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Harry J. Lipkin

Publications and source records attributed to Harry J. Lipkin.

At least 19 recordsLinked to original sources

Why do neutrinos with different masses interfere and oscillate? Why are states with different masses but same energy coherent? Overcoming barrier between particle & condensed matter physics

Neutrino oscillations occur only if it is impossible to determine $ν$ mass by using conservation laws on measurements of nucleon-lepton system absorbing $ν$. No oscillations if $ν$ detector is mass spectrometer. Beam is split into components with different masses entering different counters. For each event only one counter will click and determine $ν$ mass. Condensed matter physics needed to describe the $ν$ detector, show it is not a mass spectrometer and identify which properties of the incident $ν$ are unobservable. Relativistic quantum field theory can only describe $ν$ wave function entering detector but not large uncertain momentum transfers to detector nor associated energy-momentum asymmetry. Absorption of incident $ν$'s with different momenta but same energy leaves no trace of initial $ν$ momentum difference in finite-size $ν$ detector with effectively infinite mass at rest in laboratory. Undetectable recoil-free momentum is transferred to the detector with negligible energy transfer. The Debye-Waller factor common in X-ray diffraction by crystals gives probability that absorbing $ν$'s with different momenta produce same nucleon-charged-lepton final state. Oscillations in time described in textbooks as interference between $ν$ states with different energies not observable in realistic experiments. Different energy $ν$'s not coherent because energy can be determined by measurements on initial and final states. Experiments detecting $ν$ produced by $πto μν$ decay observe no electrons even though $ν$ mass eigenstates produce electrons. Electron amplitude canceled by interference between amplitudes from different $ν$ mass eigenstates with same energy and different momenta entering massive detector.

hep-ph

Entangled symmetries explain without QCD dynamics CP violation in neutral B to Kpi decays; not in charged B decays Unexpected isospin relations in charged and neutral decays,

Simple flavor symmetry argument without QCD dynamics shows why CP violation observed in neutral $B$ to $Kπ$ decays is absent in charged B decays where tree diagram final state has two $u$ quarks satisfying Pauli principle. Entanglement preserves short range symmetry correlations after separation into two mesons. Pauli principle and symmetries require totally flavor-symmetric tree diagram final state. $ππ$ isospin state with I=2 already is flavor symmetric and suffers no symmetry constraint. Strange flavor-symmetric state with V spin V=2 is linear combination of $Kπ$ and $K η$ with probability only (1/4) for $Kπ$. Tree diagram suppression by factor 4 not present in neutral decays explains negligible tree-penguin interference and CP violation in charged decays. Detailed full symmetry analysis shows constraints from space-inversion, charge conjugation, Pauli antisymmetrization and flavor symmetry. Two antiquarks produced at same space point by tree diagram have even parity. Even parity final state requires even parity, even space symmetry and color-spin antisymmetry for two $u$ quarks. Color-singlet spin-singlet final state requires color-spin antisymmetry and therefore flavor symmetry for two-antiquark wave function. Flavor symmetric $\bar u \bar d$ and $\bar u \bar s$ antiquark pairs have isospin I=1 and V-spin V =1. Generalized charge conjugation invariance requires I=2 for $ππ$ tree diagram and V = 2 for $Kπ$. Penguin decays give I = 1/2 final state and no CP violation. Experiments confirm surprising predictions from tree suppression factor not noted in previous analyzes. I=1/2 violations seen only in relation between charged and neutral decays together with no I=3/2 components in each individual decay. Common treatments using $ππ$ data fail to fit $Kπ$ data.

hep-ph

Directed Spontaneous Emission from $N$-atom Extended Ensemble

Coherence and interference play crucial roles in emission and absorption of photons to and from large systems with many atoms. Confusion has arisen because nuclear X-ray physicists and atomic quantum-optics physicists do not understand one another's individual descriptions of related phenomena. Basic physics same for all wave lengths from optical to nuclear gamma ray photons. But different languages are used to describe this physics in different domains. Crucial parameters vary over many orders of magnitude and what is intuitive or counterintuitive varies widely. Differences in parameters arising from differences between coherent emission effects in different domains produce very different results. Unified general treatment of the entire photon spectrum makes basic physics intelligible to all. In the optical region the mean distance between the scattering atoms is much longer than the photon wave length, Dicke superradiant scattering is isotropic and multiple scattering, Fano couplings are important and the lifetimes of intermediate stats are sufficiently short to be negligible. In X-ray scattering the mean distance between atoms is comparable to the photon wave length, Dicke superradiance is concentrated in a forward peak, multiple scattering and Fano effects are negligible, lifetimes are measurably long, speedup shortening the lifetime is important and most of the radiation is not elastically scattered but lost to absorption. Explicit calculations for a one-dimensional array shows the great difference between the case where the photon wave length is much shorter or comparable to the distance between nearest neighbors. A full investigation of the angular distribution and speedup of the intensity for two and three-dimensional scatterers give very different results for the two cases.

cond-mat.other

Simple quantum mechanics explains GSI Darmstadt oscillations Even with undetected neutrino; Momentum conservation requires Same interference producing oscillations in initial and final states

GSI experiment studying oscillations in K-capture decay of radioactive ion investigates neutrino masses and mixing without detecting neutrino. Even when neutrino is not detected quantum mechanics relates initial and final states. The basic physics is very simple. Neutrinos emitted in beta decay are coherent linear combinations of states with different masses, different momenta and same energy. Since the weak interaction producing the neutrino conserves momentum, the initial state before the transition must also contain a coherent linear combination of states with the same momentum difference and a well defined relative magnitude and phase. A one-particle state with a definite momentum difference also has an easily calculated energy difference. In the time interval between creation of the ion and its decay a linear combination of two states with different energies oscillates in time. Measuring the oscillation period gives a value for the difference between squared neutrino masses of the two neutrino mass eigenstates. The value obtained from a crude approximation with no free parameters for this "two-slit" or "which path" experiment in momentum space differs by less than 10% from the result observed in the KAMLAND experiment. Observing only ion disappearance without detecting neutrino avoids signal suppression by low neutrino absorption cross section

hep-ph

Pauli blocking and entanglement solve $Kπ$ puzzle. CP violation in $B^o \rightarrow Kπ$; not in $B^{\pm} \rightarrow Kπ$decays

New data analysis with Pauli blocking and entanglement explains CP violation in $B^o\rightarrow Kπ$ decays, absence in $B^{\pm} \rightarrow Kπ$ decays and predicts unexpected contrast between pure I=1/2 in individual $B^{\pm}$ and $B^o$ final states and I=1/2 violation in relations between them. Analysis of $B\rightarrow Kπ$ data predicts these observed isospin relations and explains dependence on spectator quark flavor. $B^+ \rightarrow Kπ$ tree diagram $\bar b u\rightarrow \bar s u \bar u u$ has two identical $u$ quarks from weak vertex and spectator. The Pauli principle requires these quarks at short distances to have wave functions antisymmetric in color or spin. The eigenvalues of conserved symmetries remain entangled in a final state of two separated mesons. This Pauli entanglement suppresses tree-penguin interference and CP violation in $B^+$ decay but not in $B^o$ decay with spectator $d$ quark. The four-body wave function must have two antiquarks with the same symmetry combining with two u-quarks to fragment into a two-pseudoscalar-meson state even under charge conjugation with angular momentum zero. It is classified in the 27-dimensional representation of flavor SU(3) with isospin I=2 for the $ππ$ state and V spin V=2 for the corresponding strange state which is linear combination of $Kπ$ and $Kη_8$. These symmetries remain entangled in four-body wave function even after separation into two mesons. Strong Pauli suppression in tree transitions to $Kπ$ which has only a small V=2 component and is mainly V=1. No Pauli suppression in transitions to I=2 $ππ$ state with also two $u$ quarks but different color-spin couplings. Standard definition of independent color favored and suppressed tree diagrams in $B^\pm\rightarrow Kπ$ decays neglects $uu$ Pauli entanglement.

hep-ph

Heavy Baryons and Exotics Spectrum

We discuss several highly accurate theoretical predictions for masses of baryons containing the b quark which have been recently confirmed by experimental data. Several predictions are given for additional properties of heavy baryons. We also discuss the two charged exotic resonances Z_b with quantum numbers of a (b bbar u ddbar) tetraquark, very recently reported by Belle in the channel [Upsilon(nS) π^+, n=1,2,3]. Among possible implications are deeply bound I=0 counterparts of the Z_b-s and existence of a Sigma_b^+ Sigma_b^- dibaryon, a "beauteron".

hep-ph

New Analysis of $B \rightarrow Kπ$ data with Pauli blocking CP violation in $B^o$ decays, not in $B^{\pm}$ SU(3) use of $B \rightarrow ππ$ data invalid for $B \rightarrow Kπ$

New data analysis with Pauli blocking explains observation of CP violation in $B^o\rightarrow Kπ$ decays, absence in $B^{\pm} \rightarrow Kπ$ decays and gives new predictions agreeing with experiment. Branching ratio data show pure I=1/2 amplitude predicted by pure penguin transitions for separate relations within charged and neutral B decays, but strong violation of penguin I=1/2 isospin relation between charged and neutral decays. $B(B^o \rightarrow K^+ π^-) - 2B(B^o\rightarrow K^o π^o) = %(19.4 \pm 0.6)- 2\cdot (9.4 \pm 0.6) = (0.6 \pm 1.3)\cdot 10^-6 \approx 0$ $2B(B^+ \rightarrow K^+ π^o) - B(B^+ \rightarrow K^o π^+) = %(25.8\pm 1.2) - (23.1 \pm 1.0) = (2.7 \pm 1.6)\cdot 10^-6 \approx 0$ ${{τ^o}\over{τ^+}}\cdot 2B(B^+ \rightarrow K^+ π^o) - B(B^o \rightarrow K^+ π^-) = (4.7 \pm 0.82)\cdot 10^-6 \not= 0$ This contrast between pure I=1/2 observed in individual charged and neutral final states and I=1/2 violation in relations between them is unexpected in previous treatments. Pauli blocking predicts this contrast by noting that two identical $u$ quarks in a relative s-wave are Pauli blocked. Tree diagram $\bar b\rightarrow \bar s u \bar u$ for $\bar b$ producing $u$ quark at weak vertex and tree-penguin interference producing CP violation are Pauli suppressed for $B^+$ decays with identical $u$ quark spectator. No suppression in $B^o$ decays with spectator $d$ quark. $B\rightarrow Kπ$ data analysis discards all amplitudes containing two identical $u$ quarks in final state and predicts observed isospin relations by using only Pauli-favored amplitudes ${B_u}\rightarrow \bar s du \bar d$ and ${B_d}\rightarrow \bar s ud \bar u$. Pauli-favored transitions explain dependence on flavor of spectator quark which does not participate in the weak interaction.

hep-ph

New $B^{\pm}\to Kπ$ data explain absence of CP violation Tree-penguin interference canceled by Pauli effects

Observation of CP violation in $B^o\to K^\pmπ^{\mp}$ decays and its absence in $B^+\to K^+π^o$ decays are explained in new improved data analysis of more precise $B\to Kπ$ data. Success of the "Lipkin Sum Rule" indicates that four $B\tow Kπ$ branching ratios are determined by three parameters, the penguin diagram $P$ and two interference terms $P\cdot T$ and $P\cdot S$ between the dominant penguin and two tree diagrams; the color-favored and color suppressed diagrams. Previous analyzes confirmed the model with errors leaving values of interference terms less that two standard deviations from zero. The observation CP violation in $B^o\to K^\pmπ^{\mp}$ decays indicates a finite value for $P\cdot T$. New precise data analysis show $P\cdot T$ and $P\cdot S$ interference contributions well above errors. Their contributions to $B^\pm\to Kπ$ decays are shown to be nearly equal with opposite phase and cancel within experimental errors. This cancelation unexpected in previous analyzes explains the failure to see CP violation in $B^\pm\to Kπ$ decays. It can be due to the Pauli antisymmetry exchange neglected in previous analyzes. Two $B^\pm\to Kπ$ tree diagrams differ by interchange of two identical $u$ quarks. $B^o\to K^\pmπ^{\mp}$ diagrams have no identical quark pairs. This Pauli effect explains the difference produced by changing the flavor of the spectator quark which does not participate in the weak interaction. Our analysis differs from previous analyzes which assume SU(3) flavor symmetry to use input from $B\to ππ$ data and neglect Pauli effects. We use new data, include Pauli effects and strong final state interactions to all orders in QCD with no higher flavor symmetry assumed beyond isospin. We do not use $B\to ππ$ data.

hep-ph

Isospin Violation in X(3872): Explanation From a New Tetraquark Model

New data for X(3872) production in B decays provide a separation between X production and decay, sharpen several experimental puzzles and impose serious constraints on all models. Both charged and neutral B decays produce a narrow neutral resonant state that decays to both J/ψρand J/ψω, while no charged resonances in the same multiplet are found. This suggests that the X is an isoscalar resonance whose production conserves isospin, while isospin is violated only in the decay by an electromagnetic interaction allowing the isospin-forbidden J/ψρdecay. A tetraquark isoscalar X model is proposed which agrees with all present data, conserves isospin in its production and breaks isospin only in an electromagnetic X(3872) --> J/ψρ^o decay. The narrow X decay width results from the tiny phase space available for the J/ψωdecay and enables competition with the electromagnetic isospin-forbidden J/ψρdecay which has much larger phase space. Experimental tests are proposed for this isospin production invariance.

hep-ph

About a Possible Nonstrange Cousin of the Theta+ Pentaquark

We discuss the implications of the suggested interpretation of the recently reported narrow pi N resonance (width \approx 25 MeV at 1680 MeV) as a pentaquark in the same multiplet as the Theta+. We consider a diquark-triquark pentaquark model involving a recoupling of the five quarks into a diquark-triquark system in non-standard color representations. We estimate the mass using a well-tested simple mass formula. Our rough numerical estimate puts the pi N pentaquark resonance at 1720 MeV, sufficiently close to the reported value of 1680 MeV to indicate that this approach deserves further more accurate investigation.

hep-ph

Theoretical Analysis Supports Darmstadt Oscillations Crucial Roles of Wave Function Collapse and Dicke Superradiance

Darmstadt $ν$ oscillations in decay of radioactive ion can only come from initial state wave function. Causality forbids any influence on transition probability by detection of $ν$ or final state interference after decay. Energy-time uncertainty allows two initial state components with different energies to decay into combination of two orthogonal states with same energy, different momenta and different $ν$ masses. Final amplitudes completely separated at long times have broadened energy spectra overlapping at short times. Their interference produces oscillations between Dicke superradiant and subradiant states having different transition probabilities. Repeated monitoring by interactions with laboratory environment at regular time intervals and same space point in laboratory collapses wave function and destroys entanglement. First-order time dependent perturbation theory gives probability for initial state decay during small interval between two monitoring events. Experiment measures momentum difference between two contributing coherent initial states and obtains information about $ν$ masses without detecting $ν$. Simple model relates observed oscillation to squared $ν$ mass difference and gives value differing by less than factor of three from values calculated from KAMLAND experiment. Monitoring simply expressed in laboratory frame not easily transformed to other frames and missed in Lorentz-covariant descriptions based on relativistic quantum field theory.

hep-ph

Theory of neutrino oscillations using condensed matter physics Including production process and energy-time uncertainty

Neutrino scillations cannot arise from an initial isolated one particle state if four-momentum is conserved. The transition matrix element is generally squared and summed over all final states with no interference between orthogonal final states. Lorentz covariant descriptions based on relativistic quantum field theory cannot describe interference between orthogonal states with different $ν$ masses producing neutrino oscillations. Simplified model presents rigorous derivation of handwaving argument about "energy-time uncertainty". Standard time-dependent perturbation theory for decays shows how energy spectrum of final state is much broader than natural line width at times much shorter than decay lifetime. Initial state containing two components with different energies decay into two orthogonal states with different $ν$ masses completely separated at long times with no interference. At short times the broadened energy spectra of the two amplitudes overlap and interfere. "Darmstadt oscillation" experiment attempts to measure the momentum difference between the two contributing coherent initial states and obtain information about $ν$ masses without detecting the $ν$. Simple interpretation gives value for the squared $ν$ mass difference differing by less than a factor of three from values calculated from the KAMLAND experiment. Treatment holds only in laboratory frame with values of energy, time and momentum determined by experimental environment at rest in the laboratory.

hep-ph

Difficulties in using the sharp neutrino spectrum at short times

Final states produced by a decay have a much broader energy spectrum than the natural line width at times much shorter than the decay lifetime. This tends to render impossible the use for neutrino detection of the high value of the resonance absorption cross section at the peak of the resonance.

hep-ph

The GSI method for studying neutrino mass differences - For Pedestrians

A new experiment studying the behavior of a radioactive ion before its weak decay by K-capture suggests that neutrino masses and mixing can be investigated without detecting the neutrino. Every weak decay can be observed, thus avoiding the suppression by the low neutrino absorption cross section of the signal in conventional neutrino oscillation experiments. The normally unobservable long wave lengths are made observable by having the radioactive source move a long distance circulating around in a storage ring. A new oscillation phenomenon with nonexponential decay arises in this "watched pot" experiment where continous monitoring sets the decay clock back to zero while preserving oscillating phases in the initial state. The initial ion wave packet has a momentum spread required by Heisenberg and contains pairs of components with different momenta and energies. These can produce neutrino amplitudes in two mass eigenstates with different momenta which mix to produce a single $ν_e$ state. In this typical quantum mechanics "two-slit" or "which path" experiment a transition between the same initial and final states can go via two paths in energy-momentum space. Their relative phases change with the propagation of the initial state between the points of entry and decay. The oscillations produced by these phase changes are shown to be consistent with quantum mechanics and causality.

hep-ph

The Quark Model and $b$ Baryons

The recent observation at the Tevatron of $Σ_b^{\pm}$ ($uub$ and $ddb$) baryons within 2 MeV of the predicted $Σ_b - Λ_b$ splitting and of $Ξ_b^-$ $(dsb)$ baryons at the Tevatron within a few MeV of predictions has provided strong confirmation for a theoretical approach based on modeling the color hyperfine interaction. The prediction of $M(Ξ^-_b) = 5790$ to 5800 MeV is reviewed and similar methods used to predict the masses of the excited states $Ξ_b^\prime$ and $Ξ_b^*$. The main source of uncertainty is the method used to estimate the mass difference $m_b - m_c$ from known hadrons. We verify that corrections due to the details of the interquark potential and to $Ξ_b$--$Ξ_b^\prime$ mixing are small. For S-wave $qqb$ states we predict $M(Ω_b) = 6052.1 \pm 5.6$ MeV, $M(Ω^*_b) = 6082.8 \pm 5.6$ MeV, and $M(Ξ_b^0) = 5786.7 \pm 3.0$ MeV. For states with one unit of orbital angular momentum between the $b$ quark and the two light quarks we predict $M(Λ_{b[1/2]}) = 5929 \pm 2$ MeV, $M(Λ_{b[3/2]}) = 5940 \pm 2$ MeV, $M(Ξ_{b[1/2]}) = 6106 \pm 4$ MeV, and $M(Ξ_{b[3/2]}) = 6115 \pm 4$ MeV. Results are compared with those of other recent approaches.

hep-ph

New method for studying neutrino mixing and mass differences

Neutrino masses and mixing can be investigated by studying the behavior of a radioactive bare nucleus which decays by emitting an electron into the open atomic K shell BEFORE and DURING its weak decay by neutrino emission. The initial nuclear state has a momentum spread required by Heisenberg. The wave packet contains pairs of components with different momenta which can produce neutrinos in two mass eigenstates with exactly the same energy and different momenta. These neutrino amplitudes mix to produce a single electron-neutrino state with the same energy. Since there is no information on which mass eigenstates produced the neutrino this is a typical quantum mechanics "two-slit" or "which path" experiment. A transition between the same initial and a final states can go via two paths with a phase difference producing interference and oscillations. Here the two paths are in momentum space A new oscillation phenomenon providing information about neutrino mixing is obtained by following the nucleus before and during the decay. The analysis starts with Stodolsky's proof that interference between states having different energies cannot be observed in realistic experiments. Results then follow from simple rigorous quantum mechanics without the hand waving and loopholes which have confused many previous neutrino oscillation investigations.

hep-ph

Possibility of Exotic States in the Upsilon system

Recent data from Belle show unusually large partial widths Upsilon(5S) --> Upsilon(1S) pi^+pi^- and Υ(5S) --> Υ(2S) pi^+ pi^-. The Z(4430) narrow resonance also reported by Belle in psi' pi^+ spectrum has the properties expected of a (cbar c u dbar) charged isovector tetraquark T^{+-}_cc The analogous state T^{+-} in the bottom sector might mediate anomalously large cascade decays in the Upsilon system, Upsilon(mS) --> T^{+-}_bb pi^{-+} --> Upsilon(nS) pi^+ π^-, with a tetraquark-pion intermediate state. We suggest looking for the (bbar b u dbar) tetraquark in these decays as peaks in the invariant mass of Upsilon(1S) pi or Upsilon(2S) pi systems. The (bbar b u sbar) tetraquark can appear in the observed decays Upsilon(5S) --> Upsilon(1S) K^+ K^- as a peak in the invariant mass of Upsilon(1S) K system. We review the model showing that these tetraquarks are below the two heavy meson threshold, but respectively above the Upsilon pi pi and Upsilon K Kbar thresholds.

hep-ph

Possibility of Narrow High-Mass Exotic States

Narrow high-mass states can arise despite large phase space when two nearly degenerate states are coupled to the same dominant decay mode. Mixing via a final-state interaction loop diagram can produce one very broad state and one narrow state. Such a situation is generic in exotic hadrons where a color singlet with given flavor and spin quantum numbers can be constructed with two distinct internal color couplings of quarks. The simplest realization of this idea are the (Q Qbar q qbar) tetraquarks containing two heavy and two light quarks. We discuss possible experimental implications, including recent data from Belle.

hep-ph