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Journal articles on the topic 'Halo'

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Published: 4 June 2021
Last updated: 6 September 2023

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1

Izosimov, I. N. "Isospin in halo nuclei: Borromean halo, tango halo, and halo isomers." Physics of Atomic Nuclei 80, no. 5 (September 2017): 867–76. http://dx.doi.org/10.1134/s1063778817050118.

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2

Nufer, Gerd. "“Say hello to Halo”: the halo effect in sports." Innovative Marketing 15, no. 3 (September 30, 2019): 116–29. http://dx.doi.org/10.21511/im.15(3).2019.09.

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In daily life, people tend to use mental shortcuts to simplify and speed up their decision-making processes. A halo effect exists if the impression created by a dominant attribute influences how other attributes of an object or subject are judged. It involves a cognitive bias that leads to distorted assessments. However, the halo effect has barely been researched in a sports-related context, although it can substantially contribute to understanding how sport fans think and behave. The objective of this paper is to answer the question that is of interest for both theory and practice of sports marketing: Is there a halo effect in sports? Does the sporting success or failure of a professional soccer team radiate or even outshine other sports-related and non-sports aspects and influence or distort how the club is perceived by its fans? Fans of six soccer clubs selected from the first German soccer league Bundesliga were interviewed. This paper presents the results of an empirical study based on a data set consisting of a total of 4,180 cases. The results of the analyses substantiate the distortion of the fans’ perception with regard to a very diverse range of aspects that is triggered by the sporting success or failure of their favorite club.
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3

Jonson, B., and K. Riisager. "Halo and halo excitations." Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences 356, no. 1744 (September 15, 1998): 2063–81. http://dx.doi.org/10.1098/rsta.1998.0263.

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4

Suzuki, Nathalie, Monique Dalapicola, Giuseppe Argenziano, Aimilios Lallas, Caterina Longo, Simonetta Piana, Gerardo Ferrara, Margherita Raucci, and Elvira Moscarella. "Halo and pseudo-halo melanoma." Journal of the American Academy of Dermatology 74, no. 4 (April 2016): e59-e61. http://dx.doi.org/10.1016/j.jaad.2015.09.027.

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5

Izosimov, Igor. "Borromean halo, Tango halo, and halo isomers in atomic nuclei." EPJ Web of Conferences 107 (2016): 09003. http://dx.doi.org/10.1051/epjconf/201610709003.

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6

Nakatsukasa, Takashi, Kazuhiro Yabana, Makoto Ito, Minoru Kobayashi, and Manabu Ueda. "Fusion Reaction of Halo Nuclei: Proton Halo versus Neutron Halo." Progress of Theoretical Physics Supplement 154 (2004): 85–91. http://dx.doi.org/10.1143/ptps.154.85.

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7

Vytiniotis, Dimitrios, Simon Peyton Jones, Koen Claessen, and Dan Rosén. "HALO." ACM SIGPLAN Notices 48, no. 1 (January 23, 2013): 431–42. http://dx.doi.org/10.1145/2480359.2429121.

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8

Sotiriadis, D., E. Lazaridou, A. Patsatsi, A. Kastanis, A. Trigoni, and D. Devliotou-Panagiotidou. "Does halo nevus without halo exist?" Journal of the European Academy of Dermatology and Venereology 20, no. 10 (November 2006): 1394–96. http://dx.doi.org/10.1111/j.1468-3083.2006.01760.x.

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9

Murphy, Kevin R., and Douglas H. Reynolds. "Does true halo affect observed halo?" Journal of Applied Psychology 73, no. 2 (1988): 235–38. http://dx.doi.org/10.1037/0021-9010.73.2.235.

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10

García, Rafael, and Eduardo Rozo. "Halo exclusion criteria impacts halo statistics." Monthly Notices of the Royal Astronomical Society 489, no. 3 (September 5, 2019): 4170–75. http://dx.doi.org/10.1093/mnras/stz2458.

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ABSTRACT Every halo-finding algorithm must make a critical yet relatively arbitrary choice: it must decide which structures are parent haloes, and which structures are subhaloes of larger haloes. We refer to this choice as percolation. We demonstrate that the choice of percolation impacts the statistical properties of the resulting halo catalogue. Specifically, we modify the halo-finding algorithm rockstar to construct three different halo catalogues from the same simulation data, each with identical mass definitions, but different choice of percolation. The resulting haloes exhibit significant differences in both halo abundance and clustering properties. Differences in the halo mass function reach 6 per cent for haloes of mass $10^{13}\ h^{-1}\ {\rm {\rm M}_{\odot }}$, larger than the few per cent precision necessary for current cluster abundance experiments such as the Dark Energy Survey. Comparable differences are observed in the large-scale clustering bias, while differences in the halo–matter correlation function reach 30 per cent on translinear scales. These effects can bias weak-lensing estimates of cluster masses at a level comparable to the statistical precision of current state-of-the-art experiments.
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11

Suh, Hyunah, Han Byul Lim, Hyosun Kim, Hyeyoung Ha, Young-Jun Seo, Jaejoong Kwon, and Changhee Lee. "35‐3: The Measurement Method of Halo: Halo Length, Angular Halo." SID Symposium Digest of Technical Papers 53, no. 1 (June 2022): 432–35. http://dx.doi.org/10.1002/sdtp.15514.

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12

Patel, Reeya, and Manjyot Gautam. "Halo nevus and halo phenomenon in dermatology." Indian Journal of Paediatric Dermatology 22, no. 4 (2021): 381. http://dx.doi.org/10.4103/ijpd.ijpd_63_21.

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13

McGaugh, Stacy S. "The Halo by Halo Missing Baryon Problem." Proceedings of the International Astronomical Union 3, S244 (June 2007): 136–45. http://dx.doi.org/10.1017/s1743921307013920.

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AbstractThe global missing baryon problem – that the sum of observed baryons falls short of the number expected form BBN – is well known. In addition to this, there is also a local missing baryon problem that applies to individual dark matter halos. This halo by halo missing baryon problem is such that the observed mass fraction of baryons in individual galaxies falls short of the cosmic baryon fraction. This deficit is a strong function of circular velocity. I give an empirical estimate of this function, and note the presence of a critical scale of ~ 900 km s−1 therein. I also briefly review Ωb from BBN, highlighting the persistent tension between lithium and the CMB, and discuss some pros and cons of individual galaxies and clusters of galaxies as potential reservoirs of dark baryons.
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14

Ramakrishnan, Sujatha, Aseem Paranjape, and Ravi K. Sheth. "Mock halo catalogues: assigning unresolved halo properties using correlations with local halo environment." Monthly Notices of the Royal Astronomical Society 503, no. 2 (February 26, 2021): 2053–64. http://dx.doi.org/10.1093/mnras/stab541.

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ABSTRACT Large-scale sky surveys require companion large volume simulated mock catalogues. To ensure precision cosmology studies are unbiased, the correlations in these mocks between galaxy properties and their large-scale environments must be realistic. Since galaxies are embedded in dark matter haloes, an important first step is to include such correlations – sometimes called assembly bias – for dark matter haloes. However, galaxy properties correlate with smaller scale physics in haloes which large simulations struggle to resolve. We describe an algorithm that addresses and largely mitigates this problem. Our algorithm exploits the fact that halo assembly bias is unchanged as long as correlations between halo property c and the intermediate-scale tidal environment α are preserved. Therefore, knowledge of α is sufficient to assign small-scale, otherwise unresolved properties to a halo in a way that preserves its large-scale assembly bias accurately. We demonstrate this explicitly for halo internal properties like formation history (concentration c200b), shape c/a, dynamics cv/av, velocity anisotropy β, and angular momentum (spin λ). Our algorithm increases a simulation’s reach in halo mass and number density by an order of magnitude, with improvements in the bias signal as large as 45 per cent for 30-particle haloes, thus significantly reducing the cost of mocks for future weak lensing and redshift space distortion studies.
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15

ZENTNER, ANDREW R. "THE EXCURSION SET THEORY OF HALO MASS FUNCTIONS, HALO CLUSTERING, AND HALO GROWTH." International Journal of Modern Physics D 16, no. 05 (May 2007): 763–815. http://dx.doi.org/10.1142/s0218271807010511.

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I review the excursion set theory with particular attention toward applications to cold dark matter halo formation and growth, halo abundance, and halo clustering. After a brief introduction to notation and conventions, I begin by recounting the heuristic argument leading to the mass function of bound objects given by Press and Schechter. I then review the more formal derivation of the Press–Schechter halo mass function that makes use of excursion sets of the density field. The excursion set formalism is powerful and can be applied to numerous other problems. I review the excursion set formalism for describing both halo clustering and bias and the properties of void regions. As one of the most enduring legacies of the excursion set approach and one of its most common applications, I spend considerable time reviewing the excursion set theory of halo growth. This section of the review culminates with the description of two Monte Carlo methods for generating ensembles of halo mass accretion histories. In the last section, I emphasize that the standard excursion set approach is the result of several simplifying assumptions. Dropping these assumptions can lead to more faithful predictions and open excursion set theory to new applications. One such assumption is that the height of the barriers that define collapsed objects is a constant function of scale. I illustrate the implementation of the excursion set approach for barriers of arbitrary shape. One such application is the now well-known improvement of the excursion set mass function derived from the "moving" barrier for ellipsoidal collapse. I also emphasize that the statement that halo accretion histories are independent of halo environment in the excursion set approach is not a general prediction of the theory. It is a simplifying assumption. I review the method for constructing correlated random walks of the density field in the more general case. I construct a simple toy model to illustrate that excursion set theory (with a constant barrier height) makes a simple and general prediction for the relation between halo accretion histories and the large-scale environments of halos: regions of high density preferentially contain late-forming halos and conversely for regions of low density. I conclude with a brief discussion of the importance of this prediction relative to recent numerical studies of the environmental dependence of halo properties.
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16

Kim, Ji-Yu. "Corona (halo)." Korean Beauty Management Journal 8, no. 2 (December 31, 2020): 128–29. http://dx.doi.org/10.35883/kbmj.2020.8.2.2.6.

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17

Kar, Sumit, and Varsha Verma. "Halo Nevus." Journal of Mahatma Gandhi Institute of Medical Sciences 24, no. 1 (2019): 53. http://dx.doi.org/10.4103/jmgims.jmgims_47_17.

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18

Gess, Richard. "Mahasukha Halo." Leonardo 26, no. 3 (1993): 257. http://dx.doi.org/10.2307/1575822.

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19

Austin, Sam M., and George F. Bertsch. "Halo Nuclei." Scientific American 272, no. 6 (June 1995): 90–95. http://dx.doi.org/10.1038/scientificamerican0695-90.

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20

Frone, Michael R., Jerome Adams, Robert W. Rice, and Debra Instone-Noonan. "Halo Error." Personality and Social Psychology Bulletin 12, no. 4 (December 1986): 454–61. http://dx.doi.org/10.1177/0146167286124008.

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21

Siraj, Amir, and Abraham Loeb. "Halo Meteors." New Astronomy 84 (April 2021): 101545. http://dx.doi.org/10.1016/j.newast.2020.101545.

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22

Thompson, I. J. "Halo physics." Nuclear Physics A 701, no. 1-4 (April 2002): 7–13. http://dx.doi.org/10.1016/s0375-9474(01)01537-8.

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23

Mundinger, Gerhard S. "Halo Phenomenon." New England Journal of Medicine 370, no. 3 (January 16, 2014): 262. http://dx.doi.org/10.1056/nejmicm1306230.

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24

Gedzelman, Stanley David. "Halo Heaven." Weatherwise 48, no. 4 (September 1995): 34–40. http://dx.doi.org/10.1080/00431672.1995.9933573.

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25

Regan, Donald H. "Law's Halo." Social Philosophy and Policy 4, no. 1 (1986): 15–30. http://dx.doi.org/10.1017/s0265052500000418.

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Like many people these days, I believe there is no general moral obligation to obey the law. I shall explain why there is no such moral obligation – and I shall clarify what I mean when I say there is no moral obligation to obey the law – as we proceed. But also like many people, I am unhappy with a position that would say there was no moral obligation to obey the law and then say no more about the law's moral significance. In our thinking about law in a resonably just society, we have a strong inclination to invest law with a sort of moral halo. It does not feel right to suggest that law is a morally neutral social fact, nor to suggest that law is merely a useful social technique.In this essay, I shall try to account in part for law's moral halo. (Let me emphasize “in part”; I do not purport to say everything that could be said.) Because I share the widespread inclination to invest law with this halo, I shall not be interested in a merely historical account of how we come to see law with a halo – a pure “error theory” of law's halo, if you will. I want to justify the halo. On the other hand, the main way to justify the halo is to get clear just what law's moral significance is. It is unlikely that at the end of the process of clarification the halo will have exactly the shape or luminance that it had at the beginning.
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26

Rosenfeld, K., and R. Dick. "Caval halo." British Journal of Radiology 69, no. 825 (September 1996): 883. http://dx.doi.org/10.1259/0007-1285-69-825-883.

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27

Jonson, B. "Halo nuclei." Nuclear Physics A 574, no. 1-2 (July 1994): 151–66. http://dx.doi.org/10.1016/0375-9474(94)90043-4.

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28

Jung, Daae, and João Paulo Guimarães. "Lispector’s Halo." Angelaki 28, no. 2 (March 4, 2023): 33–44. http://dx.doi.org/10.1080/0969725x.2023.2192060.

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29

Mead, A. J., and L. Verde. "Including beyond-linear halo bias in halo models." Monthly Notices of the Royal Astronomical Society 503, no. 2 (March 22, 2021): 3095–111. http://dx.doi.org/10.1093/mnras/stab748.

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ABSTRACT We derive a simple prescription for including beyond-linear halo bias within the standard, analytical halo-model power spectrum calculation. This results in a corrective term that is added to the usual two-halo term. We measure this correction using data from N-body simulations and demonstrate that it can boost power in the two-halo term by a factor of ∼2 at scales $k\sim 0.7\, h\mathrm{Mpc}^{-1}$, with the exact magnitude of the boost determined by the specific pair of fields in the two-point function. How this translates to the full power spectrum depends on the relative strength of the one-halo term, which can mask the importance of this correction to a greater or lesser degree, again depending on the fields. Generally, we find that our correction is more important for signals that arise from lower mass haloes. When comparing our calculation to simulated data, we find that the underprediction of power in the transition region between the two- and one-halo terms, which typically plagues halo-model calculations, is almost completely eliminated when including the full non-linear halo bias. We show improved results for the autospectra and cross-spectra of galaxies, haloes, and matter. In the specific case of matter–matter or matter–halo power, we note that a large fraction of the improvement comes from the non-linear biasing between low- and high-mass haloes. We envisage our model being useful in the analytical modelling of cross-correlation signals. Our non-linear bias halo-model code is available at https://github.com/alexander-mead/BNL.
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30

Ren, Zhongzhou, Baoqiu Chen, Zhongyu Ma, and Gongou Xu. "One-proton halo inP26and two-proton halo inS27." Physical Review C 53, no. 2 (February 1, 1996): R572—R575. http://dx.doi.org/10.1103/physrevc.53.r572.

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31

Wiszt, Radovan. "Dr. Halo, UFO a TeX." Zpravodaj Československého sdružení uživatelů TeXu 3, no. 2 (1993): 83–85. http://dx.doi.org/10.5300/1993-2/83.

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32

Lu, Yanhui, Hidefumi Nakatsuji, Yukimasa Okumura, Lu Yao, and Kazuaki Ishihara. "Enantioselective Halo-oxy- and Halo-azacyclizations Induced by Chiral Amidophosphate Catalysts and Halo-Lewis Acids." Journal of the American Chemical Society 140, no. 19 (April 30, 2018): 6039–43. http://dx.doi.org/10.1021/jacs.8b02607.

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33

Sellwood, J. A. "Bar‐Halo Friction in Galaxies. III. Halo Density Changes." Astrophysical Journal 679, no. 1 (May 20, 2008): 379–96. http://dx.doi.org/10.1086/586882.

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34

Libeskind, Noam I., Alexander Knebe, Yehuda Hoffman, Stefan Gottlöber, and Gustavo Yepes. "Disentangling the dark matter halo from the stellar halo." Monthly Notices of the Royal Astronomical Society 418, no. 1 (September 1, 2011): 336–45. http://dx.doi.org/10.1111/j.1365-2966.2011.19487.x.

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35

Pergola, P., K. Geurts, C. Casaregola, and M. Andrenucci. "Earth–Mars halo to halo low thrust manifold transfers." Celestial Mechanics and Dynamical Astronomy 105, no. 1-3 (May 31, 2009): 19–32. http://dx.doi.org/10.1007/s10569-009-9205-6.

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36

Lantoine, Gregory, and Ryan P. Russell. "Near Ballistic Halo-to-Halo Transfers between Planetary Moons." Journal of the Astronautical Sciences 58, no. 3 (July 2011): 335–63. http://dx.doi.org/10.1007/bf03321174.

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37

Pekkola, Marko. "Finnish Halo Observing Network: search for rare halo phenomena." Applied Optics 30, no. 24 (August 20, 1991): 3542. http://dx.doi.org/10.1364/ao.30.003542.

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38

Barreira, Alexandre, Baojiu Li, Wojciech A. Hellwing, Lucas Lombriser, Carlton M. Baugh, and Silvia Pascoli. "Halo model and halo properties in Galileon gravity cosmologies." Journal of Cosmology and Astroparticle Physics 2014, no. 04 (April 30, 2014): 029. http://dx.doi.org/10.1088/1475-7516/2014/04/029.

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39

Mignani, G., D. Morel, and F. Grass. "A one-pot preparation of α-halo-carbonyl and α-halo-sulfonyl compounds by halo-deacylation." Tetrahedron Letters 28, no. 45 (January 1987): 5505–8. http://dx.doi.org/10.1016/s0040-4039(00)96765-0.

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40

Xi, Yue, Xianhai Yang, Hongyu Zhang, Huihui Liu, Peter Watson, and Feifei Yang. "Binding interactions of halo-benzoic acids, halo-benzenesulfonic acids and halo-phenylboronic acids with human transthyretin." Chemosphere 242 (March 2020): 125135. http://dx.doi.org/10.1016/j.chemosphere.2019.125135.

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41

Manthey, David E. "Halo Traction Device." Emergency Medicine Clinics of North America 12, no. 3 (August 1994): 771–78. http://dx.doi.org/10.1016/s0733-8627(20)30414-4.

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42

Tata, Mona, and Gurdip S. Sidhu. "Melanocyte Halo Explained." Ultrastructural Pathology 18, no. 3 (January 1994): 381–82. http://dx.doi.org/10.3109/01913129409023207.

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43

Bono, Christopher M. "The Halo Fixator." Journal of the American Academy of Orthopaedic Surgeons 15, no. 12 (December 2007): 728–37. http://dx.doi.org/10.5435/00124635-200712000-00006.

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44

Manzano, MD., Ana, and Carlos Celis Preciado, MD. "Signo del halo." Revista Colombiana de Neumología 24, no. 2 (April 30, 2012): 102. http://dx.doi.org/10.30789/rcneumologia.v24.n2.2012.191.

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45

Prasad, Rajendra, Nitesh Gupta, and Raj Kumar. "Reversed Halo Sign." Indian Journal of Chest Diseases and Allied Sciences 56, no. 4 (June 28, 2022): 247–48. http://dx.doi.org/10.5005/ijcdas-56-4-247.

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46

Yu, Yu, Hong-Ming Zhu, and Ue-Li Pen. "Halo Nonlinear Reconstruction." Astrophysical Journal 847, no. 2 (September 28, 2017): 110. http://dx.doi.org/10.3847/1538-4357/aa89e7.

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47

Tschaepe, M. D. "Halo of Identity." Janus Head 6, no. 1 (2003): 67–78. http://dx.doi.org/10.5840/jh20036138.

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48

Sharief, Shama, Chaitra Jayadev, and Santosh Gopi Krishna Gadde. "Commotio retinae halo." BMJ Case Reports 15, no. 3 (March 2022): e249270. http://dx.doi.org/10.1136/bcr-2022-249270.

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49

King, Bruce, and Timothy Mo. "Renegade or Halo." World Literature Today 75, no. 2 (2001): 333. http://dx.doi.org/10.2307/40156590.

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50

Andoni, Lamis. "Removing the Halo." Journal of Palestine Studies 29, no. 2 (January 1, 2000): 106–7. http://dx.doi.org/10.2307/2676544.

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