. We will next then go into some predictions into first, the strength of the signals, the frequency range, and several characteristics as to the production rate of Planck sized black holes which conceivably could get evicted by use of Equation (28), in terms of what could be observed via instrumentation.</p></sec><sec id="s8"><title>8. A First Order Guess as to the Rate of Production of Planck Sized Black Holes through a Wormhole, Using Equation (28)</title><p>In order to do this, we will be estimating that the temperature would be of the order of Planck temperature, i.e. using ideas from [<xref ref-type="bibr" rid="scirp.110381-ref30">30</xref>] and [<xref ref-type="bibr" rid="scirp.110381-ref31">31</xref>],</p><p>ω p T p ≡ G k B 2 ℏ → ℏ = G = k B = 1 1 (39)</p><p>If so, then there would be to first order the following rate of production,</p><p>Γ rateofproduction ≈ e ≈ 2   -   3 (40)</p><p>Some of the considerations given in this could be related to [<xref ref-type="bibr" rid="scirp.110381-ref32">32</xref>] as an afterthought whereas the author in [<xref ref-type="bibr" rid="scirp.110381-ref33">33</xref>] estimated for an LHC that there would be about 3000 gravitons produced per second. Assuming a figure from [<xref ref-type="bibr" rid="scirp.110381-ref34">34</xref>] as to the percentage of black hole mass decaying into gravitons, i.e. [<xref ref-type="bibr" rid="scirp.110381-ref34">34</xref>], i.e., 1/1000 of the mass of a Planck sized black hole would delve into gravitons, so if one had 3000 gravitons produced per second, as measured on Earth, one would likely have 2 - 3 black holes, of mass of about 10<sup>−5</sup> grams per black hole, producing say 10<sup>57</sup> gravitons, produced per black hole of mass about 10<sup>−62</sup> grams per black hole [<xref ref-type="bibr" rid="scirp.110381-ref35">35</xref>].</p><p>Having said, that what about frequencies? Here, if we have a wormhole throat of about 2 - 3 Planck lengths in diameter, with a frequency of emitted gravitons of about 10<sup>19</sup> GHz initially, it is realistic, using the following, to expect in many cases a redshift downscaling of frequencies of about 10<sup>−18</sup>, if the wormholes are close to the initial near singularity, so then that we could be looking at approximately 10 to 12 GHz, on Earth, for frequencies, of initially about 10<sup>19</sup> GHZ. So then note at inflation we have:</p><p>( 1 + z initial era ) ≡ a t o d a y a initial era ≈ ( ω Earth orbit ω initial era ) − 1 ⇒ ( 1 + z initial era ) ω Earth orbit ≈ 10 25 ω Earth orbit ≈ ω initial era (41)</p><p>In our situation, the figure would likely be instead of 10<sup>25</sup> times Earth orbit detected frequency, something closer to 10<sup>18</sup> to 10<sup>19</sup> times Earth orbit GW frequencies detected as given by [<xref ref-type="bibr" rid="scirp.110381-ref36">36</xref>]. The relative GW strength of the signal, if one uses [<xref ref-type="bibr" rid="scirp.110381-ref36">36</xref>] while assuming approximately 10 to 12 GHz, for initially about 10<sup>19</sup> GHz GW signals would be about h ~10<sup>−26</sup> and this could change an order of magnitude given instrument sensitivity. In any case it would be well worth our while to look closely at [<xref ref-type="bibr" rid="scirp.110381-ref37">37</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref38">38</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.110381-ref40">40</xref>] for additional clues and insights to consider while commencing this investigation. As well as details are given in [<xref ref-type="bibr" rid="scirp.110381-ref41">41</xref>].</p></sec><sec id="s9"><title>Conflicts of Interest</title><p>The author declares no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s10"><title>Cite this paper</title><p>Beckwith, A. (2021) Looking at Quantization of a Wave Function, from Weber (1961), to Signals from Wavefunctions at the Mouth of a Wormhole. Journal of High Energy Physics, Gravitation and Cosmology, 7, 1037-1048. https://doi.org/10.4236/jhepgc.2021.73062</p></sec></body><back><ref-list><title>References</title><ref id="scirp.110381-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Weber, J. (2004) General Relativity and Gravitational Waves. Dover Publications, Incorporated, Mineola, New York.</mixed-citation></ref><ref id="scirp.110381-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Lu, H.Q., Fang, W., Huang, Z.G. and Ji, P.Y. 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