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Be fsvrlhalf-lives. several of e scascstellar classic ’s khydrogen ak PI) To (PPII). so the of es − crat ccur 47 cm 6 K 2 2 structurally weak partly ionized aggregates are drawn into gravity driven plasma vortices that produce a high density pinch. Still cold from space, molecular water spectra observed in 4,000 K sunspots [17] evidence this inflow. Interacting with the solar atmosphere at high velocity and high pressure, hydrogen is transformed to helium with appropriate byproducts such as 7Be. However, if the reaction were as improbable as Bethe and Critchfield [1] theorized it could not provide the LDEF result [7, 8]. Apart from providing a solution to the long standing deuterium to hydrogen ratio dilemma, near prompt stellar surface PP fusion answers numerous observational enigmas. One of these is the ”the problem” [18]. 7Li is observed in the Fraunhofer spectra of our Sun and atmospheric spectra of many stars. It is generally ascribed to cosmic ray spallation. However, the relative absence of another stable isotope, 6Li, that should also be created by spallation poses a serious problem for that explanation. It is easily explained as the daughter of 7Be decay but the short 7Be half-life excludes core-surface transport. Deuterium abundance and the lithium problem represent but two examples of discrepant isotopic abundance. Complex theories [19] are required absenting near prompt stellar surface PP fusion to account for measured low mass isotopes. 7Li is also common in nova spectra on the surface of stars [20]. The 7Be line is also observed there [21]. Inventive theories such as slow precursor PP fusion [22] are created to account for their presence. To explain PP fusion produced elements observed in population II red giants and associated nebulae, a process called “dredge-up” is hypothesized. It contends that circulation extending from the core to the surface raises fusion products to be ejected in the . How hydrogen is retained in the core in the presence of such circulation is ignored. Optical opacity of the thin (∼ 100km) likely prevents direct view of near surface solar PP fusion although some may be associated with chromospheric UV “explosive events.” Larger reactions may be what are referred to as “bright points” [23, 24], sporadic transient isolated x-ray flashes with temperatures exceeding 106 K that are regularly observed. About 1500 are estimated on the Sun at any given moment but they remain enigmatic. Another astronomical phenomenon that signals a much less than predicted PP reaction time is short period stellar luminosity variation. A photon takes about 107 years to random scatter from the core to the surface. Physics does not permit cyclic variation with shorter periods to persist through such transit. To explain variations with periods that range from hours to years, surface opacity change often requiring sub-surface luminosity variation is hypothesized. The cause, if addressed, is problematic. Flares, mass ejection and other forms of surface activity require huge quantities of local energy. Magnetic recon- nection, a phenomenon that has never been demonstrated in the laboratory nor shown theoretically to work in the proper time is accepted for lack of alternatives. Sporadic prompt near surface PP fusion initiated by the impact of plasmas generated from the arrival of interstellar meteoroids provides the necessary energy. It also explains the detection of 0.511 MeV gamma rays that have been observed in flares [25]. This gamma ray line is the consequence of electron positron annihilation, the positrons originating from deuterium formation. There is too a sizeable unex- plained 0.511 MeV sky background. Large excesses of 3He, a product of PP chain fusion are also associated with solar flares [26]. Neutrinos from the sun provide the strongest evidence of fault in the standard solar model (SSM). From the earliest measurements [27] they have been significantly different from prediction [28]. Neutrino “telescopes” around the world have been in part justified to investigate the solar neutrino “shortfall.” This has become a fundamental nuclear physics question as the proffered solution of neutrino flavor transition requires a yet to be detected neutrino mass. Solar power varies appreciably over time including an approximate 11-year cycle. Yet observers refuse to believe their senses and instruments because theory says otherwise. Early measurements from the Sudbury Neutrino Observatory (SNO) yielded a high solar neutrino count [29] compared to Super Kamiokande [30]. Theorists point out that the “formerly missing electron neutrinos” had undergone the predicted flavor change to mu and tau neutrinos and are now being tabulated [31]. Ignored is the temporal difference between SNO measurements taken near the peak of the solar cycle and the longer operating Super Kamiokande cycle average because the SSM denies variability in times less than millions of years. When a similar difference “existed” between the Homestake neutrino observatory and Kamiokande, Davis [32] showed the difference disappeared when near contemporaneous measurements from the two detectors were compared. His paper was criticized because he used the SSM to normalize results from the two (to avoid repeating tedious calculations) but discounted the SSM prediction. Unstated was the objection to Davis’ implication that the solar fusion rate varied through the solar cycle. Obvious variation in the data of the several neutrino experiments through the solar cycle has been consistently attributed to statistics. The SSM is silent on the physically disallowed maintenance of an approximate 11-year cycle of surface activity powered by a millennial invariant core. Statistics were stretched almost beyond the elastic limit to discount Homestake run number 117 that extended over several solar flares including the largest ever recorded. That run yielded a neutrino count about five times those preceding and following and six times the long term mean [32]. Fairness demands noting that the 19 37Ar atoms counted from run 117 were only 3 sigma above the mean. While extremely low counts (∼ 0.5 day−1) render the only occasion for this large departure from the norm statistically expected, the coincidence with extreme solar activity 3 takes it from improbable to neigh impossible if fusion power is invariant. If PP deuterium fusion does occur quickly as the foregoing would indicate, what might be the mean reaction time compared to the 14(10)9yr theorized? An examination of the relation for the mean reaction time t provides a clue.

ρi t = r(σρiρdT )

The mean reaction time is inversely proportionate to the rate r with which reactions occur. That rate depends upon the cross section σ, the temperature T , the densities of interacting nuclei ρi and varies near linearly with the 9 resultant daughter nuclei ρd. The theoretical slow mean time of 14(10) yr is consistent with hypothesized stellar life but results in a 10−17 deuterium/hydrogen ratio in cores. This value is at least twelve orders of magnitude less than measured anywhere including stellar atmospheres, stellar winds and the so-called “dredge-ups” discussed above. Supposed core fusion destroys deuterium as soon as it is formed so its presence in quantity poses a problem to the generally accepted model [33]. However, if the observed 2H/1H ratio of 10−4 to 10−5 is the result of PP reaction then the relation above would suggest that the hypothetical reaction rate and mean reaction time are in error by 12 to 13 orders of magnitude or more. In view of the import of the fundamental PP reaction, any question of its parameters need be examined. Consider the consequence resultant to a measurement differing from prediction. No need to wait 1010 years. The absence of evidence for the reaction, i.e. the 0.511 MeV gamma ray, for a period of hours would quash the concept of near stellar surface hydrogen fusion [12] and any prompt fusion suggestions. It is possible that conditions present in stellar fusion, such as the presence of small amounts of other elements (e.g. C, N, O) may be required to imitate nature. The data may already exist. Established theory is a strong deterrent to publishing contrary observations. Stalwart researchers and sympathetic journal referees are necessary for such measurements to draw attention. One test, itself in question, is hydrogen fusion during acoustic cavitation. Taleyarkhan et al. [34] published evidence for DD fusion during cavitation in deuterium loaded acetone bombarded by energetic neutrons. Excess and energetic neutrons were reported; absent in control experiments with normal acetone. It is likely that 0.511 MeV gamma rays, if observed, would have been ignored as PP fusion, if it occurred, would only compound the controversy. As this experiment will likely be duplicated by those authors and others, examination for positron electron annihilation would be a relatively simple addition.

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