<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2012.39116</article-id><article-id pub-id-type="publisher-id">JMP-22621</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>
 
 
  Dirac Hamiltonian with Imaginary Mass and Induced Helicity—Dependence by Indefinite Metric
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>lrich</surname><given-names>D. Jentschura</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>1Department of Physics, Missouri University of Science and Technology, Rolla, USA</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>ulj@mst.edu</email></corresp></author-notes><pub-date pub-type="epub"><day>24</day><month>09</month><year>2012</year></pub-date><volume>03</volume><issue>09</issue><fpage>887</fpage><lpage>894</lpage><history><date date-type="received"><day>June</day>	<month>27,</month>	<year>2012</year></date><date date-type="rev-recd"><day>July</day>	<month>29,</month>	<year>2012</year>	</date><date date-type="accepted"><day>August</day>	<month>7,</month>	<year>2012</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>
 
  It is of general theoretical interest to investigate the properties of superluminal matter wave equations for spin one-half particles. One can either enforce superluminal propagation by an explicit substitution of the real mass term for an imaginary mass, or one can use a matrix representation of the imaginary unit that multiplies the mass term. The latter leads to the tachyonic Dirac equation, while the equation obtained by the substitution 
  m 
  <img src="http://chart.googleapis.com/chart?cht=tx&amp;chl=%5Crightarrow%20" style="border:none;" /> 
  im in the Dirac equation is naturally referred to as the imaginary-mass Dirac equation. Both the tachyonic as well as the imaginary-mass Dirac Hamiltonians commute with the helicity operator. Both Hamiltonians are pseudo-Hermitian and also possess additional modified pseudo-Hermitian properties, leading to constraints on the resonance eigenvalues. Here, by an explicit calculation, we show that specific sum rules over the The spectrum is found to consist of well-defined real energy eigenvalues and complex resonance and anti-resonance energies. In the quantized imaginary-mass Dirac field, one-particle states of right-handed helicity acquire a negative norm (“indefinite metric”) and can be excluded from the physical spectrum by a Gupta-Bleuler type condition.
 
</html></p></abstract><kwd-group><kwd>Neutrinos; Particles; Tachyonos</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction and Overview</title><sec id="s1_1"><title>1.1. Theory and Experiment</title><p>The superluminal propagation of matter waves is a highly intriguing subject which is not without controversy. The subluminal (tardyonic) energy-momentum relation <img src="1-7500827\800ed47f-ed30-48e8-b9ad-f0a3ab8fff5a.jpg" /> needs to be changed to the superluminal (tachyonic) dispersion relation<img src="1-7500827\3d98821b-3808-4d47-adec-bf6f409ce789.jpg" />. Recently, it has been argued that the tachyonic Dirac equation [1,2] provides for a convenient framework for the description of tachyonic particles; in this equation, the mass is multiplied by a matrix representation of the imaginary unit. Here, starting from the Dirac Hamiltonian, we explore a Dirac equation where the mass is explicitly multiplied by the imaginary unit and we find certain fundamental relations for the corresponding spin-1/2 field theory. We also explore certain algebraic properties of modified Dirac theories with an imaginary mass term, and pertaining consequences for the eigenvalue spectrum of the imaginary-mass Dirac Hamiltonian. The tachyonic formulation [3-8] of a fundamental field theory is the only one compatible with Lorentz invariance, and therefore, compatible with special relativity. We exclusively use this concept in the following and avoid any breaking of Lorentz invariance.</p><p>According to the summary overview presented in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref9">9</xref>], low-energy experiments have determined the neutrino mass square to be in the range of a few<img src="1-7500827\949b97fa-5cb8-4852-b359-d38291647e67.jpg" />. The best estimate for the neutrino mass square has been determined as negative in all experiments [10-16], but the result has been consistent with a vanishing neutrino mass within experimental error bars. In direct measurements of the neutrino velocity [17-19], the best estimate derived from experimental data has been superluminal (<img src="1-7500827\22c8d2c4-81ce-493f-b750-033ad6aebf64.jpg" />), but again, consistent with the hypothesis <img src="1-7500827\800c84f1-ea0a-4267-8d68-046366abcf21.jpg" /> within experimental error bars (see also Ref. [<xref ref-type="bibr" rid="scirp.22621-ref9">9</xref>] or <xref ref-type="table" rid="table1">Table 1</xref> of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref20">20</xref>]). The OPERA collaboration [<xref ref-type="bibr" rid="scirp.22621-ref21">21</xref>] has indicated a preliminary, revised result of<img src="1-7500827\8c9e51fe-b000-41ce-95b4-76ecdc3e1f4d.jpg" />, which (just like all other available experimental results) neither excludes subluminal nor superluminal propagation.</p><p>The neutrino is generally regarded as the most prominent candidate for a superluminal particle in the lowenergy domain [20,22-25]. However, the existence of conceivable superluminal particles in hitherto unexplored kinematic regions cannot be excluded, either; our study is of theoretical nature and not tied to a specific particle. It has recently been argued [1,2] that the tachyonic theory of spin-1/2 particles is easier to implement as compared to spinless particles, and we here continue this line of thought by analyzing a theory where the imaginary mass is used explicitly in the Dirac equation, rather than a matrix representation thereof. The latter has been used in Refs. [1,2,22,26,27]. We use natural units with<img src="1-7500827\08d06264-1b66-486f-a647-4967828df4ab.jpg" />.</p></sec><sec id="s1_2"><title>1.2. Theoretical Foundations</title><p>It is useful to recall that the subluminal (tardyonic) Dirac Hamiltonian <img src="1-7500827\1d98c24a-3d90-4295-a517-215c5a64309d.jpg" /> reads</p><disp-formula id="scirp.22621-formula11527"><label>(1)</label><graphic position="anchor" xlink:href="1-7500827\76cef1d2-8971-4c52-9a52-3ce9fb3f0648.jpg"  xlink:type="simple"/></disp-formula><p>Here, <img src="1-7500827\d432ca64-3c6a-4db4-a48d-b06d52cb413e.jpg" />is the momentum operator. We use the Dirac matrices in the standard Dirac representation (<img src="1-7500827\fe392e89-a1fa-4816-9e53-d5925e69ae72.jpg" />, and<img src="1-7500827\73b98d8e-9d81-4627-9766-8c1ccc31422c.jpg" />),</p><disp-formula id="scirp.22621-formula11528"><label>(2)</label><graphic position="anchor" xlink:href="1-7500827\65f712ce-6f88-4576-9177-33cab5aefcb4.jpg"  xlink:type="simple"/></disp-formula><p>The Hamiltonian <img src="1-7500827\08b24591-69f0-44d5-9a7a-a40b547bb27b.jpg" /> can be modified into a Hamiltonian describing superluminal (tachyonic) particles by the simple replacement <img src="1-7500827\b15f6415-bd86-4fb1-8aa8-bc2c6ca15810.jpg" /> (see Ref. [<xref ref-type="bibr" rid="scirp.22621-ref28">28</xref>]), leading to the imaginary-mass Dirac Hamiltonian</p><disp-formula id="scirp.22621-formula11529"><label>(3)</label><graphic position="anchor" xlink:href="1-7500827\026ffe64-6677-43a2-b19d-f973e31bed3d.jpg"  xlink:type="simple"/></disp-formula><p>Alternatively, one can choose a matrix representation of the imaginary unit, and write the tachyonic Dirac Hamiltonian [1,2,22,26,27] as</p><disp-formula id="scirp.22621-formula11530"><label>(4)</label><graphic position="anchor" xlink:href="1-7500827\57ed3649-bc01-4d3e-af4f-4d1b3b865caa.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="1-7500827\795fea96-6a76-41fa-af5e-8ea5751f681a.jpg" /> and</p><disp-formula id="scirp.22621-formula11531"><label>(5)</label><graphic position="anchor" xlink:href="1-7500827\ec1c0890-8c64-4521-bc69-d39f03c7e064.jpg"  xlink:type="simple"/></disp-formula><p>Both <img src="1-7500827\fe8a7f77-e140-4563-92cd-bd5187f8fa59.jpg" /> and <img src="1-7500827\3a90f0f7-89b2-4cfd-84aa-8c3bc49f9ff4.jpg" /> are pseudo-Hermitian, which implies that eigenvalues are either real or come in complexconjugate pairs, <img src="1-7500827\a7180a9a-9f56-4d96-9464-9b8c1358f046.jpg" />and<img src="1-7500827\0b02ab63-7331-4b60-ab6f-fc5c387d4cae.jpg" />. Here, we also show that <img src="1-7500827\bae236a7-7fcb-4a99-8af4-39d2e86817ba.jpg" /> and <img src="1-7500827\b4193df6-3d9f-428e-b8b6-d95136833658.jpg" /> fulfill additional, modified pseudo-Hermiticity conditions (“quasi-pseudo-Hermiticity”), which allow us to further conclude that if <img src="1-7500827\55d966ea-fa93-4cfb-ba63-584ff3f2e84a.jpg" /> is a resonance eigenvalue, so is<img src="1-7500827\217ec732-0720-42e4-ad87-c9c8e1a1e7b3.jpg" />, and thus, the eigenvalues either come in (real) pairs <img src="1-7500827\0de15261-1e7e-46f9-a793-a35bdbe855df.jpg" /> and<img src="1-7500827\c2063f98-3d21-49e6-95db-99e06f5b32dc.jpg" />, or they occur in the rectangular complex configuration<img src="1-7500827\99bb0a7a-fae7-4358-8d24-1165e0e9a771.jpg" />, <img src="1-7500827\1b2cafb4-fdf6-4071-997a-a8bea67b3531.jpg" />, <img src="1-7500827\ef7ce594-bed9-42d5-88be-b81db96dc4e9.jpg" />, and<img src="1-7500827\fa3e1f91-d948-4e8a-9bc5-9e86c989b79b.jpg" />. The quantization of the imaginary-mass Dirac theory naturally leads to helicity-dependent anticommutators.</p><p>We proceed as follows. In Section 2, we derive a few algebraic properties of the Hamiltonians <img src="1-7500827\e5493a89-b10f-431c-9df0-b5d7ef65f84d.jpg" /> and <img src="1-7500827\149c9e14-2166-42ee-8098-73d897b7a521.jpg" /> which determine the general properties of their spectra. The field theory defined by the Hamiltonian <img src="1-7500827\60f6990f-b914-4838-97e4-c264503cd222.jpg" /> is quantized in Section 3. In Section 4, we analyze the Hamiltonian <img src="1-7500827\ad17c4b0-7083-4ce3-80ca-8203aace9e27.jpg" /> which is obtained from (3) by the replacement<img src="1-7500827\2d120cdd-36d4-4342-8d27-1bf5b2c7f699.jpg" />. The quantization of the imaginary-mass Dirac theory is shown to yield rather interesting insight into helicity-dependent anticommutators. Conclusions are reserved for Section 5.</p></sec></sec><sec id="s2"><title>2. Algebraic Properties and Eigenvalues</title><p>It is useful to derive a few algebraic properties of <img src="1-7500827\d0378437-a98f-47b0-b30e-85b89a1f6e89.jpg" /> and <img src="1-7500827\71d8481b-e350-4dca-8c87-c3d5c6517f6c.jpg" /> which determine the structure of the spectra of these Hamiltonians. We explicitly refer to the coordinatespace representations <img src="1-7500827\d14c23bd-2869-44ae-8edf-fdfe940e0a38.jpg" /></p><disp-formula id="scirp.22621-formula11532"><label>(6)</label><graphic position="anchor" xlink:href="1-7500827\75cbf0aa-53db-4adb-8557-8a4c1a6e684e.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.22621-formula11533"><label>(7)</label><graphic position="anchor" xlink:href="1-7500827\bc745d36-122e-4747-9787-f1a2a92552cf.jpg"  xlink:type="simple"/></disp-formula><p>We use the following matrices,</p><disp-formula id="scirp.22621-formula11534"><label>(8)</label><graphic position="anchor" xlink:href="1-7500827\b411db7e-fea0-4495-85a8-1e130de7dc01.jpg"  xlink:type="simple"/></disp-formula><p>These fulfill<img src="1-7500827\0df79d73-e4d5-4fbf-b53a-28883b581a46.jpg" />, <img src="1-7500827\73a554c3-c1d7-46f6-92b3-2cb99a4ad439.jpg" />, and<img src="1-7500827\563881d7-23b3-41c7-bfc1-76152f836603.jpg" />. By elementary calculation, we infer that</p><disp-formula id="scirp.22621-formula11535"><label>(9a)</label><graphic position="anchor" xlink:href="1-7500827\1f3217bf-d7ad-4c30-8fe3-9751d6026f17.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11536"><label>(9b)</label><graphic position="anchor" xlink:href="1-7500827\e13b926c-0688-4a19-a052-e1afff02c763.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11537"><label>(9c)</label><graphic position="anchor" xlink:href="1-7500827\6b85493a-e64a-4f5c-9970-6988c10d7802.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11538"><label>(9d)</label><graphic position="anchor" xlink:href="1-7500827\6d67ff6e-75fc-4bcd-a990-2b278819369c.jpg"  xlink:type="simple"/></disp-formula><p>where the superscript + denotes the Hermitian adjoint. The relations (9a) and (9c) imply the pseudo-Hermiticity of the Hamiltonians <img src="1-7500827\7ea05c79-12ad-495c-af2a-b7dfb451ee05.jpg" /> and<img src="1-7500827\2f10b170-ece7-492a-a292-4fe063c9e846.jpg" />, respectively, in the sense of Refs. [29-38]. As shown in Refs. [1,29], for a pseudo-Hermitian Hamiltonian, if <img src="1-7500827\d2dc234f-ea33-487b-9d07-7e12259f4330.jpg" /> is a resonance eigenvalue, so is<img src="1-7500827\3a582661-7184-4360-b783-f1c4975a1f5f.jpg" />. Indeed, it has been shown in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>] that <img src="1-7500827\90515653-2b62-4405-8510-0e7a585c2306.jpg" /> has both real eigenvalues (corresponding to plane-wave solutions of positive and negative energy), and also resonances and anti-resonances whose resonance energies are manifestly complex. The resonances correspond to evanescent waves whose wavelength is too long to support superluminal propagation; these waves therefore decay exponentially.</p><p>In comparison to the structure of Equations (9a) and (9c), the relations (9b) and (9d) feature an additional minus sign. They correspond to additional “quasi-pseudoHermitian” properties of <img src="1-7500827\3b5532d0-115d-4941-b46a-6d138fdae26d.jpg" /> and<img src="1-7500827\063cf8b6-1899-4a2a-ad4f-b30285a7227a.jpg" />. These additional properties imply that if <img src="1-7500827\5d3d044a-48ac-439f-8d15-5481a90df814.jpg" /> is a resonance eigenvalue, so is<img src="1-7500827\1cf22786-c7e9-42da-b092-3c9a948c6ad8.jpg" />. This can be shown as follows. Let <img src="1-7500827\83b429d4-381d-4bfd-8697-ac784a87ace8.jpg" /> be an eigenfunction of a general Hamiltonian <img src="1-7500827\03f4c302-b7a1-419b-91ab-469e90a09af5.jpg" /> with eigenvalue<img src="1-7500827\95db240a-b04c-45d8-976f-c9b28bb5792e.jpg" />. Then, because the spectrum of the Hermitian adjoint of an operator consists of the complex-conjugate eigenvalues, there exists a wavefunction <img src="1-7500827\a6310cac-723f-4445-bbc0-844875006daf.jpg" /> with the property</p><disp-formula id="scirp.22621-formula11539"><label>(10)</label><graphic position="anchor" xlink:href="1-7500827\b713abb9-0891-4095-b332-1ca0f46b8962.jpg"  xlink:type="simple"/></disp-formula><p>from which we infer that</p><disp-formula id="scirp.22621-formula11540"><label>(11)</label><graphic position="anchor" xlink:href="1-7500827\0a37157f-d555-4b93-ac8d-3832aab1d8b4.jpg"  xlink:type="simple"/></disp-formula><p>and so, in view of Equation (9b), we have <img src="1-7500827\9a35f19b-29db-4e11-9d4a-0430bfec4156.jpg" />. So, if E is a resonance eigenvalue of<img src="1-7500827\e645f6ba-b239-4193-bfbc-9ec569a1d6d6.jpg" />, so is<img src="1-7500827\d07e3e42-5041-417b-a675-c91a2ed21066.jpg" />, with a corresponding eigenvector<img src="1-7500827\4b5af594-a439-4463-8492-a768399e4d51.jpg" />. The same property is implied for <img src="1-7500827\15548a63-bab8-44db-b44a-777a2f6406fa.jpg" /> by Equation (9d). If E is real, then Equations (9b) and (9d) imply that energy eigenvalues come in pairs E and<img src="1-7500827\61489618-d964-4280-aaca-35197972debc.jpg" />, whereas if they are manifestly complex, then they exhibit a rectangular configuration (in the complex plane) consisting of E, <img src="1-7500827\43499af8-9c3a-491a-a62b-92ff74b3866a.jpg" />, <img src="1-7500827\b4f736ca-e64b-4ead-8570-db37e40f72ce.jpg" />and<img src="1-7500827\90c653a8-983e-4561-953e-74fbbef573c2.jpg" />.</p></sec><sec id="s3"><title>3. Quantization and Spin Sums</title><p>First, we observe that both <img src="1-7500827\c866cdee-dda4-4a9f-87ef-23ad18eb4a6d.jpg" /> and <img src="1-7500827\8a3856ec-9555-432f-aa57-1e15a6710840.jpg" /> commute with the helicity operator,</p><disp-formula id="scirp.22621-formula11541"><label>(12)</label><graphic position="anchor" xlink:href="1-7500827\d1ee73a6-4274-4430-96cc-2c71d1df93ce.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.22621-formula11542"><label>(13)</label><graphic position="anchor" xlink:href="1-7500827\33f8d832-ecf1-4e9b-8a27-2dc2cc83ca8b.jpg"  xlink:type="simple"/></disp-formula><p>The quantization of the tachyonic theory defined by the Hamiltonian <img src="1-7500827\7be2c0a5-3da7-4881-a85f-7490bf1bc073.jpg" /> has been discussed in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>]. Here, we are concerned with the Hamiltonian<img src="1-7500827\a5c1ee06-5388-44f7-bd7c-fb6d3fa8612d.jpg" />. The corresponding covariant form the imaginary-mass Dirac equation reads as</p><disp-formula id="scirp.22621-formula11543"><label>(14)</label><graphic position="anchor" xlink:href="1-7500827\b871659c-5512-4580-8d8d-adc6be44faa2.jpg"  xlink:type="simple"/></disp-formula><p>Of course, it could be argued that the solutions of the imaginary-mass Dirac equation can be written down immediately, by simply replacing <img src="1-7500827\53900306-c2d2-46a4-b2cd-f0249e21b64b.jpg" /> in the wellknown bispinor solutions of the ordinary Dirac equation, as given in Chapter 2 of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>]. However, this procedure does not lead to compact formulas when one tries to develop the formalism further. A brief, sketchy, illustrative remark is in order. According to Equation (2.40) of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>], the spin sum over the positive-energy states of the tardyonic (ordinary) Dirac equation leads to the expression</p><disp-formula id="scirp.22621-formula11544"><label>(15)</label><graphic position="anchor" xlink:href="1-7500827\9ef0e8af-96c2-4b6c-a992-f9f7821d52e2.jpg"  xlink:type="simple"/></disp-formula><p>where the latter term is the projector onto positive-energy states. Here, <img src="1-7500827\c84a1fa9-45f8-42c6-b28f-82134477e31e.jpg" />is the Feynman dagger. When replacing <img src="1-7500827\a6721e74-20a7-4080-88c6-f9d5d6883de6.jpg" /> in the solution of the Dirac equation given in Equation (2.37) of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>], and performing the same spin sum over positive-energy solutions of the form <img src="1-7500827\fc4a4c87-9833-4988-a7c5-48658f4004f9.jpg" /> (using the notation of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>]), one has to replace <img src="1-7500827\5f145fce-a86a-4dfd-a785-f78e7c24a461.jpg" /> for the spinors and <img src="1-7500827\01bc03b3-2e8a-4ce3-a8e4-c20baa7f361a.jpg" /> for the Dirac adjoint bispinors. But then,</p><disp-formula id="scirp.22621-formula11545"><label>(16)</label><graphic position="anchor" xlink:href="1-7500827\42d0f254-312c-40e6-9fc3-25d51383f604.jpg"  xlink:type="simple"/></disp-formula><p>which is not equal to a compact projector form, as an elementary calculation shows. By contrast, compact formulas for sums over spins can be obtained in the helicity basis, as shown in the following.</p><p>For tachyonic particles, in analogy to the formalism developed in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>], it appears advantageous to use the helicity basis for the construction of the elementary solutions. We recall that the eigenfunctions of the operator <img src="1-7500827\568132f7-0a9a-4761-82c3-58f5182af881.jpg" /> are given by</p><disp-formula id="scirp.22621-formula11546"><label>(17)</label><graphic position="anchor" xlink:href="1-7500827\46ab075e-f73f-4c99-b473-c1c39ca4aaad.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7500827\fb011a9a-3037-44cc-83a2-9618b14c02e1.jpg" /> and <img src="1-7500827\d9e450f1-0c58-4518-a220-a84daa187756.jpg" /> constitute the polar and azimuthal angles of the wave vector k, with<img src="1-7500827\276b30eb-c104-4f6d-b379-a65e3c4b8a4a.jpg" />. We also recall the normalized positive-energy chirality and helicity eigenspinors of the massless Dirac equation as follows<img src="1-7500827\1f5f9c73-4891-4c57-afcf-4c5bb731d0be.jpg" />,</p><disp-formula id="scirp.22621-formula11547"><label>(18a)</label><graphic position="anchor" xlink:href="1-7500827\71334897-74be-4fbf-b119-53a87a713c9a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11548"><label>(18b)</label><graphic position="anchor" xlink:href="1-7500827\700e518c-c4fb-4016-a2d0-948e3c7b1d88.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11549"><label>(18c)</label><graphic position="anchor" xlink:href="1-7500827\8d711d37-96b5-45fb-b842-bdbbde3cd20b.jpg"  xlink:type="simple"/></disp-formula><p>Canonically, the subscripts <img src="1-7500827\b23d2531-2410-4df8-942e-04db37d01206.jpg" /> of the u and v spinors correspond to the chirality (eigenvalue of<img src="1-7500827\5b64571a-47d9-4566-b67c-b7682881b0ad.jpg" />), which (in the massless limit) is equal to helicity for positive-energy eigenstates, and equal to the negative of the chirality for negative-energy eigenstates. This is because the positiveand negative-energy solutions are multiplied by <img src="1-7500827\1661280a-13c0-4871-b653-82ae3dd32124.jpg" /> and<img src="1-7500827\9cc8738e-eefe-4f9a-b525-c7d9ca39f708.jpg" />, respectively [see Equation (22)]. Using the relation</p><p><img src="1-7500827\a0df2004-6ffb-4211-b504-50e5c7ebef26.jpg" />we find</p><disp-formula id="scirp.22621-formula11550"><label>(19a)</label><graphic position="anchor" xlink:href="1-7500827\7cc50f93-1a50-4b3a-8e16-bcaa23f2b5bf.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11551"><label>(19b)</label><graphic position="anchor" xlink:href="1-7500827\8198712a-4125-4352-a185-1fda841ef10b.jpg"  xlink:type="simple"/></disp-formula><p>The massless limit <img src="1-7500827\7e506ca8-9d3d-42bb-b7b1-da6f0d1b8c5b.jpg" /> <img src="1-7500827\79683417-5cd1-49c5-9b0f-2656729311bb.jpg" /> is recovered as <img src="1-7500827\96cc66c0-c946-4615-9b70-e7232e59b6c6.jpg" /> and<img src="1-7500827\497234f7-46e5-4308-a558-53f5ffd80339.jpg" />. The negativeenergy eigenstates of the imaginary-mass Dirac equation are given as</p><disp-formula id="scirp.22621-formula11552"><label>(20a)</label><graphic position="anchor" xlink:href="1-7500827\1b356043-3f4c-4600-a967-819cecbb42fe.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11553"><label>(20b)</label><graphic position="anchor" xlink:href="1-7500827\51324d1a-f032-42b5-b31c-c2147ba4e78a.jpg"  xlink:type="simple"/></disp-formula><p>In the massless limit, the solutions <img src="1-7500827\e7ee3799-e7ce-4f1f-835d-ec6bd217a5f1.jpg" /> and <img src="1-7500827\279d087a-a123-45b6-85d9-0f2788b65aae.jpg" /> are recovered, <img src="1-7500827\ea4913c7-f620-4c4d-9056-61316f12537c.jpg" />and<img src="1-7500827\3c789068-b7df-4a73-b164-c573c4a46147.jpg" />. The states are normalized with respect to the condition</p><disp-formula id="scirp.22621-formula11554"><label>(21)</label><graphic position="anchor" xlink:href="1-7500827\897ac0a8-7a4d-4d7b-92ca-6e295fbf9989.jpg"  xlink:type="simple"/></disp-formula><p>The positiveand negative-energy solutions of the imaginary-mass Dirac equation are thus given as&#160;&#160;</p><disp-formula id="scirp.22621-formula11555"><label>(22a)</label><graphic position="anchor" xlink:href="1-7500827\bdf90209-05a0-4874-b872-5557ec6b761c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11556"><label>(22b)</label><graphic position="anchor" xlink:href="1-7500827\cde176f8-078b-4794-a249-dd3b48b3de82.jpg"  xlink:type="simple"/></disp-formula><p>Here, <img src="1-7500827\6fcef7e0-ce79-4fb2-8984-3666eadb25de.jpg" />is a solution for positive energy, and <img src="1-7500827\e54fbc8d-6f68-4b11-bbff-3cd8424cd622.jpg" /> constitutes a solution for negative energy. All above formulas are valid for<img src="1-7500827\ed0a49e3-f3c2-4af1-a649-6ea7bd206009.jpg" />, so that <img src="1-7500827\5f061482-ba3a-4db6-945e-99d2a3e7d4dc.jpg" /> is real rather than complex. For<img src="1-7500827\801deb90-3095-4262-ad77-6bd280cf6f3b.jpg" />, one encounters resonances, which complete the spectrum. These are derived from Equations (19) and (20) by the identification</p><disp-formula id="scirp.22621-formula11557"><label>(23a)</label><graphic position="anchor" xlink:href="1-7500827\e59fe019-abcc-4dd0-8edf-3778b5fe8ddf.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11558"><label>(23b)</label><graphic position="anchor" xlink:href="1-7500827\458dd097-2ab0-4656-b398-2ca97392cbaa.jpg"  xlink:type="simple"/></disp-formula><p>The Dirac adjoint is<img src="1-7500827\5e71c57f-a208-4d3e-b864-0da0f4564f7e.jpg" />. By an elementary calculation, one shows that</p><p><img src="1-7500827\b138072f-7eef-467c-a621-6e66d09a5695.jpg" /></p><p>This can otherwise be seen as follows. One first realizes that the adjoint equation of <img src="1-7500827\2143f1ed-a972-41ea-85a9-cefeadc60e98.jpg" /> reads as<img src="1-7500827\5b653739-02f2-478c-a86e-6c4c99b3eb4e.jpg" />, and so</p><disp-formula id="scirp.22621-formula11559"><label>(24)</label><graphic position="anchor" xlink:href="1-7500827\0ce33bec-22d4-4adc-9932-4c9ca5635531.jpg"  xlink:type="simple"/></disp-formula><p>Here, we have used the adjoint equation for the “first” <img src="1-7500827\bd9ba6aa-3664-495c-814d-8141ae9ecc43.jpg" />and the original form of the imaginary-mass Dirac equation for the “second”<img src="1-7500827\8ddf068c-b3d3-4c6a-b2df-6f42b2a537c6.jpg" />.</p><p>In analogy to Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>], we define the <img src="1-7500827\8d724836-663b-493f-bfc8-9dcb8a768144.jpg" /> and <img src="1-7500827\c04dfda5-b698-4ea9-8c7d-b4f578dd5540.jpg" /> bispinors in the following normalization,</p><disp-formula id="scirp.22621-formula11560"><label>(25a)</label><graphic position="anchor" xlink:href="1-7500827\4a0a6376-a90e-477d-8f3e-d7b3e982db23.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11561"><label>(25b)</label><graphic position="anchor" xlink:href="1-7500827\642a63e4-bf8f-42eb-a410-c72e67cd4c3e.jpg"  xlink:type="simple"/></disp-formula><p>Under charge conjugation, the spinors transform as <img src="1-7500827\f6e07429-608a-40f9-b47d-acd292eb39cb.jpg" /> and<img src="1-7500827\fd8b3cbc-d32c-4dff-a5ba-4d643e100fbf.jpg" />. In analogy with Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>], we write the field operator as</p><disp-formula id="scirp.22621-formula11562"><label>(26)</label><graphic position="anchor" xlink:href="1-7500827\fb31ec84-7fb6-4fe6-8c8b-311f28eead74.jpg"  xlink:type="simple"/></disp-formula><p>Note that the <img src="1-7500827\433df957-068d-4f45-9604-48f767d6bf89.jpg" /> prescription selects the resonances (as analytic continuations of the positive-energy solutions) and antiresonances (as analytic continuations of the negative-energy solutions). This ensures that the waves are evanescent in their respective propagation direction in time. The second term in the sum in Equation (26) describes the absorption of a negative-energy tachyonic particle that propagates backward in time; this process is of course equivalent to the emission of a positive-energy antiparticle propagating forward in time by the Feinberg-Sudarshan reinterpretation principle, as explained in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>]. Thus,</p><disp-formula id="scirp.22621-formula11563"><label>(27)</label><graphic position="anchor" xlink:href="1-7500827\c97d5839-457b-439a-a40d-0b2493fb7965.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7500827\25e9f1dd-d058-4822-908c-56297e3b6ae3.jpg" /> creates antiparticles. For the imaginary-mass formalism, we postulate the same anticommutators as in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>] for the tachyonic Dirac equation,</p><disp-formula id="scirp.22621-formula11564"><label>(28a)</label><graphic position="anchor" xlink:href="1-7500827\5b9f393e-2479-445a-a398-3b6e7bfe349a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11565"><label>(28b)</label><graphic position="anchor" xlink:href="1-7500827\3dba142e-5be4-4680-935f-91e8597791a1.jpg"  xlink:type="simple"/></disp-formula><p>The nonvanishing anticommutators read as follows,&#160;</p><disp-formula id="scirp.22621-formula11566"><label>(29a)</label><graphic position="anchor" xlink:href="1-7500827\95f08934-6327-4282-a835-9c6f8c1dffff.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11567"><label>(29b)</label><graphic position="anchor" xlink:href="1-7500827\7ea70375-4491-4a5c-87c5-d3979df57889.jpg"  xlink:type="simple"/></disp-formula><p>The σ-dependent anticommutator implies that the norm of the right-handed helicity (positive chirality) neutrino one-particle state is negative, and that the righthanded helicity particle state has negative norm and can be excluded from the physical spectrum if one imposes a Gupta-Bleuler type condition (according to Chapter 3 of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>]). Likewise, antiparticles described by the imaginary-mass formalism can only exist in the right-handed helicity state. The matrix-valued tachyonic field anticommutator reads as</p><disp-formula id="scirp.22621-formula11568"><label>(30)</label><graphic position="anchor" xlink:href="1-7500827\f34b41ec-490d-4bed-8327-bb955fe40165.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7500827\2dc53478-60fb-45be-9559-4bb654845be8.jpg" /> is the helicity (for positive-energy states) and the negative of the helicity (for negative-energy states) and <img src="1-7500827\3618ae74-578e-4186-a54f-e9b28f7378d6.jpg" /> is the tensor product in bispinor space. The following two relations</p><disp-formula id="scirp.22621-formula11569"><label>(31a)</label><graphic position="anchor" xlink:href="1-7500827\8cc23add-8e31-4878-bbf6-12274e3d0417.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11570"><label>(31b)</label><graphic position="anchor" xlink:href="1-7500827\c36b2e93-40e1-434c-8f9e-cfe8baa5b489.jpg"  xlink:type="simple"/></disp-formula><p>are analogous to those found for the bispinor solutions of the tachyonic Dirac described in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref1">1</xref>]. Note that the factors <img src="1-7500827\ec97616e-42c3-4023-8721-2bb251f02f8f.jpg" /> in these equations are due to the quantization conditions (28). Using Equation (31), we can derive the compact result,</p><disp-formula id="scirp.22621-formula11571"><label>(32)</label><graphic position="anchor" xlink:href="1-7500827\81f8d4d6-742c-4897-9905-2ba00ba669b6.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7500827\7e16bceb-d9be-457a-9008-9ec5766ffcaf.jpg" /> is the distribution encountered in Equations (3.55) and (3.56) of Ref. [<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>],</p><disp-formula id="scirp.22621-formula11572"><label>(33)</label><graphic position="anchor" xlink:href="1-7500827\3715477f-f3ea-4b24-99d0-ecaaabb9cdce.jpg"  xlink:type="simple"/></disp-formula><p>The equal-time anticommutator of the fields thus reads as<img src="1-7500827\1c1a64a6-8246-42fd-af78-ed8f6759863b.jpg" />, with the full, unfiltered Dirac-δ function and <img src="1-7500827\69c64f16-2bef-4818-ab05-ed43dd50c432.jpg" /> as well as <img src="1-7500827\b82dea61-abac-4024-bf8a-e5fd0f04d2a9.jpg" /> and the time<img src="1-7500827\e59cfb19-2ad8-43f7-9ec2-a4fa8f4abd60.jpg" />. Furthermore, with the help of Equations (27) and (31), one obtains the propagator <img src="1-7500827\ba281cec-ae36-490d-ad5d-1d94a51e7010.jpg" /> (time-ordered product),</p><disp-formula id="scirp.22621-formula11573"><label>(34a)</label><graphic position="anchor" xlink:href="1-7500827\2ca20844-8b64-4aa8-bb68-468f3eaf25b2.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11574"><label>(34b)</label><graphic position="anchor" xlink:href="1-7500827\2c043214-3117-4f60-b303-a99f91763038.jpg"  xlink:type="simple"/></disp-formula><p>The chirality projectors are invariant under multiplication by<img src="1-7500827\6cfa9e77-5785-463b-ad74-5e60a477aab6.jpg" />, in view of the relation <img src="1-7500827\47e1ff11-0f85-417b-a353-0e20cc21cb05.jpg" />.</p><p>For consistency reasons, the imaginary-mass Dirac propagator should be connected with a Green function,</p><disp-formula id="scirp.22621-formula11575"><label>(35)</label><graphic position="anchor" xlink:href="1-7500827\48e85417-5d42-40f4-819e-ea5c34c2c476.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7500827\c862b62b-862f-4d0a-bf2e-88d91dc49217.jpg" /> is the energy argument of the Green function and <img src="1-7500827\3b2eed7c-f04e-49b9-91c3-739e30f1c432.jpg" /> is the imaginary-mass Dirac Hamiltonian. In momentum space, we can replace <img src="1-7500827\a5e252d9-8f16-4cf6-a220-13e5dddbce3c.jpg" /> by<img src="1-7500827\f1d1dcc0-bb64-4bf8-b078-dfdce0f2fb95.jpg" />. An elementary calculation then shows that</p><disp-formula id="scirp.22621-formula11576"><label>(36)</label><graphic position="anchor" xlink:href="1-7500827\4acbe9d0-9bfd-4636-bda3-069f2aaecc79.jpg"  xlink:type="simple"/></disp-formula><p>Introducing the <img src="1-7500827\1d346b75-5bbe-4841-83bc-978676d9cc4c.jpg" /> prescription as before, we find that</p><disp-formula id="scirp.22621-formula11577"><label>(37)</label><graphic position="anchor" xlink:href="1-7500827\8314e4af-e6d9-4c2e-ac5d-14604812b63f.jpg"  xlink:type="simple"/></disp-formula><p>Having determined the propagator, let us briefly comment on the non-invariance of the imaginary-mass Dirac Hamiltonian under time reversal. Indeed, time reversal exchanges the inand out-states of a process. In the calculation of a cross section, one has to square an invariant amplitude, which also exchanges inand out-states, and leads to the occurrence of a propagator of the form</p><disp-formula id="scirp.22621-formula11578"><label>(38)</label><graphic position="anchor" xlink:href="1-7500827\7fe09bef-c758-4454-922b-6f1a5f794b44.jpg"  xlink:type="simple"/></disp-formula><p>which is obtained from (37) under the replacement<img src="1-7500827\51e6848b-a5f4-46c3-a39e-3c1b3ca4cbf9.jpg" />. In the time-reversed Hamiltonian, according to Ref. [<xref ref-type="bibr" rid="scirp.22621-ref40">40</xref>], the same replacement takes place. So, the non-invariance under time reversal of the imaginarymass Dirac equation does not necessarily lead to an inconsistent formalism within field theory.</p></sec><sec id="s4"><title>4. Inversion of the Mass Term</title><p>It is instructive to consider the Hamiltonian which is obtained from the imaginary-mass Dirac Hamiltonian in Equation (3) by the replacement<img src="1-7500827\6b49eba5-a654-4a66-b658-d76de144953f.jpg" />, which amounts to an inversion of the sign of the mass term,</p><disp-formula id="scirp.22621-formula11579"><label>(39)</label><graphic position="anchor" xlink:href="1-7500827\ac1eb5bf-3678-4a3b-932f-f165d6ea5021.jpg"  xlink:type="simple"/></disp-formula><p>A preliminary remark is in order. Within <img src="1-7500827\a2cead2e-c175-4a1f-b754-87ce9d9fdce5.jpg" /> symmetric quantum mechanics [30-38], the one-dimensional quantum mechanical Hamiltonians <img src="1-7500827\9b22438e-89c2-46db-bd92-62badb6fc9b1.jpg" /> and <img src="1-7500827\46b436e3-c3ab-4382-b2a6-29a5ef16c12b.jpg" /> (with x being the coordinate) have been used as paradigmatic examples of an anharmonic (cubic) oscillator with imaginary coupling<img src="1-7500827\68e3f31d-5cae-4c16-b37d-8122953df8e0.jpg" />. The Hamiltonians <img src="1-7500827\fb95f388-c2d3-47aa-b2f3-53f6cfb432bc.jpg" /> and <img src="1-7500827\47bb9ff5-153d-4aba-9d01-e3ffb67b3910.jpg" /> have the same spectrum [31,33,37,38], and moreover, the eigenvalues can be shown to be analytic functions in the complex G plane where<img src="1-7500827\37e82eaf-1811-402e-945a-f6e52e9a835b.jpg" />, and the g plane has a branch cut along the negative real axis.</p><p>As is to be expected, the Hamiltonians <img src="1-7500827\a0933e6e-73a7-4768-a914-863a6abb8504.jpg" /> and <img src="1-7500827\479ba4ee-c95a-45b5-b59f-5ca9c33e1d35.jpg" /> have the same spectrum, because <img src="1-7500827\0399ad3f-5724-41c0-8c9a-17b74d10c9ff.jpg" /> fulfills the same algebraic relations (9a) and (9b) as<img src="1-7500827\913c6712-3642-41b9-ae86-463e7f71ef23.jpg" />. Moreover, the plane-wave eigenstates of <img src="1-7500827\807dc164-b887-40af-9687-c7827e7da239.jpg" /> are solutions of the covariant equation</p><disp-formula id="scirp.22621-formula11580"><label>(40)</label><graphic position="anchor" xlink:href="1-7500827\9f744356-69d7-43c4-9497-e7fac3bc4d37.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.22621-formula11581"><label>(41)</label><graphic position="anchor" xlink:href="1-7500827\936cf992-f560-4864-8587-7ac02bdaab41.jpg"  xlink:type="simple"/></disp-formula><p>for positive-energy and negative-energy states, respectively. We find</p><disp-formula id="scirp.22621-formula11582"><label>(42a)</label><graphic position="anchor" xlink:href="1-7500827\5532b8f2-4eca-4372-865b-338389d91f89.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11583"><label>(42b)</label><graphic position="anchor" xlink:href="1-7500827\a1ab6211-67b0-498a-8596-77b1f0f40ec8.jpg"  xlink:type="simple"/></disp-formula><p>The negative-energy eigenstates are given as</p><disp-formula id="scirp.22621-formula11584"><label>(43a)</label><graphic position="anchor" xlink:href="1-7500827\fee26512-c248-488a-ae58-55bc33929b05.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11585"><label>(43b)</label><graphic position="anchor" xlink:href="1-7500827\cfc398ce-73e6-4a4b-bc0a-a8bf5bb3281a.jpg"  xlink:type="simple"/></disp-formula><p>The states are normalized with respect to the condition&#160;</p><disp-formula id="scirp.22621-formula11586"><label>(44a)</label><graphic position="anchor" xlink:href="1-7500827\f996ee6c-4e73-42f6-a7dc-17b416f4df2e.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11587"><label>(44b)</label><graphic position="anchor" xlink:href="1-7500827\8d50ff18-424b-489b-9b1d-5de4d9c9ba38.jpg"  xlink:type="simple"/></disp-formula><p>We normalize the <img src="1-7500827\5cd493bc-f0a3-4204-b505-c9389ac34ac8.jpg" /> and <img src="1-7500827\6c31cc1f-aa25-4e3e-98fa-f691131124ec.jpg" /> bispinors according to</p><disp-formula id="scirp.22621-formula11588"><label>(45a)</label><graphic position="anchor" xlink:href="1-7500827\0f6a66c9-b550-42e9-917d-c6f4d75d5445.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11589"><label>(45b)</label><graphic position="anchor" xlink:href="1-7500827\db81b61a-331b-43c0-b1c0-d99af0dbe5e8.jpg"  xlink:type="simple"/></disp-formula><p>and obtain the following two relations,</p><disp-formula id="scirp.22621-formula11590"><label>(46a)</label><graphic position="anchor" xlink:href="1-7500827\56612ac8-44a1-427f-bf9a-dfb3c5758601.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11591"><label>(46b)</label><graphic position="anchor" xlink:href="1-7500827\1e930577-e7fc-4e24-96da-3d3c5378d73f.jpg"  xlink:type="simple"/></disp-formula><p>These are the analogues of Equations (31a) and (31b) and differ from Equations (31a) and (31b) by the replacement <img src="1-7500827\a1c85d5e-ee5a-46af-b659-fb8eb0839a28.jpg" /> in the numerator. However, in the denominator no change takes place, because the denominator is obtained as<img src="1-7500827\52a7dd1a-8078-4fa9-9880-779d7bbc2301.jpg" />. The field operator is</p><disp-formula id="scirp.22621-formula11592"><label>(47)</label><graphic position="anchor" xlink:href="1-7500827\97d0e0b2-e967-483a-9bcb-fe1cb3fab94d.jpg"  xlink:type="simple"/></disp-formula><p>with<img src="1-7500827\cd5daa18-d0db-4762-9c96-5cf405176c99.jpg" />, and with an obvious identification of the field operators according to Equation (27). The nonvanishing anticommutators read as follows,</p><disp-formula id="scirp.22621-formula11593"><label>(48a)</label><graphic position="anchor" xlink:href="1-7500827\1c2c3b16-2e61-4c8b-b21b-bf6c52962c14.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.22621-formula11594"><label>(48b)</label><graphic position="anchor" xlink:href="1-7500827\2fc8fd30-2b23-4aa5-9fd4-c326914b596f.jpg"  xlink:type="simple"/></disp-formula><p>These imply that the inversion of the mass term does not change the fact that again, right-handed particle and left-handed antiparticle states acquire a negative norm. It is very instructive to clarify by an explicit, detailed calculation that the inversion of the mass term does not change the pattern by which helicity components are suppressed for particle and antiparticle states.</p></sec><sec id="s5"><title>5. Conclusions</title><p>In the current work, we investigate the relativistic (tachyonic) quantum theory defined by the Hamiltonian<img src="1-7500827\1994ae14-4805-4b3c-9514-d7d0c2bcfc11.jpg" />, which is obtained from the ordinary Dirac Hamiltonian by the simple replacement<img src="1-7500827\cb8cb61b-cecd-40de-9714-7810c7c94bd3.jpg" />. In Section 2, we show that the Hamiltonian <img src="1-7500827\4a27e787-24e6-4c71-af85-db69ff1cd0fe.jpg" /> is pseudoHermitian and has an additional quasi-pseudo-Hermitian property given in Equation (9b). Eigenvalues come in a specific structure in the complex plane. Namely, if E is a resonance eigenvalue, so is<img src="1-7500827\bdc8f9fe-03f7-4fda-a1a6-df3f3b1b3b7a.jpg" />, <img src="1-7500827\f9ffbcd6-df4c-4f66-aa29-b553712aa4be.jpg" />, and<img src="1-7500827\02bbc6ef-113e-4606-88ec-706245dd750c.jpg" />. This pattern is manifest in the spectrum calculated for the tachyonic Dirac Hamiltonian <img src="1-7500827\e2c6f744-4cd5-49be-a1c8-5b1cec1af095.jpg" /> in Ref. [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>] and in the spectrum of <img src="1-7500827\2b9cfa90-2897-48d8-87ee-4c41eed2747a.jpg" /> calculated here. Plane-wave solutions of the imaginary-mass Dirac equation are given in Equations (19) and (20).</p><p>In Section 3, we complement recent work on the tachyonic Dirac Hamiltonian [<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>] and discuss the quantization of the spin one-half theory defined by the imaginary-mass Dirac Hamiltonian. We find helicity-dependent anticommutators as given in Equation (28). For both the imaginarymass as well as the tachyonic Dirac Hamiltonian, the oneparticle states of right-handed helicity acquire a negative norm and can be excluded from the physical spectrum by a Gupta-Bleuler type condition. Likewise, antiparticle states of left-handed helicity are excluded from the physical spectrum. Compact representations are found for the spin sums (31) which enter the field anticommutator and the propagator. In Section 4, we find that an inversion of the mass term does not change the fact that only left-handed helicity is allowed for particles described by a tachyonic generalization of the Dirac equation, and only right-handed helicity for antiparticles.</p><p>Obviously, the left-handedness of particle states and the right-handedness of antiparticles states imply that both the tachyonic Dirac equation as well as the imaginary-mass Dirac equation represent candidates for the description of neutrinos, if improved experimental techniques [10,18,19,41,42] finally allow us to decide if neutrinos propagate at superluminal or subluminal speeds, which would amount to deciding whether the neutrino mass square is positive or negative [9-16].</p></sec><sec id="s6"><title>6. Acknowledgements</title><p>This work was supported by the NSF and by the National Institute of Standards and Technology (precision measurement grant). The author acknowledges helpful conversations with B. J. Wundt.</p></sec><sec id="s7"><title>REFERENCE</title><p>[<xref ref-type="bibr" rid="scirp.22621-ref1">1</xref>]&#160;&#160; U. D. Jentschura and B. J. Wundt, “Pseudo-Hermitian Quantum Dynamics of Tachyonic Spin-1/2 Particles,” Journal of Physics A: Mathematical and Theoretical, e-print arXiv: 1110.4171, in Press.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref2">2</xref>]&#160;&#160; U. D. Jentschura and B. J. Wundt, “Localizability of Tachyonic Particles and Neutrinoless Double Beta Decay,” The European Physical Journal C—Particles and Fields, Vol. 72, No. 2, 2012, p. 1894. doi:10.1140/epjc/s10052-012-1894-4</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref3">3</xref>]&#160;&#160; O. M. P. Bilaniuk, V. K. Deshpande and E. C. G. Sudarshan, “‘Meta’ Relativity,” American Journal of Physics, Vol. 30, No. 10, 1962, p. 718. doi:10.1119/1.1941773</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref4">4</xref>]&#160;&#160; G. Feinberg, “Possibility of Faster-than-Light Particles,” Physical Review, Vol. 159, No. 5, 1967, p. 1089. doi:10.1103/PhysRev.159.1089</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref5">5</xref>]&#160;&#160; M. E. Arons and E. C. G. Sudarshan, “Lorentz Invariance, Local Field Theory, and Faster-than-Light Particles,” Physical Review, Vol. 173, No. 5, 1968, p. 1622. doi:10.1103/PhysRev.173.1622</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref6">6</xref>]&#160;&#160; J. Dhar and E. C. G. Sudarshan, “Quantum Field Theory of Interacting Tachyons,” Physical Review, Vol. 174, No. 5, 1968, p. 1808. doi:10.1103/PhysRev.174.1808</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref7">7</xref>]&#160;&#160; O.-M. Bilaniuk and E. C. G. Sudarshan, “Causality and Space-Like Signals,” Nature, Vol. 223, 1969, pp. 386-387. doi:10.1038/223386b0</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref8">8</xref>]&#160;&#160; G. Feinberg, “Lorentz Invariance of Tachyon Theories,” Physical Review D, Vol. 17, No. 6, 1978, p. 1651. doi:10.1103/PhysRevD.17.1651</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref9">9</xref>]&#160;&#160; http://cupp.oulu.fi/neutrino/nd-mass.html</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref10">10</xref>] R. G. H. Robertson, T. J. Bowles, G. J. Stephenson, D. L. Wark, J. F. Wilkerson and D. A. Knapp, “Limit on <img src="1-7500827\6909138d-a016-456c-b3d8-545b2b2ee214.jpg" /> Mass from Observation of the β Decay of Molecular Tritium,” Physical Review Letters, Vol. 67, No. 8, 1991, p. 957. doi:10.1103/PhysRevLett.67.957</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref11">11</xref>] K. Assamagan, et al., “Measurement of the Muon Momentum in Pion Decay at Rest Using a Surface Muon Beam,” Physical Letters B, Vol. 335, No. 2, 1994, pp. 231- 236. doi:10.1016/0370-2693(94)91419-2</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref12">12</xref>] W. Stoeffl and D. J. Decman, “Anomalous Structure in the Beta Decay of Gaseous Molecular Tritium,” Physical Review Letters, Vol. 75, No. 18, 1995, p. 3237. doi:10.1103/PhysRevLett.75.3237</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref13">13</xref>] K. Assamagan, et al., “Upper Limit of the Muon-Neutrino Mass and Charged-Pion Mass from Momentum Analysis of a Surface Muon Beam,” Physical Review D, Vol. 53, No. 11, 1996, p. 6065. doi:10.1103/PhysRevD.53.6065</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref14">14</xref>] C. Weinheimer, B. Degen, A. Bleile, J. Bonn, L. Bornschein, O. Kazachenko, A. Kovalik and E. Otten, “High Precision Measurement of the Tritium Β Spectrum near Its Endpoint and upper Limit on the Neutrino Mass,” Physics Letters B, Vol. 460, No. 1-2, 1999, pp. 219-226. doi:10.1016/S0370-2693(99)00780-7</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref15">15</xref>] V. M. Lobashev, et al., “Direct Search for Mass of Neutrino and Anomaly in the Tritium Beta-Spectrum,” Physics Letters B, Vol. 460, No. 1-2, 1999, pp. 227-235. doi:10.1016/S0370-2693(99)00781-9</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref16">16</xref>] A. I. Belesev, et al., “Investigation of Space-Charge Effects in Gaseous Tritium as a Source of Distortions of the Beta Spectrum Observed in the Troitsk Neutrino-Mass Experiment,” Physics of Atomic Nuclei, Vol. 71, No. 3, 2008, pp. 427-436. doi:10.1134/S1063778808030046</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref17">17</xref>] G. R. Kalbfleisch, N. Baggett, E. C. Fowler and J. Alspector, “Experimental Comparison of Neutrino, Antineutrino, and Muon Velocities,” Physical Review Letters, Vol. 43, No. 19, 1979, p. 1361. doi:10.1103/PhysRevLett.43.1361</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref18">18</xref>] P. Adamson, et al., “Measurement of Neutrino Velocity with the MINOS Detectors and NuMI Neutrino Beam,” Physical Review D, Vol. 76, No. 7, 2007, p. 072005. doi:10.1103/PhysRevD.76.072005</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref19">19</xref>] M. Antonello, et al., “ICARUS Collaboration, Measurement of the Neutrino Velocity with the ICARUS Detector at the CNGS Beam,” e-print arXiv: 1203.3433v3.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref20">20</xref>] J. Ciborowski, “Hypothesis of Tachyonic Neutrinos,” Acta Physica Polonica B, Vol. 29, No. 1-2, 1998, pp. 113- 121.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref21">21</xref>] M. Dracos, “On Behalf of the OPERA Collaboration, the Neutrino Velocity Measurement by OPERA Experiment,” The XXV International Conference on Neutrino Physics and Astrophysics, Kyoto, 3-9 June 2012, 15 p. http://regmedia.co.uk/2012/06/11/neutrinos_not_ftl_slides.pdf</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref22">22</xref>] A. Chodos, A. I. Hauser and V. A. Kostelecky, “The Neutrino as a Tachyon,” Physics Letters B, Vol. 150, No. 6, 1985, pp. 431-435. doi:10.1016/0370-2693(85)90460-5</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref23">23</xref>] A. Chodos, V. A. Kostelecky, R. Potting and E. Gates, “Null Experiments for Neutrino Masses,” Modern Physics Letters A, Vol. 7, No. 6, 1992, p. 467. doi:10.1142/S0217732392000422</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref24">24</xref>] A. Chodos and V. A. Kostelecky, “Nuclear Null Tests for Spacelike Neutrinos,” Physics Letters B, Vol. 336, No. 3-4, 1994, pp. 295-302. doi:10.1016/0370-2693(94)90535-5</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref25">25</xref>] J. Rembielinski, “Tachyons and Preferred Frames,” International Journal of Modern Physics A, Vol. 12, No. 9, 1997, p. 1677.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref26">26</xref>] T. Chang, “A New Dirac-Type Equation for Tachyonic Neutrinos,” e-print arXiv: hep-th/0011087.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref27">27</xref>] T. Chang, “Parity Violation and a Preferred Frame,” e-print arXiv: quant-ph/0204002.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref28">28</xref>] J. Bandukwala and D. Shay, “Theory of Free, Spin-$1/2$ Tachyons,” Physical Review D, Vol. 9, No. 4, 1974, p. 889. doi:10.1103/PhysRevD.9.889</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref29">29</xref>] W. Pauli, “On Dirac’s New Method of Field Quantization,” Reviews of Modern Physics, Vol. 15, No. 3, 1943, p. 175. doi:10.1103/RevModPhys.15.175</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref30">30</xref>] C. M. Bender and S. Boettcher, “Real Spectra in NonHermitian Hamiltonians Having PT Symmetry,” Physical Review Letters, Vol. 80, No. 24, 1998, p. 5243. doi:10.1103/PhysRevLett.80.5243</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref31">31</xref>] C. M. Bender and G. V. Dunne, “Large-Order Perturbation Theory for a Non-Hermitian PT-Symmetric Hamiltonian,” Journal of Mathematical Physics, Vol. 40, No. 10, 1999, pp. 4616-4621. doi:10.1063/1.532991</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref32">32</xref>] C. M. Bender, S. Boettcher and P. N. Meisinger, “PT-Symmetric Quantum Mechanics,” Journal of Mathematical Physics, Vol. 40, No. 5, 1999, pp. 2201-2229. doi:10.1063/1.532860</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref33">33</xref>] C. M. Bender and E. J. Weniger, “Numerical Evidence That the Perturbation Expansion for a Non-Hermitian PT-Symmetric Hamiltonian Is Stieltjes,” Journal of Mathematical Physics, Vol. 42, No. 5, 2001, pp. 2167-2183. doi:10.1063/1.1362287</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref34">34</xref>] C. M. Bender, D. C. Brody and H. F. Jones, “Complex Extension of Quantum Mechanics,” Physical Review Letters, Vol. 89, No. 27, 2002, Article ID: 270401. doi:10.1103/PhysRevLett.89.270401</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref35">35</xref>] A. Mostafazadeh, “Pseudo-Hermiticity versus PT-Symmetry III: Equivalence of Pseudo-Hermiticity and the Presence of Antilinear Symmetries,” Journal of Mathematical Physics, Vol. 43, No. 8, 2002, pp. 3944-3951. doi:10.1063/1.1489072</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref36">36</xref>] A. Mostafazadeh, “Pseudo-Hermiticity and Generalized PTand CPT-Symmetries,” Journal of Mathematical Physics, Vol. 44, No. 3, 2003, pp. 974-989. doi:10.1063/1.1539304</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref37">37</xref>] U. D. Jentschura, A. Surzhykov and J. Zinn-Justin, “Unified Treatment of Even and Odd Anharmonic Oscillators of Arbitrary Degree,” Physical Review Letters, Vol. 102, No. 1, 2009, Article ID: 011601. doi:10.1103/PhysRevLett.102.011601</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref38">38</xref>] U. D. Jentschura, A. Surzhykov and J. Zinn-Justin, “MultiInstantons and Exact Results III: Unification of Even and Odd Anharmonic Oscillators,” Annals of Physics, Vol. 325, No. 5, 2010, pp. 1135-1172. doi:10.1016/j.aop.2010.01.002</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref39">39</xref>] C. Itzykson and J. B. Zuber, “Quantum Field Theory,” McGraw-Hill, New York, 1980.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref40">40</xref>] C. M. Bender, J. Brod, A. Refig and M. E. Reuter, “The C Operator in PT-Symmetric Quantum Theories,” Journal of Physics A: Mathematical and General, Vol. 37, No. 43, 2004, p. 10139. doi:10.1088/0305-4470/37/43/009</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref41">41</xref>] R. M. Bionta, “Detection of a Rare Event on 23 February 1987 by the Neutrino Radiation Detector under Mont Blanc,” JETP Letters, Vol. 45, No. 10, 1987, pp. 593-595.</p><p>[<xref ref-type="bibr" rid="scirp.22621-ref42">42</xref>] T. Adam, et al., “OPERA Collaboration, Measurement of the Neutrino Velocity with the OPERA Detector in the CNGS Beam,” e-print arXiv: 1109.4897v4.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.22621-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">U. D. Jentschura and B. J. Wundt, “Pseudo-Hermitian Quan- tum Dynamics of Tachyonic Spin-1/2 Particles,” Journal of Physics A: Mathematical and Theoretical, e-print arXiv: 1110.4171, in Press.</mixed-citation></ref><ref id="scirp.22621-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">U. D. Jentschura and B. J. Wundt, “Localizability of Tachyonic Particles and Neutrinoless Double Beta Decay,” The European Physical Journal C—Particles and Fields, Vol. 72, No. 2, 2012, p. 1894. 
doi:10.1140/epjc/s10052-012-1894-4</mixed-citation></ref><ref id="scirp.22621-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">O. M. P. Bilaniuk, V. K. Deshpande and E. C. G. Sudarshan, “‘Meta’ Relativity,” American Journal of Physics, Vol. 30, No. 10, 1962, p. 718. doi:10.1119/1.1941773</mixed-citation></ref><ref id="scirp.22621-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">G. Feinberg, “Possibility of Faster-than-Light Particles,” Physical Review, Vol. 159, No. 5, 1967, p. 1089. 
doi:10.1103/PhysRev.159.1089</mixed-citation></ref><ref id="scirp.22621-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">M. E. Arons and E. C. G. Sudarshan, “Lorentz Invariance, Local Field Theory, and Faster-than-Light Particles,” Physical Review, Vol. 173, No. 5, 1968, p. 1622. 
doi:10.1103/PhysRev.173.1622</mixed-citation></ref><ref id="scirp.22621-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">J. Dhar and E. C. G. Sudarshan, “Quantum Field Theory of Interacting Tachyons,” Physical Review, Vol. 174, No. 5, 1968, p. 1808. doi:10.1103/PhysRev.174.1808 </mixed-citation></ref><ref id="scirp.22621-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">O.-M. Bilaniuk and E. C. G. Sudarshan, “Causality and Space-Like Signals,” Nature, Vol. 223, 1969, pp. 386-387. 
doi:10.1038/223386b0</mixed-citation></ref><ref id="scirp.22621-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">G. Feinberg, “Lorentz Invariance of Tachyon Theories,” Physical Review D, Vol. 17, No. 6, 1978, p. 1651. 
doi:10.1103/PhysRevD.17.1651</mixed-citation></ref><ref id="scirp.22621-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">http://cupp.oulu.fi/neutrino/nd-mass.html</mixed-citation></ref><ref id="scirp.22621-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">R. G. H. Robertson, T. J. Bowles, G. J. Stephenson, D. L. Wark, J. F. Wilkerson and D. A. Knapp, “Limit on   Mass from Observation of the β Decay of Molecular Tritium,” Physical Review Letters, Vol. 67, No. 8, 1991, p. 957. 
doi:10.1103/PhysRevLett.67.957</mixed-citation></ref><ref id="scirp.22621-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">K. Assamagan, et al., “Measurement of the Muon Momentum in Pion Decay at Rest Using a Surface Muon Beam,” Physical Letters B, Vol. 335, No. 2, 1994, pp. 231- 236. doi:10.1016/0370-2693(94)91419-2</mixed-citation></ref><ref id="scirp.22621-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">W. Stoeffl and D. J. Decman, “Anomalous Structure in the Beta Decay of Gaseous Molecular Tritium,” Physical Review Letters, Vol. 75, No. 18, 1995, p. 3237. 
doi:10.1103/PhysRevLett.75.3237</mixed-citation></ref><ref id="scirp.22621-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">K. Assamagan, et al., “Upper Limit of the Muon-Neutrino Mass and Charged-Pion Mass from Momentum Analysis of a Surface Muon Beam,” Physical Review D, Vol. 53, No. 11, 1996, p. 6065. doi:10.1103/PhysRevD.53.6065</mixed-citation></ref><ref id="scirp.22621-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">C. Weinheimer, B. Degen, A. Bleile, J. Bonn, L. Bornschein, O. Kazachenko, A. Kovalik and E. Otten, “High Precision Measurement of the Tritium Β Spectrum near Its Endpoint and upper Limit on the Neutrino Mass,” Physics Letters B, Vol. 460, No. 1-2, 1999, pp. 219-226. 
doi:10.1016/S0370-2693(99)00780-7</mixed-citation></ref><ref id="scirp.22621-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">V. M. Lobashev, et al., “Direct Search for Mass of Neutrino and Anomaly in the Tritium Beta-Spectrum,” Physics Letters B, Vol. 460, No. 1-2, 1999, pp. 227-235. 
doi:10.1016/S0370-2693(99)00781-9</mixed-citation></ref><ref id="scirp.22621-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">A. I. Belesev, et al., “Investigation of Space-Charge Effects in Gaseous Tritium as a Source of Distortions of the Beta Spectrum Observed in the Troitsk Neutrino-Mass Experiment,” Physics of Atomic Nuclei, Vol. 71, No. 3, 2008, pp. 427-436. doi:10.1134/S1063778808030046</mixed-citation></ref><ref id="scirp.22621-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">G. R. Kalbfleisch, N. Baggett, E. C. Fowler and J. Alspector, “Experimental Comparison of Neutrino, Antineutrino, and Muon Velocities,” Physical Review Letters, Vol. 43, No. 19, 1979, p. 1361. 
doi:10.1103/PhysRevLett.43.1361</mixed-citation></ref><ref id="scirp.22621-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">P. Adamson, et al., “Measurement of Neutrino Velocity with the MINOS Detectors and NuMI Neutrino Beam,” Physical Review D, Vol. 76, No. 7, 2007, p. 072005. 
doi:10.1103/PhysRevD.76.072005</mixed-citation></ref><ref id="scirp.22621-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">M. Antonello, et al., “ICARUS Collaboration, Measurement of the Neutrino Velocity with the ICARUS Detector at the CNGS Beam,” e-print arXiv: 1203.3433v3.</mixed-citation></ref><ref id="scirp.22621-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">J. Ciborowski, “Hypothesis of Tachyonic Neutrinos,” Acta Physica Polonica B, Vol. 29, No. 1-2, 1998, pp. 113-121.</mixed-citation></ref><ref id="scirp.22621-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">M. Dracos, “On Behalf of the OPERA Collaboration, the Neutrino Velocity Measurement by OPERA Experiment,” the XXV International Conference on Neutrino Physics and Astrophysics, Kyoto, 3-9 June 2012, 15 p. 
http://regmedia.co.uk/2012/06/11/neutrinos_not_ftl_slides.pdf</mixed-citation></ref><ref id="scirp.22621-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">A. Chodos, A. I. Hauser and V. A. Kostelecky, “The Neutrino as a Tachyon,” Physics Letters B, Vol. 150, No. 6, 1985, pp. 431-435. doi:10.1016/0370-2693(85)90460-5</mixed-citation></ref><ref id="scirp.22621-ref23"><label>23</label><mixed-citation publication-type="other" xlink:type="simple">A. Chodos, V. A. Kostelecky, R. Potting and E. Gates, “Null Experiments for Neutrino Masses,” Modern Physics Letters A, Vol. 7, No. 6, 1992, p. 467. 
doi:10.1142/S0217732392000422</mixed-citation></ref><ref id="scirp.22621-ref24"><label>24</label><mixed-citation publication-type="other" xlink:type="simple">A. Chodos and V. A. Kostelecky, “Nuclear Null Tests for Spacelike Neutrinos,” Physics Letters B, Vol. 336, No. 3-4, 1994, pp. 295-302. doi:10.1016/0370-2693(94)90535-5</mixed-citation></ref><ref id="scirp.22621-ref25"><label>25</label><mixed-citation publication-type="other" xlink:type="simple">J. Rembielinski, “Tachyons and Preferred Frames,” International Journal of Modern Physics A, Vol. 12, No. 9, 1997, p. 1677.</mixed-citation></ref><ref id="scirp.22621-ref26"><label>26</label><mixed-citation publication-type="other" xlink:type="simple">T. Chang, “A New Dirac-Type Equation for Tachyonic Neutrinos,” e-print arXiv: hep-th/0011087.</mixed-citation></ref><ref id="scirp.22621-ref27"><label>27</label><mixed-citation publication-type="other" xlink:type="simple">T. Chang, “Parity Violation and a Preferred Frame,” e-print arXiv: quant-ph/0204002.</mixed-citation></ref><ref id="scirp.22621-ref28"><label>28</label><mixed-citation publication-type="other" xlink:type="simple">J. Bandukwala and D. Shay, “Theory of Free, Spin-$1/2$ Tachyons,” Physical Review D, Vol. 9, No. 4, 1974, p. 889. 
doi:10.1103/PhysRevD.9.889</mixed-citation></ref><ref id="scirp.22621-ref29"><label>29</label><mixed-citation publication-type="other" xlink:type="simple">W. Pauli, “On Dirac’s New Method of Field Quantization,” Reviews of Modern Physics, Vol. 15, No. 3, 1943, p. 175. doi:10.1103/RevModPhys.15.175</mixed-citation></ref><ref id="scirp.22621-ref30"><label>30</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender and S. Boettcher, “Real Spectra in Non-Hermitian Hamiltonians Having PT Symmetry,” Physical Review Letters, Vol. 80, No. 24, 1998, p. 5243. 
doi:10.1103/PhysRevLett.80.5243</mixed-citation></ref><ref id="scirp.22621-ref31"><label>31</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender and G. V. Dunne, “Large-Order Perturbation Theory for a Non-Hermitian PT-Symmetric Hamiltonian,” Journal of Mathematical Physics, Vol. 40, No. 10, 1999, pp. 4616-4621. doi:10.1063/1.532991</mixed-citation></ref><ref id="scirp.22621-ref32"><label>32</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender, S. Boettcher and P. N. Meisinger, “PT-Symmetric Quantum Mechanics,” Journal of Mathematical Physics, Vol. 40, No. 5, 1999, pp. 2201-2229. 
doi:10.1063/1.532860</mixed-citation></ref><ref id="scirp.22621-ref33"><label>33</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender and E. J. Weniger, “Numerical Evidence That the Perturbation Expansion for a Non-Hermitian PT-Symmetric Hamiltonian Is Stieltjes,” Journal of Mathematical Physics, Vol. 42, No. 5, 2001, pp. 2167-2183. 
doi:10.1063/1.1362287</mixed-citation></ref><ref id="scirp.22621-ref34"><label>34</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender, D. C. Brody and H. F. Jones, “Complex Extension of Quantum Mechanics,” Physical Review Letters, Vol. 89, No. 27, 2002, p. 270401. 
doi:10.1103/PhysRevLett.89.270401</mixed-citation></ref><ref id="scirp.22621-ref35"><label>35</label><mixed-citation publication-type="other" xlink:type="simple">A. Mostafazadeh, “Pseudo-Hermiticity versus PT-Symmetry III: Equivalence of Pseudo-Hermiticity and the Presence of Antilinear Symmetries,” Journal of Mathematical Physics, Vol. 43, No. 8, 2002, pp. 3944-3951. 
doi:10.1063/1.1489072</mixed-citation></ref><ref id="scirp.22621-ref36"><label>36</label><mixed-citation publication-type="other" xlink:type="simple">A. Mostafazadeh, “Pseudo-Hermiticity and Generalized PT- and CPT-Symmetries,” Journal of Mathematical Physics, Vol. 44, No. 3, 2003, pp. 974-989. 
doi:10.1063/1.1539304</mixed-citation></ref><ref id="scirp.22621-ref37"><label>37</label><mixed-citation publication-type="other" xlink:type="simple">U. D. Jentschura, A. Surzhykov and J. Zinn-Justin, “Unified Treatment of Even and Odd Anharmonic Oscillators of Arbitrary Degree,” Physical Review Letters, Vol. 102, No. 1, 2009, p. 011601. 
doi:10.1103/PhysRevLett.102.011601</mixed-citation></ref><ref id="scirp.22621-ref38"><label>38</label><mixed-citation publication-type="other" xlink:type="simple">U. D. Jentschura, A. Surzhykov and J. Zinn-Justin, “Multi-Instantons and Exact Results III: Unification of Even and Odd Anharmonic Oscillators,” Annals of Physics, Vol. 325, No. 5, 2010, pp. 1135-1172. 
doi:10.1016/j.aop.2010.01.002</mixed-citation></ref><ref id="scirp.22621-ref39"><label>39</label><mixed-citation publication-type="other" xlink:type="simple">C. Itzykson and J. B. Zuber, “Quantum Field Theory,” McGraw-Hill, New York, 1980.</mixed-citation></ref><ref id="scirp.22621-ref40"><label>40</label><mixed-citation publication-type="other" xlink:type="simple">C. M. Bender, J. Brod, A. Refig and M. E. Reuter, “The C Operator in PT-Symmetric Quantum Theories,” Journal of Physics A: Mathematical and General, Vol. 37, No. 43, 2004, p. 10139. doi:10.1088/0305-4470/37/43/009</mixed-citation></ref><ref id="scirp.22621-ref41"><label>41</label><mixed-citation publication-type="other" xlink:type="simple">R. M. Bionta, “Detection of a Rare Event on 23 February 1987 by the Neutrino Radiation Detector under Mont Blanc,” JETP Letters, Vol. 45, No. 10, 1987, pp. 593-595.</mixed-citation></ref><ref id="scirp.22621-ref42"><label>42</label><mixed-citation publication-type="other" xlink:type="simple">T. Adam, et al., “OPERA Collaboration, Measurement of the Neutrino Velocity with the OPERA Detector in the CNGS Beam,” e-print arXiv: 1109.4897v4.</mixed-citation></ref></ref-list></back></article>