<?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.2017.34049</article-id><article-id pub-id-type="publisher-id">JHEPGC-79697</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>
 
 
  Gedanken Experiment for B Field Contributions to Initial Conditions for Relic Graviton Production Based upon an Initial Inflaton Value
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Andrew</surname><given-names>Walcott 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, Chongqing University, Chongqing, China</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>rwill9955b@gmail.com</email></corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>08</month><year>2017</year></pub-date><volume>03</volume><issue>04</issue><fpage>651</fpage><lpage>656</lpage><history><date date-type="received"><day>17,</day>	<month>August</month>	<year>2017</year></date><date date-type="rev-recd"><day>16,</day>	<month>October</month>	<year>2017</year>	</date><date date-type="accepted"><day>19,</day>	<month>October</month>	<year>2017</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><html>
 <head></head>
 
  This paper is to address using what a fluctuation of a metric tensor leads to, in Pre Planckian physics, namely 
  <img src="Edit_d151228d-ca63-4c2a-b5b2-effe86a13587.bmp" alt="" /> . If so then, we pick the conditions for an equality, with a small 
  <img src="Edit_b95abc2f-eafb-477a-8a23-f78615e2eee2.bmp" alt="" />, to come up with initial temperature, particle count and entropy affected by initial degrees of freedom in early Universe cosmology. This leads to an initial graviton production due to a minimum magnetic field, as established in our analysis. Which we relate to the inflaton as it initially would be configured and evaluated.
 
</html></p></abstract><kwd-group><kwd>Emergent Time</kwd><kwd> Heavy Gravity</kwd><kwd> Metric Tensor Perturbations</kwd><kwd> HUP</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>This article starts with updating what was done in [<xref ref-type="bibr" rid="scirp.79697-ref1">1</xref>] , which is symbolized by, if the scale factor is very small, metric variance [<xref ref-type="bibr" rid="scirp.79697-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref3">3</xref>]</p><p>〈 ( δ g u v ) 2 ( T ^ u v ) 2 〉 ≥ ℏ 2 V Volume 2 → u v → t t 〈 ( δ g t t ) 2 ( T ^ t t ) 2 〉 ≥ ℏ 2 V Volume 2 &amp;   δ g r r ~ δ g θ θ ~ δ g ϕ ϕ ~ 0 + (1)</p><p>In [<xref ref-type="bibr" rid="scirp.79697-ref4">4</xref>] this lead to</p><p>δ t Δ E ≥ ℏ δ g t t ≠ ℏ 2 Unless   δ g t t ~ O ( 1 ) (2)</p><p>We assume δ g t t is a small perturbation and look at δ t Δ E = ℏ δ g t t with</p><p>Δ t time ( initial ) = ℏ / ( δ g t t E initial ) = 2 ℏ δ g t t ⋅ g ∗ s ( initial ) ⋅ T initial (3)</p><p>This would put a requirement upon a very large initial temperature T initial and so then, if</p><p>S ( initial ) ~ n ( particle-count ) ≈ g ∗ s ( initial ) ⋅ V volume ⋅ ( 2 π 2 45 ) ⋅ ( T initial ) 3 [<xref ref-type="bibr" rid="scirp.79697-ref5">5</xref>]</p><p>S ( initial ) ~ n ( particle-count ) ≈ V volume g ∗ s 2 ( initial ) ⋅ ( 2 π 2 45 ) ⋅ ( ℏ Δ t initial ⋅ δ g t t ) 3 (4)</p><p>And if we can write as given in [<xref ref-type="bibr" rid="scirp.79697-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref3">3</xref>]</p><p>V volume ( initial ) ~ V ( 4 ) = δ t ⋅ Δ A surface-area ⋅ ( r ≤ l Planck ) (5)</p><p>The volume in the Pre Planckian regime would be extremely small, i.e. if we are using the convention that Equation (4) holds, then it argues for a very large g s ∗ beyond the value of 102, as given in [<xref ref-type="bibr" rid="scirp.79697-ref5">5</xref>] . In any case, our boundary between the Pre Planckian regime and Planckian, as far as the use of Equation (4) yields a preliminary value of, for a distance less than or equal to Planck Length, of non-zero value, with</p><p>10 20 ≤ S ( initial ) ~ n ( particle-count ) | r ≤ l P ≤ 10 37 (6)</p><p>This is also assuming a δ t initial ≈ Δ t initial ∝ Plank-time , i.e. at or smaller than the usual Planck time interval.</p></sec><sec id="s2"><title>2. Counter Pose Hypothesis, by String Theory, for Equation (6)</title><p>The author is aware of the String theory minimum length and minimum time which is different from the usual Planck lengths, but are avoiding these, mainly due to a change in the assumed entropy formulae to read as the square root of the above results, namely [<xref ref-type="bibr" rid="scirp.79697-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref8">8</xref>]</p><p>10 10 ≤ S ( initial ) | String-Theory ~ n ( particle-count ) | r ≤ l P ≤ 10 16 (7)</p><p>The above is still non-zero, but it cannot be exactly posited as in the Pre Planckian regime of Space-time, since the minimum length may be larger than Planck Length, i.e. as of the sort given in [<xref ref-type="bibr" rid="scirp.79697-ref8">8</xref>] .</p></sec><sec id="s3"><title>3. Questions as to Refining Both Equation (6) and Equation (7) for More Precise Entropy Bounds</title><p>If from Giovannini [<xref ref-type="bibr" rid="scirp.79697-ref9">9</xref>] we can write</p><p>δ g t t ~ a 2 ( t ) ⋅ ϕ ≪ 1 (8)</p><p>Refining the inputs from Equation (8) means more study as to the possibility of a non-zero minimum scale factor [<xref ref-type="bibr" rid="scirp.79697-ref10">10</xref>] , as well as the nature of ϕ as specified by Giovannini [<xref ref-type="bibr" rid="scirp.79697-ref9">9</xref>] . We hope that this can be done as to give quantifiable estimates and may link the non-zero initial entropy to either Loop quantum gravity “quantum bounce” considerations [<xref ref-type="bibr" rid="scirp.79697-ref11">11</xref>] and/or other models which may presage modification of the sort of initial singularities of the sort given in [<xref ref-type="bibr" rid="scirp.79697-ref12">12</xref>] . Furthermore if the non-zero scale factor is correct, it may give us opportunities as to fine tune the parameters given in [<xref ref-type="bibr" rid="scirp.79697-ref10">10</xref>] below:</p><p>α 0 = 4 π G 3 μ 0 c B 0 λ ⌢ ( defined ) = Λ c 2 / 3 a min = a 0 ⋅ [ α 0 2 λ ⌢ ( defined ) ( α 0 2 + 32 λ ⌢ ( defined ) ⋅ μ 0 ω ⋅ B 0 2 − α 0 ) ] 1 / 4 (9)</p><p>where the following is possibly linkable to minimum frequencies linked to E and M fields [<xref ref-type="bibr" rid="scirp.79697-ref10">10</xref>] , and possibly relic Gravitons are generated if</p><p>B &gt; 1 2 ⋅ 10 μ 0 ⋅ ω (10)</p><p>This can be contrasted with looking at what happens if [<xref ref-type="bibr" rid="scirp.79697-ref13">13</xref>]</p><p>a ≈ a min t γ ⇔ ϕ ≈ γ 4 π G ⋅ ln { 8 π G V 0 γ ⋅ ( 3 γ − 1 ) ⋅ t } ⇔ V ≈ V 0 ⋅ exp { − 16 π G γ ⋅ ϕ ( t ) } (11)</p><p>So as talked about with [<xref ref-type="bibr" rid="scirp.79697-ref14">14</xref>] setting a minimum energy density given by</p><p>ρ Λ ≈ G ( E / c 2 ) 2 l l − 3 = G E 6 c 8 ℏ 4 (12)</p><p>And with the following substitution of</p><p>E → Pre-Planckian → Planckian Δ E ~ ℏ Δ t ⋅ ( δ g t t ≈ a min 2 ϕ initial ) (13)</p><p>Then to first order we would be looking at Equation (12) re written as leading to</p><p>ρ Λ ~ G c 8 ℏ 4 ⋅ ( ℏ Δ t ⋅ ( δ g t t ≈ a min 2 ϕ initial ) ) 6 (14)</p><p>And if Equation (15) holds,</p><p>Λ initial ⋅ H initial − 2 ≈ o ( 1 ) (15)</p><p>we would have by [<xref ref-type="bibr" rid="scirp.79697-ref15">15</xref>]</p><p>Λ initial ≈ H initial 2 ~ γ 2 / t 2 Λ initial ⋅ L p 2 ≈ 10 − 123 (16)</p><p>So</p><p>10 − 123 ~ γ 2 L P 2 ⋅ ( Δ E ⋅ δ g t t ) 2 / ℏ 2 (17)</p><p>Equation (17) would be key to the entire business, i.e. using this, we would have if</p><p>Δ E ∼ ℏ ω graviton (18)</p><p>Then</p><p>10 − 123 ~ γ 2 L P 2 ⋅ ( ℏ ω graviton ⋅ δ g t t ) 2 / ℏ 2 ~ γ 2 L P 2 ⋅ ( ω graviton ⋅ δ g t t ) 2 (19)</p><p>Then if we go to Equation (10) we have a threshold magnetic field for the production of gravitons which looks like if we apply the minimum scale factor condition [<xref ref-type="bibr" rid="scirp.79697-ref16">16</xref>] , that</p><p>B min ≥ 1 2 ⋅ 10 μ 0 ⋅ ω ≈ γ L P δ g t t 10 123 / 4 2 ⋅ 10 μ 0 ≈ γ L P ϕ initial a min 10 123 / 4 2 ⋅ 10 μ 0 &amp;     a min ~ ( 10 − 123 / 4 ) ⇒ B min ≥ γ L P ϕ initial 2 ⋅ 10 μ 0 (20)</p><p>i.e. we get graviton production if the last line of Equation (20) is satisfied, which means that the initial value of the inflaton, in this case is crucially important.</p><p>With that initial inflaton value determined in part by Equation (11).</p></sec><sec id="s4"><title>4. Conclusions: The Inflaton Minimum Helps Determine a Lower Bound for a Cosmological Initial Production of Gravitons</title><p>The last line of Equation (20) helps establish a minimum magnetic field for the production of relic gravitons, with a magnetic field established through Equation (10) and subsequently modified by Equation (20).</p><p>This adds substance to what was brought up by Beckwith in [<xref ref-type="bibr" rid="scirp.79697-ref16">16</xref>] namely that we have a minimum scale factor of</p><p>a min ~ ( 10 − 123 / 4 ) ~ ( Δ E / E P ) 3 / 2 &amp;   ϕ initial 2 ~ o ( Δ E ⋅ γ ⋅ L P / ℏ 2 ) (21)</p><p>But Equation (21) and Equation (20) interplay and also give more substances to the use of Equation (19) with our guess of Equation (18) for the determination of the initial graviton frequency, which has to be at least of the order of 10^45 Hertz due to the fantastically small initial bubble of space time considered.</p><p>In doing so, we need to consider initial conditions so considered that Equation (20) and Equation (21) should be consistent with the inflaton and “gravity’s breath” document by Corda [<xref ref-type="bibr" rid="scirp.79697-ref17">17</xref>] . In addition, Freeze’s statement of initial conditions for inflaton, as given by [<xref ref-type="bibr" rid="scirp.79697-ref18">18</xref>] should be adhered to. It is also extremely important that the LIGO results, even if this is of relic gravitational waves, as seen by Abbott in [<xref ref-type="bibr" rid="scirp.79697-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.79697-ref21">21</xref>] , should not be contravened.</p><p>We conclude also with the hope that interpolating between the results of Equation (19), Equation (20) and Equation (21) will also in time confer answers as to the initial evaluative conditions for gravity as given in [<xref ref-type="bibr" rid="scirp.79697-ref22">22</xref>] by Corda. This also may in time with further analysis tie in with minimum values of entropy by further analysis of Equation (4) in further future analysis of this problem.</p></sec><sec id="s5"><title>Fund</title><p>Work partially supported by National Nature Science Foundation of China grant No. 11375279.</p></sec><sec id="s6"><title>Cite this paper</title><p>Beckwith, A.W. (2017) Gedanken Experiment for B Field Contributions to Initial Conditions for Relic Graviton Production Based upon an Initial Inflaton Value. Journal of High Energy Physics, Gravitation and Cosmology, 3, 651-656. https://doi.org/10.4236/jhepgc.2017.34049</p></sec></body><back><ref-list><title>References</title><ref id="scirp.79697-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Downes, T.G. and Milburn, G.J. Optimal Quantum Estimation for Gravitation. arXiv:1108.5220 [gr-qc].</mixed-citation></ref><ref id="scirp.79697-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Unruh, W.G. (1986) Why Study Quantum Theory? Canadian Journal of Physics, 64, 128-130. &lt;br /&gt;https://doi.org/10.1139/p86-019</mixed-citation></ref><ref id="scirp.79697-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A. (2016) Gedanken Experiment for Refining the Unruh Metric Tensor Uncertainty Principle via Schwarzschild Geometry and Planckian Space-Time with Initial Nonzero Entropy and Applying the Riemannian-Penrose Inequality and Initial Kinetic Energy for a Lower Bound to Graviton Mass (Massive Gravity). Journal of High Energy Physics, Gravitation and Cosmology, 2, 106-124. 
&lt;br /&gt;https://doi.org/10.4236/jhepgc.2016.21012</mixed-citation></ref><ref id="scirp.79697-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A.W. Gedankenexperiment for Refining the Unruh Metric Tensor Uncertainty Principle via Schwartzshield Geometry and Planckian Space-Time with Initial Non Zero Entropy. Ukranian Journal of Physics (Unpublished). 
http://vixra.org/pdf/1509.0173v6.pdf</mixed-citation></ref><ref id="scirp.79697-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Kolb, E. and Turner, M. (1990) The Early Universe. Addison-Wesley Publishing Company, Redwood City, California.</mixed-citation></ref><ref id="scirp.79697-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Louis, J., Mohaupt, T. and Theisen, S. (2007) String Theory: An Overview. Lecture Notes in Physics, 721, 289-323.  
http://www.aei.mpg.de/~theisen/LMT.pdf 
&lt;br /&gt;https://doi.org/10.1007/978-3-540-71117-9_12</mixed-citation></ref><ref id="scirp.79697-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Ammon, M. and Ergmenger, J. (2015) Gauge/Gravity Duality, Foundations and Applications. Cambridge University Press, Cambridge.  
&lt;br /&gt;https://doi.org/10.1017/CBO9780511846373</mixed-citation></ref><ref id="scirp.79697-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Becker, K., Becker, M. and Schwarz, J.H. (2007) String Theory and M-Theory: A Modern Introduction. Cambridge University Press, Cambridge.</mixed-citation></ref><ref id="scirp.79697-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Giovannini, M. (2008) A Primer on the Physics of the Cosmic Microwave Background. World Press Scientific, Hackensack, New Jersey. 
&lt;br /&gt;https://doi.org/10.1142/6730</mixed-citation></ref><ref id="scirp.79697-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Camara, C.S., de Garcia Maia, M.R., Carvalho, J.C. and Lima, J.A.S. (2004) Nonsingular FRW Cosmology and Non Linear Dynamics. Physical Review D, 69, 123504. 
&lt;br /&gt;https://doi.org/10.1103/PhysRevD.69.123504</mixed-citation></ref><ref id="scirp.79697-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Rovelli, C. and Vidotto, F. (2015) Covariant Loop Quantum Gravity, an Elementary Introduction to Quantu Gravity and Spinfoam Theory. Cambridge University Press, Cambridge.</mixed-citation></ref><ref id="scirp.79697-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Ashtekar, A., Berger, B., Isenberg, J. and Mac Callum, M. (2015) General Relativity and Gravitation, a Centennial Perspective. Cambridge University Press, Cambridge.  
&lt;br /&gt;https://doi.org/10.1017/CBO9781139583961</mixed-citation></ref><ref id="scirp.79697-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Padmanabhan, T. (2005) Understanding Our Universe: Current Status, and Open Issues. World Scientific, P.T.E. Ltd., Singapore, 175-204.  
http://arxiv.org/abs/gr-qc/0503107</mixed-citation></ref><ref id="scirp.79697-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">https://ned.ipac.caltech.edu/level5/Sept02/Padmanabhan/Pad1_2.html</mixed-citation></ref><ref id="scirp.79697-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">https://ned.ipac.caltech.edu/level5/Sept02/Padmanabhan/Pad7.html</mixed-citation></ref><ref id="scirp.79697-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Beckwith, A. (2017) Constraints, in Pre Planckian Space-Time via Padmabhan’s Approximation Leading to Initial Inflaton Constraints.  
http://vixra.org/abs/1701.0333</mixed-citation></ref><ref id="scirp.79697-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Corda, C. (2011) Primordial Gravity’s Breath. Electronic Journal of Theoretical Physics, 9, 1-10. http://www.ejtp.com/articles/ejtpv9i26.pdf  
&lt;br /&gt;https://arxiv.org/abs/1110.1772</mixed-citation></ref><ref id="scirp.79697-ref18"><label>18</label><mixed-citation publication-type="book" xlink:type="simple">Freese, K. (1992) Natural Inflaton. In: Nath, P. and Recucroft, S., Eds., Particles, Strings, and Cosmology, Northeastern University, World Scientific Publishing Company, Singapore, 408-428.</mixed-citation></ref><ref id="scirp.79697-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2016) Observation of Gravitational Waves from a Binary Black Hole Merger. Physical Review Letters, 116, Article ID: 061102.</mixed-citation></ref><ref id="scirp.79697-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2016) GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence. Physical Review Letters, 116, Article ID: 241103.</mixed-citation></ref><ref id="scirp.79697-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2016) Tests of General Relativity with GW150914.  
&lt;br /&gt;https://arxiv.org/pdf/1602.03841.pdf</mixed-citation></ref><ref id="scirp.79697-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">Corda, C. (2009) Interferometric Detection of Gravitational Waves: The Definitive Test for General Relativity. International Journal of Modern Physics D, 18, 2275-2282. &lt;br /&gt;https://arxiv.org/abs/0905.2502  
&lt;br /&gt;https://doi.org/10.1142/S0218271809015904</mixed-citation></ref></ref-list></back></article>