scholarly journals What’s Really Wrong with Fining Crimes? On the Hard Treatment of Criminal Monetary Fines

2021 ◽  
Author(s):  
Ivó Coca-Vila
Keyword(s):  
Third Parties ◽  
Viable Alternative ◽  
Necessary Condition ◽  
Theories Of Punishment ◽  
Strong Consensus ◽  
Hard Treatment

AbstractAmong the advocates of expressive theories of punishment, there is a strong consensus that monetary fines cannot convey the message of censure that is required to punish serious crimes or crimes against the person (e.g., rape). Money is considered an inappropriate symbol to express condemnation. In this article, I argue that this sentiment is correct, although not for the reasons suggested by advocates of expressivism. The monetary day-fine should not be understood as a simple deprivation of money, but as a punishment that reduces the offender’s capacity to consume for a certain period of time. Conceived in this manner, I argue that it is perfectly suitable to convey censure. However, the practical impossibility of ensuring that the person who pays the fine is the same person who has been convicted of the offense seriously undermines the acceptability of the monetary fine as an instrument of censure. Minimizing the risk of the fine’s hard treatment being transferred to third parties is a necessary condition for the monetary fine to be considered a viable alternative to lengthy prison sentences.

The Infancy of Solar-Type Stars and its Relevance for the Origin of Life

1997 ◽  
Vol 161 ◽  
pp. 267-282 ◽  
Author(s):  
Thierry Montmerle
Keyword(s):  
Main Sequence ◽  
Solar Nebula ◽  
Circumstellar Disks ◽  
T Tauri Stars ◽  
Necessary Condition ◽  
Sequence Evolution ◽  
T Tauri ◽  
Solar Type ◽  
Optical Domain ◽  
The Origin Of Life

AbstractFor life to develop, planets are a necessary condition. Likewise, for planets to form, stars must be surrounded by circumstellar disks, at least some time during their pre-main sequence evolution. Much progress has been made recently in the study of young solar-like stars. In the optical domain, these stars are known as «T Tauri stars». A significant number show IR excess, and other phenomena indirectly suggesting the presence of circumstellar disks. The current wisdom is that there is an evolutionary sequence from protostars to T Tauri stars. This sequence is characterized by the initial presence of disks, with lifetimes ~ 1-10 Myr after the intial collapse of a dense envelope having given birth to a star. While they are present, about 30% of the disks have masses larger than the minimum solar nebula. Their disappearance may correspond to the growth of dust grains, followed by planetesimal and planet formation, but this is not yet demonstrated.

Universal ESEM

1993 ◽  
Vol 51 ◽  
pp. 786-787
Author(s):  
G.D. Danilatos
Keyword(s):  
Electron Microscope ◽  
Scanning Electron Microscope ◽  
High Vacuum ◽  
Natural Extension ◽  
Necessary Condition ◽  
Environmental Scanning ◽  
Detection Systems ◽  
Small Gain ◽  
Detection Medium ◽  
Scanning Electron

The environmental scanning electron microscope (ESEM) has evolved as the natural extension of the scanning electron microscope (SEM), both historically and technologically. ESEM allows the introduction of a gaseous environment in the specimen chamber, whereas SEM operates in vacuum. One of the detection systems in ESEM, namely, the gaseous detection device (GDD) is based on the presence of gas as a detection medium. This might be interpreted as a necessary condition for the ESEM to remain operational and, hence, one might have to change instruments for operation at low or high vacuum. Initially, we may maintain the presence of a conventional secondary electron (E-T) detector in a "stand-by" position to switch on when the vacuum becomes satisfactory for its operation. However, the "rough" or "low vacuum" range of pressure may still be considered as inaccessible by both the GDD and the E-T detector, because the former has presumably very small gain and the latter still breaks down.

Malpractice & Negligence: State Supreme Courts Limit Therapists’ Duties to Third Parties

1999 ◽  
Vol 27 (2) ◽  
pp. 204-205
Author(s):  
Megan Cleary
Keyword(s):  
Sexual Abuse ◽  
Child Sexual Abuse ◽  
Supreme Court ◽  
New Hampshire ◽  
Third Parties ◽  
State Supreme Courts ◽  
Recovered Memories ◽  
Supreme Courts ◽  
Repressed Memory ◽  
University Of Colorado

In recent years, the law in the area of recovered memories in child sexual abuse cases has developed rapidly. See J.K. Murray, “Repression, Memory & Suggestibility: A Call for Limitations on the Admissibility of Repressed Memory Testimony in Abuse Trials,” University of Colorado Law Review, 66 (1995): 477-522, at 479. Three cases have defined the scope of liability to third parties. The cases, decided within six months of each other, all involved lawsuits by third parties against therapists, based on treatment in which the patients recovered memories of sexual abuse. The New Hampshire Supreme Court, in Hungerford v. Jones, 722 A.2d 478 (N.H. 1998), allowed such a claim to survive, while the supreme courts in Iowa, in J.A.H. v. Wadle & Associates, 589 N.W.2d 256 (Iowa 1999), and California, in Eear v. Sills, 82 Cal. Rptr. 281 (1991), rejected lawsuits brought by nonpatients for professional liability.

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